Exchange-Rate Dark Matter
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Mr. Martin D Evans
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Author’s E-Mail Address: mevans@imf.org

Dark matter accounts for 83 percent of the matter in the universe and plays a central role in cosmology modeling. This paper argues that an analogous form of dark matter plays a similarly important role in international macroeconomics. Exchange-rate dark matter is invisible, but its existence can be inferred from observations on real exchange rates and interest rates. I first show that dark matter is the dominant driver of short- and medium-term changes in real exchange rates for the G-7 countries; accounting for more than 90 percent of the variance at the five-year horizon. I then develop a model in which risk shocks account for dark matter's role as a driver of exchange-rate dynamics and other macro variables.

Abstract

Dark matter accounts for 83 percent of the matter in the universe and plays a central role in cosmology modeling. This paper argues that an analogous form of dark matter plays a similarly important role in international macroeconomics. Exchange-rate dark matter is invisible, but its existence can be inferred from observations on real exchange rates and interest rates. I first show that dark matter is the dominant driver of short- and medium-term changes in real exchange rates for the G-7 countries; accounting for more than 90 percent of the variance at the five-year horizon. I then develop a model in which risk shocks account for dark matter's role as a driver of exchange-rate dynamics and other macro variables.

1 Introduction

In cosmology, “dark matter” is a mysterious material that exerts a gravitational pull but does not emit light or other electromagnetic radiation. As such, it cannot be directly detected with a telescope but its existence is inferred from observations on the movements of galaxies and other astrological phenomena. Dark matter is believed to account for 83 percent of the matter in the universe and plays a central role in cosmology modeling (see Trimble, 1987). This paper argues that an analogous form of dark matter plays an important role in international macroeconomics.

Like its cosmological counterpart, economic dark matter cannot be directly observed, but its existence can be inferred from observations on key variables. In particular, the first part of this paper shows that dark matter is the dominant driver of changes in real exchange rates for the G-7 currencies over short-and medium-term horizons; accounting for more than 90 percent of the variance at the five-year horizon. This finding is not based on any economic model. Instead it is derived from the discrepancy between the observed dynamics of real exchange rates and those that can be attributed to the behavior of real interest differentials. As a matter of accounting, the current real exchange rate reflects: (i) current and expected future real interest differentials, (ii) expected future excess returns on foreign currency positions, and (iii) expectations concerning the long-run real exchange rate. Consequently, any discrepancy between the observed depreciation rate and the change attributable to the behavior of real interest differentials must reflect variations in expected excess returns and/or the expected long-run real exchange rate. Exchange-rate dark matter exerts a force on these expectations but not on current and future real interest differentials.

The empirical importance of dark matter as a driver of real exchange rates poses an important question: Is the nature of the dark matter such that it only affects exchange rates, or does it play a central role in the determination of international macroeconomic relationships? I take up this question in the second part of the paper. Here I present a DSGE model in which households’ preferences are subject to risk shocks that affect their degree of risk aversion. In equilibrium, these risk shocks change the risk premia embedded in real exchange rates and other asset prices, as well as households’ consumption, saving and portfolio decisions. Importantly, they also represent a possible source of exchange-rate dark matter because they change the excess currency returns households expect without significantly affecting real interest differentials.

I calibrate the model to match the moments of real depreciation rates, consumption growth rates and real interest differentials and use the equilibrium dynamics to compute the contribution of dark matter to the variance of real depreciation rates over a range of horizons. The results of these calculations are similar to the estimates found in the G-7 data: Dark matter accounts for 87 percent of the variance in real depreciation rates at the five-year horizon. I then show that risk shocks have significant macroeconomic effects; they are the main driver of consumption growth, real interest rates and trade flows. Indeed, risk shocks play the dominant role in determining economic activity throughout the world economy. Thus, in a model where risk shocks are important enough to account for the role dark matter plays in driving exchange-rate dynamics, they also are the primary source of international macroeconomic dynamics. This result brings a different perspective to the widely-held view that exchange rates are largely disconnected from macroeconomic fundamentals (Obstfeld and Rogoff, 2001). It suggests that exchange-rates appear disconnected from traditional macroeconomic fundamentals because they are particularly susceptible to risk shocks that drive variations in expected excess currency returns, but these same shocks also have significant macroeconomic implications.

This paper contributes to the literature on exchange-rates and international macroeconomics in several ways. First, it provides a new perspective on some long-standing exchange-rate puzzles. Since Meese and Rogoff (1983), researchers have found it very difficult to consistently and reliably relate short- and medium-term variations in exchange rates to changing macroeconomic variables. For example, recent models by Mark (2009), Engel and West (2006) and Engel, Mark, and West (2008) link short-term spot rate movements to changing expectations concerning the future path of interest rates controlled by central banks, but they account for a small faction of actual spot rate volatility over months and quarters (see Evans, 2011). The empirical results in Section 1 show how the poor empirical performance of these models reflects the importance of dark matter. More specifically, I find that the fraction of the variance in real depreciation rates for the G-7 countries (verses the U.S.) attributable to expectations and news concerning future real interest differentials falls from (a cross-country average) of four percent at the one month horizon to below two percent at five years. In effect, then, variations in real interest rates have little relevance for understanding real exchange rate behavior among the G-7 countries.

My analysis also contributes to the literature on the Forward Premium Puzzle. Traditionally, researchers have focused on the factors affecting the estimated coefficient on the interest differential in the Fama (1984) regression. For example, Moore and Roche (2009), Verdelhan (2010) and Bansal and Shaliastovich (2010) develop models where variations in the foreign exchange risk premium induce omitted variable bias in the coefficient estimate; while others, including Froot and Thaler (1990), Evans and Lewis (1995) and Bacchetta and Van Wincoop (2010) consider the effects of informational frictions. In contrast, my results provide perspective on the regression R2 statistics. If dark matter were absent, the small values for the R2 statistics we typically observe could be viewed as evidence that news concerning future interest differentials dominates variations in the current differential. My results show that this interpretation is only partially correct. News concerning future differentials does dominate the variations in the current differential, but the small R2 statistics arise because future depreciation rates are primarily driven by dark matter in a manner that cannot be forecast by the current interest differential. News may account for the difficulty in forecasting depreciation rates, but it is not news related to future interest differentials.

The model presented in Section 2 draws on several lines of research from the asset-pricing and open-economy macro literatures. The core of the model is entirely standard. There are two countries, each populated by a continuum of infinitely-lived households with preferences defined over the consumption of two perishable traded goods. For the sake of clarity, the world supply of each traded good follows an exogenous endowment process and there are no impediments to international trade. To this simple structure I add three key features: external habits, incomplete markets and collateral constraints. This is a novel combination of features to find in an open-economy DSGE model, but they are all necessary to provide a rationale for the role that dark matter plays in exchange-rate determination.

I introduce external habits into the specification of households’ preferences for a simple reason. Campbell and Cochrane (1999) (hereafter CC) first showed how the presence of habits could account for behavior of equity prices in a model where the equilibrium real interest rates was constant, so it is natural to conjecture that a model with habits could produce exchange-rate dynamics without large variations in interest differentials. I adapt the CC habit specification to an open-economy setting. In their model the consumption surplus ratio varies in response to consumption shocks which are entirely determined by an exogenous endowment process.1 This makes little sense in an open-economy setting because the composition of households’ consumption basket varies endogenously with the terms of trade. I assume, instead, that the consumption surplus ratios for households in each country are subject to exogenous shocks. These shocks have the natural interpretation of risk-shocks because they change the local curvature of the households’ utility. As in the CC model, this specification implies that habits vary with changes in aggregate consumption, but the relationship is derived endogenously allowing for the effects of risk shocks on consumption via the terms of trade.

The macroeconomic effects of risk shocks are influenced by two restrictions of households’ asset holdings. There are four asset markets in the model; two for real bonds and two for equities. Domestic (foreign) bonds provide the holder with a known return measured in terms of the domestic (foreign) consumption basket, while domestic (foreign) equity represents a claim on the endowment stream for the domestic (foreign) good.2 To impede international risk-sharing, I prohibit households from holding foreign equity. If this restriction were absent, markets would be complete and risk shocks would produce a negative correlation between the consumption surplus ratio and aggregate consumption via variations in the terms of trade. This would make habits more volatile than consumption - a counterintuitive implication.3 There is, of course, a long literature studying open economy models with incomplete markets and a single bond. My model adds to a newer line of research that examines DSGE models with multiple assets and incomplete markets (see, e.g., Evans and Hnatkovska, 2005a, 2005b, 2007; Van Wincoop and Tille, 2007; Hnatkovska, 2010; Devereux and Sutherland, 2010; and Pavlova and Rigobon, 2010).

The model places an additional restriction on households’ asset holdings: a collateral constraint that limits the extent to which they can accumulate international debt. Specifically, I assume that households must hold foreign bonds as collateral against the value of their international liabilities (i.e. their short position in domestic bonds). This constraint plays a critical role in the international transmission of risk shocks. As in the CC model, variations in the consumption surplus ratio affect the prices of risky assets via a change in the curvature of households’ utility, but here these valuation effects are concentrated in a few asset markets because the prohibition on holding foreign equity inhibits international risk-sharing. For example, a risk shock that increases domestic risk aversion induces a fall in home equity prices that pushes domestic households towards their collateral constraint. As a result, domestic households adjust their portfolios in a way that puts downward pressure on the foreign exchange risk premium inducing an immediate depreciation in the real exchange rate. Thus the collateral constraints play the central role of translating domestically induced capital gains and losses in local asset markets into the portfolio shifts that change the risk premia embedded in the exchange rates. This role for the collateral constraints differs from that found in the recent literature on sudden stops (see, e.g., Mendoza, 2010). In those models the presence of collateral constraints cuts off foreign borrowing following adverse shocks. Here households take the pre-emptive measure of shifting their portfolios as they move closer to the point where the constraint would bind. Notice, also, that this mechanism linking risk shocks to the exchange rate via portfolio shifts and variations in the risk premium is foreshadowed in Kollmann (2001), Devereux and Engel (2002), Obstfeld and Rogoff (2003), Duarte and Stockman (2005) and Blanchard, Giavazzi, and Sa (2005). It is also reminiscent of work on portfolio balance models by Kouri (1976) and Henderson and Rogoff (1982).

The remainder of the paper is divided into three sections. Section 1 describes my empirical analysis of the role played by dark matter in the determination of real depreciation rates for the G-7 currencies. Section 2 presents the model with risk shocks. In Section 3 I examine whether risk-shocks can be a possible source of exchange-rate dark matter, and whether they have significant effects on the real economy beyond the foreign exchange market. Section 4 concludes.

2 Dark Matter and Depreciation Rates

In this section, I first present a method for estimating the importance of real interest differentials as drivers of real depreciation rates over a wide range of horizons. I then use data from the G-7 countries during the post Bretton-Woods era to estimate the contribution of real interest rate variations to the volatility of depreciation rates with horizons of one month to five years. These estimates produce a remarkably consistent picture: Real interest rates have been a minor driver of depreciation rates during the floating-rate period. Indeed for major currency pairs, they are a very minor driver. Most of the volatility in real exchange rates we have observed for the past 35 years reflects the effects of changing expectations concerning excess current returns and long-run real exchange rates. Exchange-rate dark matter exerts a force on these expectations but not on current and future real interest differentials.

2.1 Depreciation Rate Accounting

I use an accounting identity to identify all the factors driving the real depreciation rate. Let εt denote the log real exchange rate defined as the log relative price of the foreign consumption basket in terms of the home consumption basket at the start of period t. Throughout I will designate the U.S. as the home country, so a rise (fall) in εt signifies a real depreciation (appreciation) of the U.S. dollar. The identity is based on the definition of the expected log excess real return on holding foreign currency between the start of periods t and t + 1 :

δ t = E t ε t + 1 ε t + r ^ t r t , ( 1 )

where rt and r^t denote the log of the U.S. and foreign gross real interest rate (hereafter, hats “^” identify foreign variables) and 𝔼t denotes expectations conditioned on information known at the start of period t. I will refer to δt as the foreign exchange risk premium, although, strictly speaking, δt also contains a Jensen inequality term to account for the fact that we are dealing with log rather than gross returns.

To derive the accounting identity, I rewrite (1) as a difference equation in the log real exchange rate and solve forward. Applying the Law of Iterated Expectations to the resulting expression produces

ε t = 𝔼 t Σ i = 0 { r ^ t + i r t + i } 𝔼 t Σ i = 0 δ t + i 𝔼 t ε ¯ , ( 2 )

where ε¯limtεt. Thus, the real exchange rate reflects current and expected future real interest differentials, r^t+irt+i; current and expected future risk premia, δt+i; and expectations concerning the long-term real exchange rate, ε¯. Any change in the real exchange rate must come from variations in at least one of these factors.

For empirical purposes it proves useful to consider the implications of (2) for the h-period depreciation rate, Δhεt+hεt+hεt. By definition, this h-period rate equals the sum of expected depreciation rate, 𝔼tΔhεt+h, and the h–period-ahead forecast error, εt+h – 𝔼tεt+h. Both components can be directly computed from (2) as

𝔼 t Δ h ε t + h = 𝔼 t Σ i = 0 h 1 ( r t + i r ^ t + i ) + 𝔼 t Σ i = 0 h 1 δ t + i and ( 3 )
ε t + h t ε t + h = ( t + h t ) Σ i = h ( r ^ t + i r t + i ) ( t + h t ) Σ i = h δ t + i + ( t + h t ) ε ¯ . ( 4 )

Substituting these expressions into the identity Δεt+hh=𝔼tΔhεt+h+εt+h𝔼tεt+h produces

Δ h ε t + h = 𝔼 t Σ i = 0 h 1 ( r t + i r ^ t + i ) + ( 𝔼 t + h 𝔼 t ) Σ i = h ( r ^ t + i r t + i ) + 𝔼 t Σ i = 0 h 1 δ t + i ( 𝔼 t + h 𝔼 t ) Σ i = h 𝔼 t + i + ( 𝔼 t + h 𝔼 t ) ε ¯ . ( 5 )

Equation (5) identifies all the factors that can drive the h-period depreciation rate. The expression follows simply from the Law of Iterated Expectations and the definition of the risk premium in (1). It contains no assumptions about the behavior of interest rates, the expected long-run real exchange rate, or anything else about the structure of the economy. Consequently, (5) provides us with a framework for studying the empirical drivers over real depreciation rates without reference to a particular economic model.

We can use equation (5) to decompose observed variations in depreciation rates along two dimensions. The first concerns the split between anticipated and unanticipated variations. As (3) and (4) show, variations in the depreciation rate will be largely unanticipated when news between t and t + h concerning future interest rates, risk premia and/or the long-term real exchange rate dominates the changes in the expected near-term path for the interest differential and risk premium. Insofar as short-horizon depreciation rates appear largely unforecastable with standard macro variables, we should expect to find that news accounts for most of the variations in Δhεt+h at short horizons h.

The second dimension concerns the split between the role of the real interest differential and the other factors. In principle, the differential can drive the depreciation rate via both expectations as in (3) and news as in (4). The total contribution is therefore given by the first two terms on the right-hand-side of (5). Equation (5) makes clear that depreciation rates could also be driven by other factors that affect the risk premia and revisions in the expected long-run real exchange rate, ε¯t+h𝔼tε¯t+h. In macro models where the variations in δt are small, and ε¯ is pinned down by a unique steady state value for the real exchange rate (e.g. via PPP), the terms in the second row of (5) are unimportant, so the real interest differentials are the prime driver of the real depreciation rate at all horizons.

To investigate whether this macro perspective on the driver of depreciation rates is supported in the data, I compare actual real depreciation rates for major currency pairs against estimates of the first two terms on right-hand-side of (5) computed from Vector Autogression (VAR) models. More specifically, we can rewrite (5) as

Δ h ε t + h = r t , h E + r t , h U + ζ t + h , ( 6 )

where rt,hE=𝔼tΣi=0h1(rt+ir^t+i),rt+hU=(𝔼t+h𝔼t)Σi=h(r^t+irt+i),

and ζt+h=𝔼tΣi=0h1δt+i(𝔼t+h𝔼t)Σi=hδt+i(𝔼t+h𝔼t)ε¯.

I refer to ζt+h as exchange-rate dark matter in the sense that it exerts a force on the real depreciation rate that is not detectable from data on interest differentials.

At this stage I will be agnostic about whether the effects of dark matter are transmitted through the risk premia on long-term exchange rate expectations. My goal is simply to infer its empirical importance by estimating the variance contribution of the interest differential. For this purpose, I use (6) to compute the following variance ratios:

h r = 𝕍 ( r t , h E + r t + h U ) 𝕍 ( Δ h ε t + h ) , h r E = 𝕍 ( r t , h E ) 𝕍 ( Δ h ε t + h ) , and h r U = 𝕍 ( r t + h U ) 𝕍 ( Δ h ε t + h ) , ( 7 )

where 𝕍(.) denotes the population variance. Here hr measures the fraction of the variance in the h-period depreciation rate that can be attributed to variations in the interest differential, while hre and hrU identify the faction operating via variations in expected future differentials, rt,hE, and news concerning future differentials, rt+hU, respectively. Below I report estimates of these ratios for horizons h ranging from one month to five years.

2.2 Estimation

It is straightforward to estimate the ratios in (7) from a VAR. Let the vector

x t = [ î t i t , Δ p ^ t Δ p t , Δ ε t , s p r t , s p r ^ t ] ʹ

follow a k′th. order VAR:

xt = a1xt–1 + a2xt–2 + ….akxt–k + ut,

where the ai’s are matrices of coefficients from each of the VAR equations, and ut is a vector of mean-zero shocks. The xt vector contains the interest differential on one-period nominal bonds, ît – it; the inflation differential, Δp^tΔpt; the real depreciation rate, Δεt; and the spreads between long- and short-term nominal rates, sprt and spr^t. To compute the variance ratios, the VAR is written in companion form

[ x t x t k + 1 ] = [ a 1 a k I I 0 ] [ x t 1 x t k ] + [ u t 0 0 ] ,

or, more compactly,

X t = A X t 1 + U t . ( 8 )

Multi-period forecasts are easily computed from (8) as 𝔼[Xt+i|Xt] = AiXt, where Ai denotes i multiplications of the companion matrix A.

Several features of the VAR deserve mention. First, the specification includes the monthly real depreciation rate rather than the log real exchange rate, εt. It is well-known that the time series for εt displays a great deal of persistence across many currency pairs. Indeed, the econometric evidence on the presence or absence of a unit root is not clear cut. By contrast, depreciation rates display very little persistence, so the VAR estimates will not be vulnerable to the statistical issues associated with the presence of a unit root in εt. The second feature concerns the inclusion of the interest and inflation differentials, ît – it and Δp^tΔpt; and the spreads between long- and short-term rates, sprt and spr^. These differentials and spreads exhibit much less persistence than do nominal interest rates and inflation rates separately. Again, the use of these variables effectively side-steps any issues related to the presence of unit roots in the VAR. The third feature concerns timing. By construction, all the variables in xt are publicly known at the start of period t. This means that expectations conditioned on Xt are conditioned on a true subset of the information available to agents at the start of the period.

To compute the variance ratios in (7) let the vectors

li = [1 0 0 … 0], lΔp = [0 1 0 … 0] and lε = [0 0 1 0 … 0]

select îtit, Δp^tΔpt and Δεt from Xt. We can now compute estimates of the real interest rate differential as r^trt=lrXt, where lr = lilΔpA. The interest rate elements in the variance ratios are now calculated as

r t , h E = l r Σ i = 0 h 1 A i X t = l r ( I A ) 1 ( I A h ) X t , and r t + h U = l r ( I A ) 1 ( BU t + h + ABU t + h 1 + ….. A h 1 BU t + 1 ) ,

while the h-period depreciation rate is given by

Δ h ε t + h = l ε Σ i = 1 h A i X t + l ε ( I A ) 1 Σ i = 1 h ( I A i ) BU t + i = l ε ( I A ) 1 ( I A h ) X t + l ε ( I A ) 1 Σ i = 1 h ( I A i ) BU t + i .

Finally, let ∑u denote the variance of Ut, the vector of shocks in the VAR. Since the specification of the VAR insures that Xt is covariance stationary process, the variance of Xt, ∑x, solves ∑x = A∑xA′ + ∑u. We can now use the expressions above to compute

𝕍 ( r t , h E ) = l r ( I A ) 1 ( I A h ) Σ x ( I A h ) ( 1 A ) 1 l r , 𝕍 ( r t , h U ) = l r ( I A ) 1 ( Σ i = 0 h 1 A i u B ( A i ) ) ( I A ) 1 l r , and 𝕍 ( Δ h ε t + h ) = l ε ( I A ) 1 ( I A h ) Σ x ( I A h ) ( I A ) 1 l ε + l ε ( 1 A ) 1 ( Σ i = 1 h ( I A i ) u B ( I A i ) ) ( I A ) 1 l ε .

The ratios in (7) are calculated from these three variances.

2.3 Data and Results

My empirical results use monthly data spanning 1975:01 to 2007:12, subject to the availability of individual series. I deliberately omitted the 2008 financial crises from the sample period in order to focus on the role played by interest differentials under normal market conditions. Since basic arbitrage conditions, such as covered interest parity, broke down at the height of the crisis, we might anticipate that risk premia played a larger role in driving depreciation rates during this period than at other times. Consequently, extending the sample period to include the 2008 financial crisis could well lead me to under-estimate the importance of real interest differentials under normal conditions.

I examine the behavior of real depreciation rates for the U.S. relative to Canada, France, Germany, Italy, Japan, and the U.K.. The VARs are estimated using monthly data on spot rates, Eurodeposit rates, and consumer price indices obtained from Datastream. The real exchange rate at the start of month t, t ≡ exp(εt), is computed as StP^t/Pt, where St is the spot price (USD/FC) at the end of trading (i.e. 12:00 noon E.S.T.) on the last trading day (Monday - Friday) in month t – 1. Pt and P^t are the last reported levels for the U.S. and foreign country consumer price indices before the start of month t. The value of t is therefore public information at the start of month t. I use two sets of interest rates in the VAR. The real interest differential is computed from inflation and the one month nominal rates on Eurodeposits. Specifically, I compute the one month U.S. real rate at the start of month t, rt, as it𝔼˜t(pt+1pt), where it is the midpoint of the bid and offer rates on the last trading day of month t - 1, and 𝔼˜t(pt+1pt)=lΔpA˜Xt is an estimate of inflation during month t computed from the VAR. The one month real rate in the foreign country is computed analogously as r^t=ît𝔼˜t(p^t+1p^t). I also use the spread between the one year and one month Eurodeposit rates, sprt=it12it and spr^t=ît12ît where it12 and ît12 are the midpoints for the 12-month Eurodeposit rate on the last trading day of month t – 1.

Table 1 reports summary statistics for the estimated VARs used to compute the variance ratios. The first two rows of Panel A show the sample period and number of observations used to estimate the VAR for each currency pair. The third row reports the order of the VAR that minimizes the Akaike Information criterion. This is the number of lags included in the VAR used to estimate the variance ratios discussed below, but computing the ratios from VARs with one more or less lag does not materially affect the results.

Table 1:

VAR Summary Information

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Notes: The variables in the VAR are the one-month nominal interest differential, î–i; the one month inflation differential, Δp^Δp, the one month real depreciation rate, Δε; the US one-year one-month nominal spread, spr; and the foreign country spread, spr^. Panel B reports the R2 from the real depreciation equation, and the implied R2 for the real interest differential computed as (lr^lr)A˜Σ˜xA˜ʹ(lr^lr)ʹ/(lr^lr)Σ˜x(lr^lr)ʹ, where à and Σ˜x are the estimated companion matrix and covariance matrix of Xt. Panel C reports the p-value for the null hypothesis that lags of the variable shown in the left hand column does not Granger Cause the equation variable shown at the top of each list. P-values are computed from the ξ2 statistics using heteroskedasticity consistent estimates of the coefficient covariance matrix.

Panel B reports the R2 statistics from the depreciation and interest differential equations in the VARs. As one would expect, very little of the variance in monthly real depreciation rates is accounted for by lagged variables in the VAR. The R2 statistics are generally in the five to six percent range, with the exception of the US/FF rate that is nine percent. The second row in Panel reports the R2 for the real interest differential implied by the estimated equations for the nominal interest rate and inflation differentials. This statistic is computed as the estimated variance of the one-month-ahead forecast for the real differential relative to the estimated variance of the differential; i.e., 𝕍(𝔼[r^trt|Xt1])/𝕍(r^trt). These statistics are a good deal larger than their counterparts for the depreciation rate. They show that the variables in the VAR have an economically significant degree of forecasting power for future real interest rate differentials.

Further statistical evidence on the forecasting power of the variables in the VAR is provided in Panel C where I report the p-values for Granger Causality tests on the nominal interest and inflation differentials. There is very strong evidence rejecting the null hypothesis that spreads do not Granger Cause interest differentials across all currency pairs. The spreads appear to have significant incremental forecasting power for future interest differentials beyond that contained in their own history, so including them in the VAR improves the precision of the forecasts of future interest differentials used in computing the variance ratios. The results of the other Granger Causality tests are less clear cut. Lagged depreciation rates have some incremental forecasting power for future interest differentials and inflation differentials in some of the currency pairs. Similarly, lagged interest differentials and spreads have forecasting power for future inflation differentials in some cases, but there is no uniform pattern.

Table 2 reports estimates of the variance ratios, hr and hrU, for horizons ranging from one month to five years (i.e., h = 1,..60), computed from the VARs for each currency pair. The table also reports the 5’th. and 95’th. percentiles of the bootstrap distribution of the ratio at each horizon. To compute this distribution, I first generating a pseudo data series for the vector of variables xt equal to the span of the data sample using the VAR parameter estimates and a bootstrap sample of the VAR residuals. I then re-estimate the VAR with this pseudo data and compute the variance ratios for h = 1,..60. This procedure is repeated 5000 times to generate a bootstrap distribution of the variance ratios at each horizon from which the percentiles are calculated.

Table 2:

Variance Ratios

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Notes: The first row of statistics in each block are the estimates of hr (Panel A) and hrU (Panel B) computed from the VARs as specified in Table 1 for each of the currency pairs. The second and third rows report the 5’th. and 95’th. percentiles from the bootstrap distribution of hr (Panel A) and hrU (Panel B).

Panel A of Table 2 reports estimates of the variance contribution of the real interest differential, hr, at horizons of one month, one quarter, one, two and five years. Two features immediately stand out: The estimates of hr are surprisingly small for every currency pair and they decline as the horizon increases. At the one month horizon, the largest estimate for hr is just 0.264 for the USD/ITL, while for major currencies like, the USD/EUR and USD/GBP, the estimates are as small as 0.042. At the five year horizon, the estimates are even smaller, in several cases well below 0.05. Of course, all these estimates for hr contain sampling error and so may, to some degree, understate the actual contribution of the real depreciation rate. One way to assess this possibility is to examine the 95’th percentiles of the bootstrap distribution for hr, which are reported in the third row of each block in the panel. These percentiles can be view as an optimistic upper bound on the importance of real interest differentials as a driver of depreciation rates. However, as the table shows, these bounds are not significantly above the estimates of hr. Thus, the simple message from panel A is that real interest differentials play a decidedly minor role in driving real depreciation rates up to a five year horizon.

Panel B reports estimates of hrU, the ratio that measures the variance contribution of news concerning future differentials. By definition hr=hrE+hrU so the estimates of hrU provide information on the relative importance of variations in expected future differentials, rt,hE, verses news concerning future differentials, rt+hU, as drivers of depreciation rates. As the table shows, news is comparatively more important at short horizons than at long horizons. For every currency pair, the estimates of hrU are at most a couple of percentage points less than the estimates of hr for h = 1, 3. This finding is consistent with well-know difficulty in forecasting short-term depreciation rates. If hrhrE for small h, interest differentials would have more forecasting power for short-term depreciation rates than we observe in the data. As the horizon rises beyond a couple of months, the estimates of hrU fall more quickly than the estimates of hr. This is most readily seen in Figure 1 which plots the estimates of hr and hrU against h for all seven currency pairs. The vertical distance between the two plots identifies the estimated value for hrE. The shaded band shows the 90 percent confidence band for hr from the bootstrap.

Figure 1:
Figure 1:

Variance Ratios Rhr (solid) and RhrU (dashed).

Citation: IMF Working Papers 2012, 066; 10.5089/9781463938437.001.A001

The estimated variance ratios in Table 2 and Figure 1 depend on the specifications of the VAR, so it is important to assess their robustness with respect to alternative specifications. To this end, I repeated all the calculations using one more lag of xt in the estimated VAR and one less lag (for specifications with k > 1 in Table 1). In all cases, the estimated variance ratios were very similar to those reported above. In particular, the estimates of hr are typically well below 0.15 at short horizons and decline sharply as the horizon rises.

The results may also be sensitive to the amount of information available to agents in the economy. It is possible that agents revise their long-horizon forecasts for the real interest differential on the basis of information that is uncorrelated with current interest rates, inflation rates and spreads. Such information would induce volatility in rt+hU (for large h) and contribute to the variance of the real depreciation rate, but is unlikely to be reflected in the VAR estimates unless variance of the dark matter, ζt+h, is small. Intuitively, variations in depreciation rates provide a signal on the information flow affecting long-term differential forecasts, but the signal-to-noise ratio is very low when there are significant movements in ζt+h. Consequently, although the VAR estimates of rt+hU condition on depreciation rates, they may not fully reflect the information agents use to revise their long-horizon forecasts of differentials when dark matter is present. Of course, this observation does not undermine my central finding. If dark matter were not present, the estimates of hr should be close to one. Clearly, the evidence is inconsistent with this implication. Furthermore, since the VARs include the spreads which strongly Granger Cause interest differentials, and the VAR estimates account for a large fraction of the variance in real interest differentials, it is unlikely that my results would materially change with the addition of other variables.

2.4 The UIP Perspective

These findings are new to the exchange-rate literature so it is useful to place them in perspective relative to the well-known results on Uncovered Interest Parity (UIP). In particular, the results in Table 2 compliment the information contained in regressions of real depreciation rates on real interest differentials. To see why, consider the regression of the future one-period depreciation rate on the current differential; i.e., the Fama (1984) regression for real rates:

Δ ε t + 1 = β 0 + β 1 ( r t r ^ t ) + u t + 1 . ( 9 )

Using the decomposition of the depreciation rate in (6) (with h = 1) we can compute the population values of β1 and the regression R2 statistic as

β 1 = 1 + 𝕍 ( ζ t + 1 , r t r ^ t ) 𝕍 ( r t r ^ t ) ( 10 )

and

R 2 = β 1 2 = 𝕍 ( r t , 1 E ) 𝕍 ( r t , 1 E + r t + 1 U ) 𝕍 ( r t , 1 E + r t + 1 U ) 𝕍 ( ε t + 1 ) = β 1 2 ( 1 r E 1 r ) 1 r . ( 11 )

Consider the expression for β1 in equation (10). Under rational expectations ℂ𝕍(ζt+1,rtr^t)=ℂ𝕍(δ1,rtr^t), so β1 differs from one when the current risk premium is correlated with the interest differential. Understanding the source of this correlation is the focus of recent research on the origins of real UIP deviations (see, e.g., Verdelhan, 2010). The role of the variance ratios is displayed in equation (11). Here we see that a low R2 reflects a combination of three factors: a small absolute value for β1; a low ratio for 1rE/1r; and a small value for 1r. Obviously, information on β1 is available from estimating (9), but beyond that we cannot interpreted the value for R2/β12. To illustrate, suppose that the estimated value for R2 is small (e.g. < 0.05) and we cannot reject the null that β1 = 1. In this case, although interest differentials appear to provide unbiased forecasts of future depreciation rates, they lack significant forecasting power from an economic perspective. Is this because news concerning future interest differentials dominates variations in current differentials so that 1rE/1r is small? Or, does it reflect variations in dark matter that are uncorrelated with current differentials so that 1r is small? Estimates of the variance ratios in Table 2 allow us to answer these questions. More generally, the variance ratios provide us with information on the drivers of future depreciation rates that are uncorrelated with current interest differentials.

Table 3 reports estimates of the Fama regression in (9) for the seven currency pairs in my data sample. The real interest differential on the right-hand-side is computed as iti^t𝔼˜[Δpt+1Δp^t+1|Xt], where 𝔼˜[Δpt+1Δp^t+1|Xt] denotes the forecasts computed from the VARs. Panel A of the table reports the coefficient estimates and standard errors (in parenthesis) that account for heteroskedasticity in the regression errors and the fact that the real differential is estimated from the VAR.4 Panel B reports the p-values for the null H0: β1 = 1 and decomposes the R2 statistics into the variance ratios as discussed above. These ratios are computed from the statistics in Table 2 for the cases where h = 1.

Table 3:

Real UIP Regressions

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Notes: Panel A reports coefficient estimates and asymptotic standard errors that account for heteroskedasticity and sample variation in the estimated real interest differential. The upper row in panel B reports the asymptotic p-values for the t-test of H0:β1 = 1. The remaining rows decompose the R2 statistics from the regression using the VAR ratios computed from the VARs, as reported in Table 2. Here R1rE/R1r=𝕍(rt,1E+rt+1U) and R1r=𝕍(rt,1E+rt+1U)/𝕍(Δεt+1).

Three features of Table 3 stand out. First, the estimates of β1 vary considerably from currency to currency, and have comparatively large standard errors. Consequently, in three of the seven cases we cannot reject the null of β1 = 1 at the conventional five percent level. The second feature concerns the R2 statistics. As one would expect, they are small. Real interest differentials have little economically significant forecasting power for short-term depreciation rates. Third, the drivers of depreciation rates vary across currency pairs. In particular, the estimates of hrE/hr are much lower for the USD/JPY, USD/EUR and USD/DEM than for the other currency pairs. In these cases the effects of news concerning future interest differentials dominates variations in current differentials. It is also striking that both 1rE/1r are extremely small in the case of the USD/EUR, the world’s most actively traded currency pair. Although news about future US and EU interest rates drives the USD/EUR depreciation rate to some extent, most of the variations we observe reflect the influence of dark matter. Finally, notice that even in cases where we cannot reject the null of β1 = 1, (i.e., for the USD/CAN, USD/DEM and USD/ITL) the values for Rhr indicate that real interest differentials are far from the dominant drivers of real depreciation rates. Remember that β1 = 1 under rational expectations when the risk premium is uncorrelated with the interest differential but not necessarily constant. The low values for Rhr we see across all currency pairs suggest that the risk premia could be a significant driver of depreciation rates even in instances where we cannot reject β1 = 1.

These findings compliment recent results reported by Engel (2011). He uses the accounting identity in equation (2) to study the relationship between the real interest differential and the present value of expected excess currency returns, 𝔼tΣi=0δt+i, under the assumption that long-run exchange-rate expectations, 𝔼tε¯, are constant. Since ℂ𝕍(δt,rtr^t) must be negative if variations in the risk premium account for the downward bias in the estimates of β1, one would expect that ℂ𝕍(𝔼tΣi=0δt+i,rtr^t) is also negative. Surprisingly, Engel’s estimates of this covariance are positive, suggesting that expectations of future risk premia (i.e., 𝔼tδt+i, for some i > 0) are positively correlated with the interest differential. In contrast, my findings focus on variations in 𝔼tΣi=0δt+i that are unrelated to changes in the interest differential.

The results in Tables 2 and 3 show that real interest differentials are a rather minor driver of real depreciations rates over horizons up to five years. It appears, instead, that dark matter driving changes in long-horizon real exchange-rate expectations and variations in risk premia account for the lion’s share of real exchange rate movements. This finding represents a major challenge to existing theoretical models of exchange-rate determination. Traditional macro models either assume that risk premia are constant, or are calibrated so that variations in the premia are quite minor. Thus, from the perspective of these models, the dark matter must mainly reflect variations in expectations concerning the long-term real exchange rate. Such variations could reflect Balassa-Samuelson effects (see, Balassa, 1964 and Samuelson, 1964), but if that were the case we would expect to see evidence of significant variation in the (weighted) difference between the relative prices of nontraded to traded goods across countries over long, but finite horizons. This is not what we observe. For example, Engel (1999) finds remarkably little evidence that Balassa-Samuelson type effects contribute significantly to depreciation rates at the five-year horizon. So, even if Balassa-Samuelson effects give rise to some variations in expectations concerning the long-term real exchange rate, it seems implausible to attribute all the influence of dark matter to driving such expectations.

In the remainder of this paper I pursue an alternative explanation for the findings in Tables 2 and 3. Namely, that dark matter influences exchange rates by driving variations in the risk premia. I begin this task in the next section by presenting an open-economy DSGE model in which households’ preferences are subject to risk shocks that affect their degree of risk aversion (i.e., the curvature of their utility functions). These shocks represent a possible source of exchange-rate dark matter because they change the excess currency returns households expect without significantly affecting real interest differentials.

3 The Model

The model is designed to examine the interplay between incomplete risk-sharing and collateral constraints in a world where households’ risk aversion varies stochastically. The world comprises two symmetric countries, which I refer to as the U.S. and Europe. Each country is populated by infinitely-lived households with preferences defined over the consumption of two perishable traded goods. For simplicity, there are no nontraded goods or impediments to trade in goods between the two countries. I also assume that the world supply of each traded good follows an exogenous endowment process, one located in each country. To this simple structure I add three key features: external habits, incomplete markets and collateral constraints. As I argued in the introduction, this combination of features is necessary to provide a rationale for the role that dark matter plays in exchange-rate determination.

3.1 Model Details

Household Preferences

Each country is populated by a continuum of identical households distributed on the interval [0,1]. Households’ preferences are defined over a basket of traded consumption goods. In particular, the expected utility of a representative U.S. household i ∈ [0,1] in period t is given by

𝕌 i . t = 𝔼 t Σ j = 0 β j 𝒰 ( C i , t + j , H t + j ) , w i t h 𝒰 ( C i , t , H t ) = 1 1 γ { ( C i , t H t ) 1 γ 1 } , ( 12 )

where 1 > β > 0, γ > 0 and 𝔼t denotes expectations conditioned on period-t information, which is common to all U.S. and E.U. households. Each household’s sub-utility 𝒰 (Ci,t, Ht) depends on current consumption, Ci,t, and the subsistence level of consumption, or external habit level, Ht. The habit level is treated as exogenous by individual households but varies with past aggregate U.S. consumption via an autoregressive process for the log surplus ratio, st = ln(St), with St = (CtHt)/Ct:

S t + 1 = ( 1 Φ ) s ¯ + Φ s t + ω ( s t ) v t + 1 , ( 13 )

where 1 > φ > 0 and s¯ is the steady state value of st. The i.i.d. mean-zero, unit variance vt+1 shocks affect the surplus ratio via a non-negative sensitivity function ω(st), which I discuss below. Notice that Ht = [1 – exp(st)]Ct so negative vt shocks raise habit relative to current aggregate consumption, but they cannot push habit above current consumption. In the CC habit specification, the vt shocks are identified by shocks to the endowment process for aggregate consumption. Here aggregate consumption in each country comprises an basket of traded goods that are optimally chosen by households. I therefore treat shocks to the surplus ratio process as exogenous, and derive the correlation between st and aggregate consumption as part of the equilibrium.

The U.S. consumption basket comprises U.S. and E.U. traded goods:

C i , t = 𝒞 ( C i , t U S , C i , t E U ) = ( η 1 θ C i , t U S θ 1 θ + ( 1 η ) 1 θ C i , t E U θ 1 θ ) θ θ 1 , ( 14 )

where Ci,tUS and Ci,tEU identify the consumption of U.S. and E.U. goods by U.S. household i. The parameter η ∈ (0,1) governs the desired share of each good in the basket and θ is the elasticity of substitution between goods. I follow standard practice in the literature and focus on the case where η > 1/2, so that households’ preferences exhibit consumption home-bias.

E.U. household i ∈ [0,1] has analogous preferences:

𝕌 ^ i , t = 𝔼 t Σ j = 0 β j 𝒰 ( Ĉ i , t + j , Ĥ t + j ) , ( 15 )

defined on the gap between the foreign consumption basket, Ĉi,t, and habit, Ĥt, where

Ĉ i , t = 𝒞 ( Ĉ i , t E U , Ĉ i , t U S , ) = ( η 1 θ Ĉ i , t E U θ 1 θ + ( 1 η ) 1 θ Ĉ i , t U S θ 1 θ ) θ θ 1 . ( 16 )

The log surplus ratio, ŝt = lnŜt, with Ŝt = ((ĈtĤt)/Ĉt, follows

ŝ t + 1 = ( 1 Φ ) s ¯ + Φ ŝ t + ω ( ŝ t ) v ^ t + 1 , ( 17 )

where v^t+1 are i.i.d. mean-zero, unit variance shocks.

Shocks to the surplus ratios affect the local curvature of households’ utility functions. In particular, for a representative U.S. and E.U household

C i , t 𝒰 ( C i , t , H t ) 𝒰 c c ( C i , t , H t ) = γ exp ( s t ) and C ^ i , t 𝒰 ( C ^ i , t , H ^ t ) 𝒰 c c ( C ^ i , t , H ^ t ) = γ exp ( s ^ t ) .

Thus negative shocks to the log surplus ratios in (13) and (17) increase the local curvature making households more risk-averse, ceteris paribus. Hereafter, I therefore refer to vt and v^t as risk shocks. Following CC, I assume that the sensitivity function, ω(·), is decreasing in the surplus ratio:

ω ( S ) = { ω ( s max S ) S s max 0 S > s max

where ω is a positive parameter. In the continuous time limit, st and ŝt never exceed the upper bound of smax, so there is a corresponding lower limit on households’ risk-aversion.

Prices and Exchange Rates

I focus on two international relative prices: the terms of trade and the real exchange rate. These prices are linked through the consumption price indices in each country. Let PtUS and PtEU denote the prices of the U.S. and E.U. goods in dollars, while P^tUS and P^tEU denote their prices in euros, respectively. The U.S. and E.U. price indices corresponding to the consumption baskets in (14) and (16) are

P t = ( η ( P t U S ) 1 θ + ( 1 η ) ( P t E U ) 1 θ ) 1 1 θ and P ^ t = ( η ( P ^ t E U ) 1 θ + ( 1 η ) ( P ^ t U S ) 1 θ ) 1 1 θ .

The real exchange rate is defined as the relative price of the E.U. consumption basket in terms of the U.S. basket, t=𝒮tP^t/Pt, where 𝒮t denotes the dollar price of euros. There are no impediments to international trade between the U.S. and the E.U. so the law of one price applies to both the U.S. and E.U. goods: i.e., PtUS=𝒯tP^tUS and PtEU=𝒮tP^tEU. Combining these expressions with the definitions of the real exchange rate and the price indices gives

t = ( η 𝒯 t 1 θ + ( 1 η ) η + ( 1 η ) 𝒯 t 1 θ ) 1 1 θ , ( 18 )

where 𝒯t is the U.S. terms of trade, defined as the relative price of imports in terms of exports, PtEU/PtUS. When there is home bias in consumption (η > 1/2), a deterioration in the U.S. terms of trade (i.e. a rise in 𝒯t) is associated with a real depreciation of the dollar (i.e. a rise in ℰt).

Equation (18) makes clear that the model attributes all variations in real exchange rates to changes in the relative prices of traded goods via the terms of trade. This implication of the model is consistent with the data. When real exchange rates are computed from retail prices, almost all the variations in real depreciation rates originate from changes in the relative prices of traded goods rather than changes in the difference between the relative prices of traded and nontraded goods across countries at horizons of five years or less (Engel, 1999). Thus, the exclusion of nontraded goods from the model will not materially impair its ability to account for the short- and medium-term dynamics of real depreciation rates. Equation (18) also implies that the real depreciation rate is strongly correlated with changes in the terms of trade when there is home bias in consumption. This implication is also consistent with the data. Real depreciation rates are very strongly correlated with changes in terms of trade over short horizons (see, e.g., Evans, 2011).

Assets and Goods Markets

There are four financial markets: a market for U.S. equities, E.U. equities, U.S. bonds and E.U. bonds. U.S. equity represents a claim on the stream of U.S. good endowments. In particular, at the start of period t, the holder of one share of U.S. equity receives a dividend of Dt=(PtUS/Pt)Yt, where Yt is the endowment of the U.S. good, measured in terms of the U.S. consumption basket. The ex-dividend price of U.S. equity in period t is Qt, again measured in terms of U.S. consumption. A share of E.U. equity pays a period-t dividend of D^t=(P^tEU/p^t)Y^t and has an ex-dividend price of Q^t, where Ŷt is the period-t endowment of the E.U. good. Notice that Q^t and D^t are measured relative to the E.U. consumption basket. Households can also hold one-period real U.S. and E.U. bonds. The gross return on holding U.S. bonds between periods t and t + 1 is Rt, measured in terms of U.S. consumption; the analogous return on E.U. bonds is R^t, measured in terms of E.U. consumption.

Households face restrictions on their asset holdings: U.S. households are prohibited from holding shares of E.U. equity, and E.U. households are prohibited from holding U.S. equity. In addition to their holdings of domestic equity, households can hold domestic and foreign bonds subject to a collateral constraint (discussed below). Let Bi,tUS, Bi,tEU and Ai,tUS respectively denote the number of U.S. bonds, E.U. bonds and the number of shares of U.S. equity held by U.S. household i in period t. The budget constraint facing the household is

B i , t U S + t B i , t E U + Q t A i , t U S + C i , t = R t 1 B i , t 1 U S + t R ^ t 1 + A i , t 1 U S ( Q t + D t ) . ( 19 )

The budget constraint facing a typical E.U. household is

B i , t U S / t + B ^ i , t E U + Q ^ t A ^ i , t E U + C ^ i , t = R t 1 B ^ i , t 1 U S / t + R ^ t 1 B ^ i , t 1 E U + A ^ i , t 1 E U ( Q ^ t + D ^ t ) , ( 20 )

where B^i,tUS, B^i,tEU and A^i,tEU respectively denote the number of U.S. bonds, E.U. bonds and the number of shares of E.U. equity held by E.U. household i in period t.

The asset market clearing conditions are straightforward. Both U.S. and E.U bonds are in zero net supply so the bond market clearing conditions are

0 = 0 1 B i , t U S d i + 0 1 B ^ i , t U S d i and 0 = 0 1 B i , t E U d i + 0 1 B ^ i , t E U d i . ( 21 )

The supplies of the U.S. and E.U. equities are normalized to one, so market clearing requires that

1 = 0 1 A i , t U S d i and 1 = 0 1 A ^ i , t E U d i . ( 22 )

Household Decision-Making

Households choose consumption and their portfolios to maximize expected utility subject to the budget constraint and a collateral constraint that prevents the use of Ponzi-schemes in international debt markets. For the case of U.S. household i, the constraint takes the form of a lower bound on U.S. bond holdings:

B i , t U S ( 1 + χ ) t B i , t E U , ( 23 )

where χ > 0. The constraint implies that U.S. households can borrow in the domestic bond market up to the point where the real vale of their debt is (1 + χ) times the value of their foreign bond holdings. The constraint facing E.U. household i takes an analogous form:

B ^ i , t E U ( 1 + χ ) B ^ i , t U S / t . ( 24 )

Market clearing in the goods markets requires that aggregate demand from U.S. and E.U. households matches the world endowment of each traded good:

Y t = 0 1 C i , t U S d i + 0 1 C ^ i , t U S d i and Y ^ t = 0 1 C i , t EU d i + 0 1 C ^ i , t EU d i . ( 25 )

I assume that the log endowments, yt = ln Yt and ŷt = ln Ŷt, follow non-stationary unit root processes:

y t = t + z t and y ^ t = t + z ^ t , with ( 26 a )
t = t 1 + g + u t , z t = ρ z t 1 + e t and z ^ t = ρ z ^ t 1 + e ^ t . ( 26 b )

Here 𝔗t identifies the stochastic trend, while zt and t denote the cyclical components that follow AR(1) processes with 1 > ρ > 0. The three endowment shocks, ut, et and êt are mutually uncorrelated mean-zero normal random variables, with variances σu2, σe2 and σe2, respectively. In the absence of any shocks, both endowments grow at rate g.

The constraints in (23) and (24) have several noteworthy implications. First, they do not limit the total amount of borrowing by any household. For example, (23) implies an upper bound of tBi,tEU on the value of net international debt held by a U.S. household, rather than a hard borrowing limit. Second, the constraints do not restrict households’ choice of debt instrument until they bind. For example, U.S. household can borrow by selling either U.S. or E.U. bonds while Bi,tUS+(1+𝓍)tBi,tEU>0.5 Note, however, that (23) and (24) do exclude the possibility of using equity as collateral. Since households are precluded from holding foreign equity in this simple model, it makes little sense for them to accept foreign equity as collateral when lending internationally.

It proves useful to express the consumption and portfolio decisions facing households in terms of portfolio shares and financial wealth. Let Wi,t denote the real wealth of U.S. household i at the start of period t and let αi,tEQ and αi,tFB identify the fraction of wealth held in domestic equity and foreign bonds at the end of period t:

α i , t E Q = Q t A i , t U S / ( W i , t C i , t ) and α i , t F B = t B i , t EU / ( W i , t C i , t ) .

The problem facing U.S. household i may now be written as

M a x { C i , t U S , C i , t E U , α i , t E Q , α i , t F B } t Σ j = 0 β j ( ( C i , t + j U S , C i , t + j E U ) , H t + j ) ( 27 a )
s . t . W i , t + 1 = R i , t + 1 W ( W i , t C i , t ) and ( 27 b )
N i , t = ( 1 α i , t EQ + χ α i , t FB ) ( W i , t C i , t ) 0. ( 27 c )

Equation (27b) rewrites the budget constraint in terms of wealth and the real return on the households’ portfolio:

R i , t + 1 W = R t + α i , t EQ ( R t + 1 EQ R t ) + α i , t FB ( ( t + 1 / t ) R ^ t R t ) , ( 28 )

where Rt+1EQ=(Qt+1+Dt+1)/Qt is the real return on U.S. equity. Equation (27c) rewrites the collateral restriction in (23) using the portfolio shares.

The problem facing E.U. household i is analogous:

M a x { C ^ i , t US , C ^ i , t EU , α ^ i , t EQ , α ^ i , t FB } 𝔼 t Σ j = 0 β j 𝒰 ( 𝒞 ( C ^ i , t + j EU , C ^ i , t + j US ) , H ^ t + j ) ( 29 a )
s . t . W ^ i , t + 1 = R ^ i , t + 1 W ( W ^ i , t C ^ i , t ) and ( 29 b )
N ^ i , t = ( 1 α ^ i , t EQ + χ α ^ i , t FB ) ( W ^ i , t C ^ t ) 0. ( 29 c )

Here α^i,tEQ and α^i,tFB are the fractions of wealth invested in E.U. equity and foreign (i.e., U.S.) bonds:

α ^ i , t EQ = Q ^ t A ^ i , t EU / ( W ^ i , t C ^ i , t ) and α ^ i , t FB = ( B ^ i , t US / t ) ( W ^ i , t C ^ i , t ) ,

Ŵi,t is real wealth (measured in terms of E.U. consumption) at the start of period t, and R^i,t+1W is the real return on the household’s portfolio:

R ^ i , t + 1 W = R ^ t + α ^ i , t EQ ( R ^ t + 1 EQ R ^ t ) + α ^ i , t FB ( ( t / t + 1 ) R t R ^ t ) , ( 30 )

with R^t+1EQ=(Q^t+1+D^t+1)/Q^t.

Since households within each country have the same preferences and face the same constraints, we can focus on the behavior of a representative U.S. and E.U. household without loss of generality. Hereafter, I drop the i subscripts on consumption and the portfolio shares to simplify notation.

3.2 Equilibrium

An equilibrium comprises a sequence for the real exchange rate {t}, real interest rates {RtandR^t}, and equity returns {RtEQandR^tEQ}, consistent with market clearing in the goods and asset markets given the optimal consumption and portfolio decisions of households and the exogenous endowments. In this model finding the equilibrium processes for {t,Rt,R^t,RtEQandR^tEQ} is complicated by the presence of incomplete markets, portfolio choice, and occasionally binding collateral constraints. This combination of features precludes the use of standard solution methods, so I develop a new procedure that combines barrier methods with second-order approximations around the model’s stochastic steady state. This section provides an overview of the solution procedure. A more complete description of how I solve for the equilibrium is contained in the appendix.

Barrier Methods

Barrier methods are widely used in the optimal control literature to solve optimization problems involving inequality constraints (see Forsgren Anders and Wright, 2002). The basic idea is to modify the objective function so that the optimizing agent is penalized as his actions bring him closer to the barrier described by the inequality constraint. The advantage of this approach is that it converts the original optimization problem with inequality constraints into one with only equality constraints. I then use a set of second-order approximations to solve for the equilibrium exchange-rate and return processes that clear markets given the consumption and portfolio decisions of households from the modified optimization problems. Preston and Roca (2007) and Kim, Kollmann, and Kim (2010) use barrier methods in this way to solve incomplete markets’ models with heterogenous agents. Here I extend the approach to solve a model that also includes portfolio choice.

Following Kim, Kollmann, and Kim (2010), I modify the sub-utility functions for the representative U.S. and E.U. households to

𝒰 ( C t , H t , N t ) = 1 1 γ { ( C t H t ) 1 γ 1 } + μ N ¯ t ( C ¯ t S ¯ ) γ { ln ( N t N ¯ t ) ( N t N ¯ t N ¯ t ) } ( 31 a )

and

𝒰 ( C ^ t , H ^ t , N ^ t ) = 1 1 γ { ( C ^ t H ^ t ) 1 γ 1 } + μ N ¯ t ( C ¯ t S ¯ ) γ { ln ( N ^ t N ¯ t ) ( N ^ t N ¯ t N ¯ t ) } , ( 31 b )

where μ > 0 and bars denote the values of variables in the steady state (defined below). These modifications penalize households as their portfolio choices bring them closer to their respective collateral constraints. In particular, as U.S. households’ bond holdings close in on the point where the constraint binds, Nt=(1αtEQ+𝓍αtFB)(WtCt) nears zero, and the last term on the right-hand-side of (31a) approaches its limiting value of –∞. Similarly, the last term in (31b) approaches –∞ when E.U. households near the point where their collateral constraint binds. The term preceding {.} governs the rate at with the utility cost rise as the household approaches the collateral constraint. In particular, small values for the barrier parameter μ imply that the costs only become significant in a close neighborhood of the constraint. Notice, also, that both terms in parentheses disappear when bond holdings are at their steady state values.

We can understand how these modifications affect households’ decision-making by comparing the first-order conditions from the original optimization problems with those from maximizing (12) subject to (27b) with 𝒰(Ci,t, Ht, Ni,t) replacing 𝒰(Ci,t, Ht) and those from maximizing (15) subject to (29b) with 𝒰(C^i,t,H^t,N^i,t) replacing 𝒰(Ĉi,t, Ĥt). Both sets of first-order conditions for a typical U.S. household can be written as

1 = β t [ ( C t + 1 C t ) γ ( S t + 1 S t ) γ R t + 1 E Q ] , ( 32 a )
1 = β t [ ( C t + 1 C t ) γ ( S t + 1 S t ) γ t + 1 + R ^ t t ] + ( 1 + χ ) t a n d ( 32 b )
1 = β 𝔼 t [ ( C t + 1 C t ) γ ( S t + 1 S t ) γ R t ] + t . ( 32 c )

When the first-order conditions are computed from the original U.S. household’s problem in (27), t=CtγStγt, where t is the Lagrange multiplier on the collateral constraint in (27c). Thus, t is positive if and only if the U.S. constraint in (23) binds (i.e., when Nt = 0). The first-order conditions from the modified optimization problem also take the form of (32) with

t = μ ( C t S t C ¯ t S ¯ ) γ { N ¯ t N t 1 } .

Note that t → ∞ as Nt approaches zero for any positive value of μ; that is as the household moves closer to the point where the collateral constraint binds. Thus, in contrast to the original problem, the optimal bond holdings in the modified problem are chosen so that the constraint never actually binds. The importance of this distinction depends on the size of the barrier parameter, μ. In particular, if we consider a sequence of solutions to the modified problem as μ takes smaller and smaller values, the sequence will converge to the solution of the original problem in the limit as μ → 0 (see, e.g., Forsgren Anders and Wright, 2002). I will examine the robustness of the models’ equilibrium properties to alternative choices for μ that are close to zero.

Approximations

I use a set of second-order approximations to the households’ first-order conditions from the modified optimization problems and the market clearing conditions to find the equilibrium process for the real exchange rate, real interest rates, and other endogenous variables. In some models, incomplete risk-sharing induces non-stationary dynamics in household wealth so there is no unique non-stochastic steady state to use as an approximation point.6 Here I use the stochastic steady state. This is the point at which the exogenous surplus ratios, st and ŝt equal their long run value of s¯, and the cyclical components in the endowment processes, Zt and t, equal zero so the endowments of U.S. and E.U. goods are equal and follow the stochastic trend (i.e., yt = ŷt = 𝔗t). Under these circumstances, households expect both endowments to grow at rate g, (i.e., 𝔼tΔyt+i = 𝔼tΔŷt+i = g, for all i > 0), but they do not expect any future changes in the surplus ratios (i.e., 𝔼tst+i=𝔼ts^t+i=s¯foralli>0). Importantly, households also recognize that future endowments and surplus ratios are subject to shocks. It is this recognition that future shocks will affect the exogenous processes that differentiates the stochastic steady state from its conventional non-stochastic counterpart.

Beyond its conceptual appeal, the use of the stochastic steady state has two technical advantages. First, it allows us to identify a point around which to approximate the equilibrium dynamics without any further embellishment to the model.7 Second, it identifies the steady state portfolio allocations because assets do not have the same riskless return. I discuss these aspects of the solution procedure below.

The Stochastic Steady State To identify the stochastic steady state (hereafter, just the “steady state”), I focus four equilibrium conditions: the first-order conditions determining households’ bond holdings, and the goods market clearing conditions. Combining the first-order conditions for E.U. bonds to eliminate the real interest rate, ignoring the Lagrange multipliers and simplifying, we find that

ε t = I n t [ exp ( Δ c y t + 1 + Δ s t + 1 + Δ z t + 1 ) γ exp ( ε t + 1 ) ] I n t [ exp ( Δ c ^ y t + 1 + Δ s ^ t + 1 + Δ z ^ t + 1 ) γ ] , ( 33 a )

where cyt = ct – yt and cy^t=c^ty^t. Similarly, the first-order conditions for U.S. bonds imply that

ε t = I n t [ exp ( Δ c y t + 1 + Δ s t + 1 + Δ z t + 1 ) γ ] I n t [ exp ( Δ c ^ y t + 1 + Δ s ^ t + 1 + Δ z ^ t + 1 ) γ exp ( ε t + 1 ) ] . ( 33 b )

These difference equations pin down the equilibrium log real exchange rate in terms of the future growth in the endowments, surplus ratios and the consumption-output ratios, cyt and cy^t.8 They encapsulate the idea that the exchange rate acts as an asset price determined by the equilibrium in international bond markets. Of course the real exchange rate also acts as a relative price via its affects on the terms of trade. This facet is reflected in the goods market clearing conditions. Substituting for the households’ demands (i.e., CtUS=η(PtUS/Pt)θCt,CtEU=(1η)(PtEU/Pt)θCt,C^tEU=η(P^tEU/P^t)θC^t and C^tUS=(1η)(P^tUS/P^t)θC^t relative prices with the terms of trade in (25) produces

1 = η ( η + ( 1 η ) t 1 θ ) θ 1 θ exp ( c y t ) + ( 1 η ) ( η t 1 θ + ( 1 η ) ) θ 1 θ exp ( c y ^ t + z ^ t z t ) ( 34 a )

and

1 = ( 1 η ) ( η t θ 1 + ( 1 η ) ) θ 1 θ exp ( c y t + z t z ^ t ) + η ( η + ( 1 η ) t θ 1 ) θ 1 θ exp ( c y ^ t ) , ( 34 b )

where

t = { ( 1 η ) η exp ( ε t ) 1 θ ( 1 η ) exp ( ε t ) 1 θ η } 1 1 θ . ( 34 c )

Equations (33) - (34) comprise a closed system that determines the behavior of εt, cyt and from the exogenous processes for zt, ẑt, st and ŝt. Let εt=(zt,z^t,sts¯,s^ts¯) denote the solution to (33) -(34), for some some function F(·). I define the steady state value for the log real exchange rate as

ε ¯ = ( 0 , 0 , 0 , 0 ) .

In words, ε¯ is the value for log real exchange that is consistent with equilibrium in the international asset and goods’ markets when collateral constraints are not binding and when the current endowments of U.S. and E.U. goods are equal and both surplus ratios are at their long-run value. I further restrict my attention to symmetric steady states where the effects of U.S. shocks vt and et on U.S. (E.U.) variables are the same as the effects of E.U. shocks v^t and e^t on E.U. (U.S.) variables.

This definition of the steady state real exchange rate has several noteworthy features. First, the value for ε¯ depends on households’ expectations of future shocks to the endowments and surplus ratios conditioned on current steady state information {yt=y^t=𝔗t,st=s^t=s¯} via the conditional expectations on the right-hand-side of (33).9 Notice, also, that the steady state is defined with reference to the behavior of the exogenous variables, not the endogenous variables. In particular, it is the point where the distribution of {zt+1, ẑt+1, st+1, ŝt+1} conditioned on period-t information is constant. In contrast, the conditional moments of the real exchange rate depend on the form of (·). Since (·). is a nonlinear function, 𝔼t(et+1,e^t+1,ω(s¯)vt+1,ω(s¯)v^t+1) need not equal ε¯ so the expected depreciation rate in the steady state may differ from zero. Of course, in the limit as the variance of the exogenous shocks disappears, 𝔼t(et+1,e^t+1,ω(s¯)vt+1,ω(s¯)v^t+1)ε¯, so the expected deprecation rate in the steady state converges to zero. Finally, note that the steady state values for the consumption-output ratios can be computed as the solutions to (34) with εt=ε¯ and zt = ẑt = 0.

The nonlinearities (33) - (34) are too complex to find the form of (·) analytically, so (·) and hence the steady-state real exchange rate must be approximated. To do this, I use the method of undetermined coefficients. First, I conjecture that ε¯=0 and that (·) can be well-approximated by πz(zt – ẑt) + πs(st – ŝt), where πz and πs are unknown coefficients. I then take log-linear approximations to the first-order conditions governing the households’ holdings of U.S. and E.U bonds, and the goods market clearing conditions. I verify that these approximate equilibrium conditions are satisfied when εt = πz (zt – ẑt) + πs(st – ŝt) and determine the values for πz and πs in terms of the models’ parameters. This establishes zero as a candidate value for the steady state value for εt that satisfies approximate equilibrium conditions. Finally, I check that this candidate value is locally unique. The Appendix shows that if (·) is approximated by ε¯+πz(ztz^t)+πs(sts^t), the only value for ε¯ in the neighborhood of zero that solves the system of approximate equilibrium conditions is zero.

This approximation to the true value of ε¯ has a number of sensible economic implications. First, in the steady state aggregate consumption is equalized across countries (i.e., cyt=cy^t=0 solves (34) so ct = yt = 𝔗t = ŷt = ĉt). This means that trade is balanced between the two countries. By definition U.S. exports and imports are determined by E.U households’ demand for U.S. goods, and U.S. demand for E.U. goods, respectively. So, when measured in terms of the U.S. consumption basket, U.S. exports and

imports are given by

𝒳 t = ( 1 η ) ( P ^ t U S / P ^ t ) 1 θ t C ^ t = ( 1 η ) ( η 𝒳 t 1 θ + ( 1 η ) ) 1 t C ^ t a n d ( 35 a )
𝔐 t = ( 1 η ) ( P t E U / P t ) 1 θ C t = ( 1 η ) ( η 𝒳 t 1 θ + ( 1 η ) ) 1 C t . ( 35 b )

In the steady state these expressions simplify to 𝔛t = (1 – η)Ĉt and 𝔐t = (1 – η)Ct so there is a zero trade balance between the countries. The approximation also implies that real interest rates are constant and equal across countries. Since the approximation for (·) is linear, 𝔼tΔεt+1 = 0 in the steady state. Consequently, the steady state risk premium is also zero because 𝔼tΔεt+1+r^trt=δt.

Portfolio Shares Equilibrium portfolios allocations are not well-defined in the non-stochastic steady state because all financial assets have the same riskless return. This is not the case here because in the stochastic steady state households recognize that future shocks will affect the returns on individually assets differently.

I identify the portfolio shares from the households’ budget constraints and two ratios: the saving-to-consumption ratio, ΛtW=(WtCt)/Ct, and the equity price-to-dividend ratio, ΛtQ=Qt/Dt. From the U.S. first-order condition in (32) we find that

1 = β 𝔼 t [ ( C t + 1 C t ) γ ( S t + 1 S t ) γ R t + 1 W ] + t ( 1 α t F B + χ α t F B ) .

Substituting for Rt+1W from the budget constraint in (27b) and re-arranging the result gives

Λ t W = β 𝔼 t [ ( 1 + Λ t + 1 W ) ( C t + 1 C t ) 1 γ ( S t + 1 S t ) γ ] + t N t / C t . ( 36 )

Thus, the U.S. savings-to-consumption ratio depends on expectations concerning future surplus ratios and equilibrium consumption growth.10 The first-order conditions in (32) also imply that

Λ t Q = β 𝔼 t [ ( 1 + Λ t + 1 Q ) ( C t + 1 C t ) 1 γ ( S t + 1 S t ) γ exp ( Δ d c t + 1 ) ] . ( 37 )

where dct = 1n(Dt/Ct). Goods market clearing implies that Dt = Ct + 𝔛t – 𝔐t, so the log dividend-consumption ratio can be written as

d c t = I n { 1 + ( 𝔛 t 𝔐 t 1 ) 𝔐 t C t } = I n { 1 + 1 η η 𝒯 t θ 1 + ( 1 η ) ( 𝒳 t 𝔐 t 1 ) } , ( 38 )

where from (35)

𝒳 t 𝔐 t = η 𝒯 t θ 1 + ( 1 η ) η 𝒯 t 1 θ + ( 1 η ) exp ( ε t + c y ^ t c y t + z ^ t z t ) . ( 39 )

(38) and (39) imply that the equilibrium dividend-consumption ratio depends on εt,cyt,cy^tzt and t. Thus, (37) represents a difference equation in ΛtQ that can be solved given the exogenous processes for endowments and the surplus ratio and the approximate equilibrium processes for consumption-output ratio and the real exchange rate. Analogous equations determine the equity price-to-dividend and savings-to-consumption ratios in the E.U. (i.e., Λ^tQ and Λ^tW).

The ΛtQ and ΛtW ratios allow us to determine the share of equities in U.S. households’ portfolios. Since households hold the entire stock of domestic equity, the U.S. equity share is given by αtEQ=Qt/(WtCt). Combining this expression with the definitions of ΛtQ, and dct produces

α t E Q = Λ t Q Λ t W D t C t = Λ t Q Λ t W ( 1 + 𝒳 t 𝔐 t C t ) . ( 40 )

Thus, the share of equities in U.S. households’ portfolios depends on the ratios ΛtQ and ΛtW, and the net exports-to-consumption ratio. In the steady state net exports are zero, so Dt = Ct and the solutions to (36), (37) and their E.U. counterparts are constants (i.e., ΛtQ=Λ¯Q, ΛtW=Λ¯W and so on). The steady state equity shares are therefore given by α¯EQ=Λ¯Q/Λ¯W and α^¯EQ=Λ^¯Q/Λ^¯W. In practice, my approximation to the steady state produces values for Λ¯Q/Λ^¯Q,Λ¯W and Λ^¯W that are almost equal, so the steady state U.S. and E.U. equity shares are very close to unity.

To identify U.S. households’ bond holdings, I first combine the log version of the budget constraint in (27b) with the definition of ΛtW to give

Δ c t + 1 = r t + 1 w + I n Λ t + 1 w I n ( Λ t + 1 w + 1 ) . ( 41 )

I next combine this expression with an continuous-time approximation to the log return on wealth

r t + 1 w = r t + α t ʹ e r t + 1 + 1 2 α t ʹ ( d i a g ( 𝕍 t ( e r t + 1 ) ) 𝕍 t ( e r t + 1 ) ) α t , ( 42 )

where αt=[αtEQ,αtFB] is the vector of portfolio shares, ert+1=[rt+1EQrt,Δεt+1+r^trt] is a vector of log excess returns on equity and foreign bonds (measured in terms of U.S. consumption), and 𝕍t(·) is the variance conditioned on period—t information.11 Finally, I combine (38) with (42) to compute the conditional covariance between consumption growth and the real exchange rate. Re-arranging the resulting expression

α t F B = 𝕍 t ( ε t + 1 , Δ c t + 1 ) 𝕍 t ( ε t + 1 ) α t E Q 𝕍 t ( ε t + 1 , r t + 1 E Q ) 𝕍 t ( ε t + 1 ) + 𝕍 t ( ε t + 1 , I n ( Λ t + 1 W + 1 ) ) 𝕍 t ( ε t + 1 ) , ( 43 )

where rt+1EQ is the log return on U.S. equity. By definition,

rt+1EQ=ln(Λt+1Q+1)ln(ΛtQ)+Δdct+1+Δct+1, so all the terms on the right-hand-side are readily computed from the equilibrium behavior of real exchange rate, consumption, ΛtQ,ΛtW and dct. In the approximate steady state, (43) simplifies to αtFB=𝕍t(εt+1,dct+1)/𝕍t(εt+1), which is a positive constant, ᾱfb. This means that the steady state value of Nt is 𝓍α¯FBΛ¯WCt>0, so the U.S. collateral constraint does not bind. E.U. households’ bond holdings are determined from these results and the market clearing conditions in (21). In particular, the foreign bond share is a α^tFB=B^US/(tW^ttC^t)=(αtFB+αtEQ1)(Ct/tC^t). Clearly, α^tFB=α¯FB>0 in the steady state, so the E.U. collateral constraint doesn’t bind. These results confirm that we can ignore the Lagrange multipliers on the collateral constraints when computing the steady state real exchange rate as an approximate solution to (33).

Equilibrium Dynamics I use the set of second-order approximations to the households’ first-order conditions from the modified optimization problems and the market clearing conditions around the steady state to characterize the equilibrium process for the real exchange rate, consumption, real interest rates, trade flows, dividends and the ΛtQ,ΛtW,Λ^tQ and Λ^tW ratios. These processes are conditionally heteroskedastic. Recall that the sensitivity of the surplus ratios to future risk shocks varies with the current surplus ratio, so insofar as the surplus ratios affect the endogenous variables, they display conditional heteroskedasticity. As a consequence, time-varying conditional second moments are a source of variation in the foreign exchange risk premium and in households’ savings and portfolio decisions. The appendix provides a complete list of the approximations used to derive the equilibrium dynamics.

4 Results

This section examines whether the model can account for the behavior of real exchange rates and other macro variables. I parameterize the model so that habits exhibit behavior similar to that found in other studies and the variance of the equilibrium real depreciation rate, real interest and consumption growth differentials match estimates from actual data. I then study the roles played by endowment and risk shocks as drivers of real exchange rates and other macro variables. This analysis address three key questions. First, can a model that incorporates both endowment and risk shocks account for observed behavior of exchange rates and other macro variables? Second, are risk shocks an important driver of exchange rates? Third, do risk shocks have significant macro effects? As we shall see, the analysis provides an affirmative answer to all three questions.

4.1 Parameterization

The model contains 14 parameters: the preference parameters, β, γ, η and θ; the parameters governing habits, φ, s¯, smax and ω; the parameters of the endowment processes, ρ, g, σe2 and σu2 the collateral constraint, χ, and the barrier parameter, μ. I assign values to a first subset of these parameters that appear elsewhere in the literature. The values of a second subset are calibrated to key ratios, and a final subset are chosen so that the model matches moments in the data. This hybrid approach strikes a balance between two goals. On one hand I want some aspects of the model to be comparable with others in the literature, so I assign values to many of the preference and habit parameters that have been used elsewhere. On the other, my aim is to investigate whether the model can account for the behavior of exchange rates, so the values of the other parameters are chosen to match important moments in the data. The values of all the parameters are summarized in Table 4.

Table 4:

Parameterization

article image
Notes: Parameter values that are chosen to match moments in the data are denoted by . * expressed in per cent per quarter.

The model is parameterized so that one period corresponds to one quarter. β is set equal to 0.99, while γ and η are assigned standard values of 2 and 0.85, respectively, so households have a strong bias towards the consumption of domestic goods. The value for the long run growth rate, g, is chosen so that the steady state real interest rate in both countries equals 1.5 per cent (per year).

Let σs2 denote the unconditional variance of st and ŝt. The surplus processes in (13) and (17) imply that σs2=ω(smaxs¯)/(1Φ2). I set φ equal to 0.92 and s¯=ln(S¯) equal to ln(0.05) so that the average consumption surplus ratio is 5 percent. The upper bound on the consumption surplus ratio smax = ln (Smax) is determined as σs2(1Φ2)/ω+s¯, where the values for σs2 and φ are chosen to match the moments described below. This produces a value for Smax of 5.5 per cent.

I set the values of four parameters to match moments in the data: (i) the variance of the real depreciation rate for the USD verses the EUR, (ii) the variance in the per capita consumption growth differential between the US and Euro area, (iii) the variance of the real interest differential between the US and Euro area, and (iv) the first-order autocorrelation in the real interest differential. Sample moments are calculated at the quarterly frequency from data spanning 1990:I to 2007:IV (132 observations). Real interest rates are computed as the fitted values from an AR(2) regression for the ex post real return on Eurodeposits (i.e., the 3-month nominal Eurodeposit rate minus realized inflation). I choose the values for σs2, ω, ρ and σe2 so the unconditional moments computed from the equilibrium of the model match the four sample moments. This procedure produces values for ω of 0.148. The implied semi-elasticity of the real interest differential with respect to variations in st – ŝt is 0.012. This is very close to the value of 0.1 used in Verdelhan (2010).12

In actual economies the relative prices of domestic- and foreign-produced consumer goods are relatively unresponsive to quarterly variations in spot exchange rates because the effects are absorbed by the production and distribution sectors. These sectors are absent in this simple model. Consequently, variations in the real exchange rate are directly reflected in the relative prices that drive households’s consumption decisions. To compensate for this feature, I treat θ as a composite parameter, θ*(1 – ς), where ς denotes the fraction of exchange rate variations absorbed by the un-modeled production and distribution sectors, and θ* is the “true” elasticity of substitution. Setting θ* equal to 0.72, as in Hnatkovska (2010) and Corsetti, Dedola, and Leduc (2008), and ς equal to 0.85, gives a value for θ of 0.11.13 Again, I discuss the robustness of my main results to alternative values for θ below.

The remaining parameters are χ and μ. Because the foreign asset and liability portfolios of actual countries contain more than the default-free debt included in the model, there is no simple and direct way to calibrate either of these parameters. Instead, I choose values for χ and μ that imply “reasonable” restrictions on the degree of international borrowing. χ determines the upper bound on the ratio of foreign liabilities to assets that a country can accumulate. In U.S. case, the constraint implies that BtUS/tBtEU<1+𝓍, so the upper bound is 1 + χ. These limits are readily translated into an upper bound on the net foreign liability to income ratio for each country along the steady state growth path. I set χ equal to 0.3, which implies an upper bound of 200 percent. Since actual debt to GDP ratios rarely approach these levels without any perceived risk of default, this choice for χ places a rather weak restriction on international borrowing in the model. In the appendix I show that the value for μ determines the semi-elasticity of the risk premium with respect to variations in the log ratio of foreign liabilities to assets. I set μ equal to 0.03. in the baseline parameterization, and consider the robustness of the equilibrium to alternate values.

4.2 Model Moments

Table 5 provides a comparison of key moments computed from the equilibrium of the model against estimates computed from U.S. and Euro-area data. Panel A shows that when the model is solved using the parameter values from Table 4, the variance of the real depreciation rate, consumption growth differential and real interest differential match the sample variances estimated in the data. Notice that the variance of the real depreciation rate is approximately four times larger than the variance of the consumption growth differential, which in turn is 30 percent larger than the variance of the interest differential. The model accounts for these differences via the influence of the the risk shocks.

Table 5:

Comparison of Data and Model Moments

article image
Notes: Matched moments are indicated by .

Panel B of Table 5 compares the autocorrelation properties of the real interest differential, depreciation rate and consumption growth differential. Recall that the parameters were not chosen to match the latter two autocorrelations, so a comparison is informative about the ability of the model to replicate these features of the data. As the table shows, the model has no trouble replicating the lack of serial correlation in the real depreciation rate because risk-shocks are the dominant drivers of the real depreciation rate and there is little serial correlation in Δst and Δŝt.

The consumption growth differential displays a greater degree of serial correlation in both the data and the model. To understand why, consider the following equation derived from first-order approximations to the goods market clearing conditions in (35)

Δ c t Δ c ^ t = ( 2 φ 1 ) ( Δ y t Δ y ^ t ) 4 θ ( 1 η ) φ Δ ε t , ( 44 )

where φ = η/(2η – 1) > 0. Since the model produces little autocorrelation in the real depreciation rate, serial correlation in Δyt – Δŷt is the prime source of serial correlation in the consumption growth differential. Indeed, the value for ρ of 0.77 implies autocorrelation in Δct – Δĉt equal to -0.11 when the depreciation rate is serially uncorrelated.

Panel C of Table 5 compares the exchange-rate behavior in the model and data along two key dimensions. The first line compares the sample correlation between the real depreciation rate and the consumption growth differential computed from US and Euro-area data with the unconditional correlation computed from the model. Under complete markets, the real depreciation rate must match the difference between the growth in U.S. and E.U. marginal utility: i.e.,

Δ ε t = γ ( Δ c t Δ c ^ t ) + γ ( Δ s t Δ s ^ t ) .

Clearly, there must be a positive correlation between the depreciation rate and the consumption growth differential if variations in the surplus differential are absent. Backus and Smith (1993) first pointed to this discrepancy between the negative sample correlations found across many country pairs and the theoretical correlation implied by a complete markets model where households have isoelastic, time-separable utility. Here the presence of incomplete markets and risk shocks break this simple link, producing a strongly negative correlation of -0.41.

The second row of Panel C compares the slope coefficient from the Fama regression for the real USD/EUR reported in Table 3, with the theoretical value implied by the model. As the table shows, the theoretical value is negative but above the estimate of -2.99 computed from the USD/EUR data. Since the model is calibrated to match the variance of the real interest differential, this difference reflects a discrepancy between the value of ℂ𝕍(δt,rtr^t) in the model and its sample counterpart. Variations in the risk premium covary negatively with the interest differential but not strongly enough to produce a coefficient of -2.99.14 I examine the mechanism driving variations in the risk premium and interest differential below.

4.3 Identifying Dark Matter

Let us now turn to the central issue: Can the model replicate the plots of the estimated variance ratios for the G-7 currencies in Figure 1? Recall that hr identifies the fraction of the variance in the h-period depreciation rate that can be attributed to variations in the interest differential, while hrU identifies the fraction attributable to news concerning future differentials. Figure 2 plots the values of hr and hrU for horizons of 1 to 20 quarters computed from the equilibrium real exchange rate and interest differential processes implied by the model. Clearly, the plots have the same general shape as the estimates for the G7 currencies in Figure 1. More specifically, Figure 2 shows that real interest differentials are a minor (proximate) driver of real depreciation rates in the model, with hr falling from 15 to 13 per cent as the horizon rises from one to 20 quarters. This ratio is comparable to the short-horizon estimates of hr for the USD/CAN and USD/JPY in Table 2, but is well above the estimates for other currencies such as the USD/GBP and USD/EUR. Figure 2 also shows that news concerning future interest differentials is comparatively more important as a driver of real depreciation rates at short horizons. The values for hrU fall more quickly than hr as the horizon increases, but they do not fall to the estimated values for hrU in the G7 currencies reported in Table 2.

Figure 2:
Figure 2:

Plots of hr (solid) and hrU (dashed) implied by the model

Citation: IMF Working Papers 2012, 066; 10.5089/9781463938437.001.A001

The general message conveyed by Figure 2 is clear. In this model variations in interest differentials are not the main (proximate) driver of depreciation rates. More precisely, endowment and risk shocks affect equilibrium real interest rates, but these effects play a minor role in the determining how exchange rates respond to the shocks. Instead, variations in exchange rate rates are primarily driven the effects endowment and risk shocks have on current and future risk premia. Indeed, in this model there is a unique steady-state real exchange rate so variations in the risk premia must account for all the effects of exchange-rate dark matter.

4.4 Dark Matter and Macroeconomics

I now examine whether the risk shocks needed to account for these exchange-rate moments have significant macroeconomic implications. For this purpose, I first compare the transmission of endowment and risk shocks to exchange rates and other macroeconomic variables in equilibria with different degrees of risk-sharing. I then examine the relative importance of risk and endowment shocks as drivers of exchange-rate and macroeconomic variations.

Analyzing the effects of endowment and risk shocks is complicated by the presence of incomplete markets and the collateral constraints. It therefore proves useful to compare the impulse responses of different shocks with their counterparts in an equilibrium where markets are complete and the collateral constraints are absent. The appendix shows that this equilibrium can be computed as a special case where the barrier parameter μ equals zero.

Endowment Shocks

Figure 3 shows the impulse responses of the real exchange rate, consumption, real interest rates and the risk premium following a one standard deviation positive shock to the U.S. endowment process.

Figure 3:
Figure 3:

Impulse Responses to a Positive U.S. Endowment Shock

Citation: IMF Working Papers 2012, 066; 10.5089/9781463938437.001.A001

Notes: The plots show the response of each variable to a one standard deviation positive shock to the U.S. endowment process. The vertical axis in each plot shows the response per one percent of the shock. Responses from the complete markets version of the model (without collateral constraints) are indicated by plots with bullets. In panels B and C, U.S. and E.U. variables are identified by the solid and dashed plots, respectively. The horizontal axis measures the time elapsed since the shock in quarters.

Overall, the plots show that incomplete risk-sharing and the borrowing constraints have little effect on how the economy responds to the effects of the endowment shock.15 In both versions of the model there is a real depreciation, and rise (fall) in U.S. (E.U.) consumption and a fall (slight rise) in U.S. (E.U.) interest rates. The only qualitative difference appears in the behavior of the risk premium, which rises very slightly in the incomplete markets equilibrium while remaining unchanged when markets are complete.

The economics behind these plots is straightforward. At pre-existing consumption levels, the positive shock to the U.S. endowment requires a deterioration in the U.S. terms of trade (i.e., a fall in PtUS/PtEU) to maintain goods market clearing. Since this, in turn, implies a real depreciation of the dollar, under complete risk sharing there must also be arise in relative consumption, Ctt, to maintain the equality of marginal utility across countries. Panel B in Figure 3 shows that this is achieved by a larger rise in U.S. consumption than the fall in E.U. consumption because the former has a larger impact on the demand for U.S. goods in the presence of home-bias (η > 1/2). This asymmetry carries over into real rates. Panel C shows that the U.S. real rate falls further than the rise in the E.U. rate because expected consumption growth in the U.S. is much lower than in the E.U. until the effects of the shock dissipate.

The response of the economy under incomplete markets is very similar. To understand why, it is useful to return to the accounting identity linking the real exchange rate to interest rates and the risk premium in equation (2). Since εt = 0 in the steady state, the identity implies that

ε t = 𝔼 t Σ i = 0 { r ^ t + i r t + i } 𝔼 t Σ i = 0 δ t + i . ( 45 )

We can approximate the terms on the right-hand-side from the households’ first-order conditions as

r t r ^ t = γ t [ Δ c t + 1 + Δ s t + 1 ] γ t [ Δ c ^ t + 1 + Δ s ^ t + 1 ] + 1 2 γ 2 { t ( c t + 1 + s t + 1 ) t ( c ^ t + 1 + s ^ t + 1 ) } + μ ( n t n ^ t ) , and ( 46 )
δ t = 1 2 γ 𝕍 t ( c t + 1 + c ^ t + 1 , ε t + 1 ) 1 2 γ 𝕍 t ( s t + 1 + s ^ t + 1 , ε t + 1 ) + 1 2 μ χ ( n t n ^ t ) . ( 47 )

Substituting these expressions into (45) and simplifying, produces

ε t = γ ( c t c ^ t ) + γ ( s t s ^ t ) + 𝔼 t Σ i = 0 χ t + i , w h e r e ( 48 )
χ t = 1 2 γ 2 { 𝕍 t ( c t + 1 + s t + 1 ) 𝕍 t ( c ^ t + 1 + s ^ t + 1 ) } 1 2 γ 𝕍 t ( s t + 1 + s ^ t + 1 , ε t + 1 ) 1 2 μ ( 2 + χ ) ( n t n ^ t ) . ( 49 )

Thus, the log real exchange rate is pushed away from the level that equates marginal utility across countries when 𝔼tΣi=0xt+i differs from zero. Endowment endowment shocks have no effect on the conditional variance of future consumption or the surplus ratios, so the first two terms on the right-hand-side of (49) equal zero and χt is determined by the effects of the collateral constraints. Recall that the collateral constraints facing U.S. and E.U. households take the form of Nt ≥ 0, so ntn^t=ln(Nt/N^t) rises as E.U. households move closer to their constraint and/or U.S. households move away from theirs. This is exactly what happens following the U.S. endowment shock because it raises the wealth of U.S. households and lowers the wealth of E.U. households. Indeed Panel D of Figure 3 shows that this induces a rise in the risk premium, but the effect is very small. E.U. households move towards their collateral constraint, but nowhere near the point where it binds. Consequently, although 𝔼tΣi=0xt+i is negative immediately following the endowment shock, the gap between εt and γ(ct – ĉt) is economically insignificant.

In sum, therefore, the presence of the collateral constraints does affect how the real exchange rate responds to the endowment shock, but the effects are very small because households remain well away from the point where the constraints bind. As we shall see, this similarity in the behavior of exchange rates under complete and incomplete markets settings breaks down when we examine the effects of risk shocks.16

Risk Shocks

Figure 4 plots the impulse responses of exchange rates, consumption, interest rates and the risk premium to a risk shock that lowers the U.S. surplus ratio from it initial steady state value by one standard deviation. This shock makes U.S. households more risk averse; increasing the local curvature of their utility by approximately 6.5 per cent. Unlike Figure 3, the plots in Figure 4 show that incomplete risk-sharing and the collateral constraints have a large effect on how the economy responds to the shock.

Figure 4:
Figure 4:

Impulse Responses to a U.S. Risk Shock

Citation: IMF Working Papers 2012, 066; 10.5089/9781463938437.001.A001

Notes: The plots show the response of each variable to a one standard deviation negative shock to the U.S. log surplus ratio. Responses are measured per one percent of the shock. Responses from the complete markets version of the model without borrowing constraints are indicated by plots with bullets. In panels B and C, U.S. and E.U. variables are identified by the solid and dashed plots, respectively. The horizontal axis measures the time elapsed since the shock in quarters.

Once again, let us first consider the response of the economy under complete markets. At pre-existing consumption levels, the risk shock raises the marginal utility of U.S. households so there must be an immediate appreciation in the real exchange rate to share risk across countries. This appreciation also induces an improvement in the U.S. terms of trade so, in the presence of home bias, there must be a rise in U.S. consumption and fall in E.U. consumption to clear goods markets. Panel B shows that these responses imply a fall (rise) in expected future U.S. (E.U.) consumption growth following the shock.

The response of real interest rates and the risk premium are depicted in Panel C. The households’ first-order conditions imply that real interest rates are well-approximated by

r t = I n β + γ 𝔼 t Δ c t + 1 + γ 𝔼 t Δ s t + 1 1 2 γ 2 𝕍 t ( c t + 1 + s t + 1 ) , a n d ( 50 a )
r ^ t = I n β + γ 𝔼 t Δ c ^ t + 1 + γ 𝔼 t Δ s ^ t + 1 1 2 γ 2 𝕍 t ( c ^ t + 1 + s ^ t + 1 ) . ( 50 b )

Risk shocks affect interests rates indirectly via consumption growth, and directly via the last two terms on the right-hand-side of each equation. In particular, the negative U.S. risk shock raises both γ𝔼tΔst+1 and γ2𝕍t(ct+1 + st+1) because U.S. households anticipate a future rise in the log surplus ratio and greater volatility in marginal utility. These effects act on the equilibrium real interest rate in opposite directions. The rise in γ𝔼tΔst+1 puts upward pressure on the real interest rate because households want to borrow more, while in the increase in γ2𝕍t(ct+1 + st+1) induces greater precautionary saving. In this calibration of the model risk-shocks are very persistent (φ = 0.92), so the rise in γ𝔼tΔst+1 is small and the precautionary savings channel dominates. Consequently, as Panel C shows, the risk shock drives down U.S. interest rates. Precautionary saving also exerts downward pressure on the E.U. rate via a rise in γ2𝕍tt+1 + ŝt+1), but the effect is dominated by the increase in 𝔼tΔĉt+1 induced by goods market clearing and risk sharing. As a result there is a very small rise in rt. The combined effect is a fall in the interest differential, rtr^t, of 11 basis points per one percent of the risk-shock.

Panel D shows that the U.S. risk-shock has a much larger effect on the risk premium; it rises by more than twice the fall in the interest differential. The reason for this rise is apparent from the responses in Panels A and B. There we saw that market clearing induced a real appreciation in the dollar but little change in total consumption, ct + ĉt. So, when risk shocks are the dominant source of exchange-rate variations, ℂ𝕍(ct+1 + ĉt+1, εt+1) is close to zero and the equation for the risk premium in (47) simplifies to

δ t = 1 2 γ 𝕍 t ( s t + 1 + s ^ t + 1 , ε t + 1 ) .

The plots in Panel A imply that εt is positively correlated with st – st, so the covariance on the right is proportional to 𝕍t(st+1) – 𝕍tt+1). When the risk shock hits, st falls and 𝕍t(st+1) rises, so the risk premium jumps upward. Intuitively, the risk-shock makes E.U. bonds less attractive to U.S. households as a hedge against future unexpected changes in the real exchange rate, so the equilibrium risk premium (i.e., expected excess return) has to rise to compensate. Notice that this rise more than offsets the fall in the interest differential so the equilibrium expected depreciation rate, 𝔼tΔεt+1=rtr^t+δt, increases immediately following the shock in a manner consistent with the response of the real exchange rate show in Panel A.

The economy responds to risk shocks in an entirely different manner when markets are incomplete and households face collateral constraints. In particular, Figure 4 shows that the same U.S. risk shock induces a real depreciation of the dollar, a fall in the risk premium and relative consumption. To understand the source of these differences, consider first the direct effects of the shock on the value of U.S. equites, Qt. Recall that Qt=ΛtQDt where ΛtQ satisfies (37). Inspection of this equation reveals that ΛtQ must fall as the risk-shock hits even when the future paths for consumption and dividends remain unchanged. Intuitively, since the shock increases the risk aversion of U.S. households, market clearing requires that the expected return on equity must rise in compensation so there is an immediate fall in Qt. The risk shock also affects household saving. Equation (36) shows that Λtw=(WtCt)/Ct falls by the same amount as ΛtQ. This means that U.S. households reduce their savings by the same amount as their capital loss on equities so αtQ remains at one and Nt=(1αtQ+𝓍αtFB)(WtCt)=𝓍αtFBQt falls towards the lower bound of zero via the capital loss on equities.17 In sum, therefore, the direct effect of the risk shock is to push U.S. households towards their collateral constraint.

The indirect effects of risk shock now come into play. In particular, U.S. households’ demand to hold E.U. bonds rather than U.S. bonds rises because the former are more valuable as collateral. This portfolio shift puts downward pressure on the equilibrium risk premium. So, ceteris paribus, the equilibrium real exchange rate must jump to a path consistent with future appreciation, like the path shown in the Panel A of Figure 4. This triggers an immediate deterioration in the U.S. terms of trade, so U.S. consumption falls and E.U. consumption rises to clear the goods markets, as shown in Panel B.

These adjustments of the exchange rate and consumption have several further consequences. First, the rise in εt reduces the real value of U.S. dividends because Dt=(PtUS/Pt)Yt and the depreciation lowers the relative price of U.S. goods. As a result, the rise in et magnifies the size of the capital loss U.S. households suffer on their equity holdings. The rise in εt also produces a capital gain for E.U. households on their equity holdings because it raises the value of dividends, D^t=(P^tEU/P^t)Y^t, via an increase in the relative price of E.U. goods.18 These revaluation effects push U.S. households towards and E.U. households away from their respective collateral constraints.

The second set of consequences concern the behavior of real interest rates. In the presence of the collateral constraints, equilibrium interest rates are approximated by

r t = I n β + γ 𝔼 t Δ c t + 1 + γ 𝔼 t Δ s t + 1 1 2 γ 2 𝕍 t ( c t + 1 + s t + 1 ) + μ ( n t n ¯ t ) , a n d ( 51 a )
r ^ t = I n β + γ 𝔼 t Δ c ^ t + 1 + γ 𝔼 t Δ s ^ t + 1 1 2 γ 2 𝕍 t ( c ^ t + 1 + s ^ t + 1 ) + μ ( n ^ t n ¯ t ) . ( 51 b )

Under complete markets, the risk shock has offsetting effects on the U.S. interest rate via an increase in 𝔼tΔst+1 and 𝕍t (ct+1 + st+1). In this equilibrium there is also a fall in nt and a rise in 𝔼tct+1 induced by goods market clearing. Panel C of Figure 4 shows that the feedback effect on expected consumption growth dominates so the risk shock raises the U.S. real interest rate. The risk shock affects the E.U. interest rate through three channels. First, goods market clearing implies that 𝔼tΔĉt+1 < 0 following the shock. Second, the fall in st implies greater volatility in the future exchange rate, so 𝕍t(ct+1 + st+1) rises because E.U. consumption is partially driven by changes in the terms of trade. Third, n^t rises as the valuation effects pull E.U. households away from their collateral constraint. Panel C shows that this last channel dominates. E.U. interest rise following the U.S. risk shock by almost as much as U.S. interest rates.

Final, we turn to the risk premium. As in the complete markets case, risk shocks induce insignificant variations in ct + ĉt so (47) simplifies to

δ t = 1 2 γ 𝕍 t ( s t + 1 + s ^ t + 1 , ε t + 1 ) + 1 2 μ χ ( n t n ^ t ) .

Risk shocks affect the risk premium via two channels: a borrowing channel identified by a change in ntn^t, and a hedging channel identified by a change in ℂ𝕍t(st+1 + ŝt+1, εt+1). As noted above, the effect of the risk shock on the value of U.S. equities pulls U.S. households towards their collateral constraint so nt falls and the risk premium is pushed below zero. This direct effect on the risk premium is amplified in two ways. First the valuation effects of the real depreciation raise n^t and push nt lower as E.U. households move further from their constraint while U.S. households are pulled closer. Second, the risk shock makes E.U. bonds a better exchange-rate hedge. Households recognize that the transmission of the U.S. risk shock that lowers st also leads to a real depreciation, or, more generally, induce a negative correlation between εt and ŝt – ŝt. This means that the covariance term is proportional to 𝕍tt+1) – 𝕍t(st+1) = ω(st – ŝt). When st falls following the U.S. risk shock, households understand that E.U. bonds have become a better hedge against future unexpected exchange-rate variations, so the equilibrium risk premium must fall to compensate.

There are three important points to take away from this discussion: First, incomplete risk-sharing and the collateral constraints play an important role in the transmission of risk shocks to exchange rates and other variables. Risk shocks affect the exchange rate because the capital loss of U.S. equities pushes U.S. households towards their constraint. If the constraints were absent, there would be no need for the risk premium to adjust so the effects of the shock would not be transmitted internationally via the depreciation of the exchange rate. Similarly, if households had access to an array of assets that permitted complete risk-sharing, the exchange rate would simply adjust to clear goods markets and equate marginal utilities so there would be little role for the risk premium.

The second point concerns the behavior of consumption and habits. Under complete markets, risk shocks make households’ habits more volatile than consumption. To see why, I use the identity ht = ht – ct + ct to write

𝕍t (ht+1) = 𝕍t (ht+1 – ct+1) + 2ℂ𝕍t (ht+1 – ct+1, ct+1) + 𝕍t (ct+1).

By definition ht – ct = ln[1 – exp(st)], so we can rewrite this expression as

𝕍 t ( h t + 1 ) 𝕍 t ( c t + 1 ) = 𝕍 t ( ln [ 1 exp ( s t + 1 ) ] ) + 2 𝕍 t ( ln [ 1 exp ( s t + 1 ) ] , c t + 1 ) ( S ¯ 1 S ¯ ) 2 𝕍 t ( s t + 1 ) 2 S ¯ 1 S ¯ 𝕍 t ( s t + 1 , c t + 1 ) .

Under complete markets, an increase U.S. households’ risk aversion lowers st and leads to a domestic consumption boom via an improvement in the terms of trade. More generally, risk shocks produce a negative covariance between consumption and the surplus ratio, so the last term on the right-hand-side is positive and 𝕍t (ht+1) > 𝕍t (ct+1). It is hard to square this implication with the idea that habits respond slowly to consumption. Indeed, it directly contradicts the assumption in standard habit specifications, such as CC, where consumption is exogenous. In contrast, risk shocks induce a positive covariance between the surplus and consumption ratio when markets are incomplete, so habits display less volatility than equilibrium consumption.

The third point concerns the behavior of interest rates and the risk premium. In both versions of the model risk shocks generate a larger response from the risk premium than from the real interest differential, rtr^t, and the responses are in the opposite directions. This means that variations in the risk premium are the dominant force changing the expected depreciation rate, and by extension the real exchange rate. It also means that the population value for the slope coefficient in the real U.I.P regression (9), β1, is negative in both versions of the model (β1 equals -1.424 and -1.015 under incomplete and complete markets, respectively). The behavior of individual interest rates is quite different. Under complete markets, the U.S. risk shock lowers the domestic interest rate but leaves foreign interest rates unaffected. As in Verdelhan (2010), greater risk aversion among U.S. households pushes down the U.S. real interest rate via precautionary saving, but here the effect is magnified by an expected fall in domestic consumption growth. In contrast, an increase in U.S. risk-aversion induces an increase in both U.S. and E.U. real interest rates when markets are incomplete. The key difference here is that U.S. households expect consumption to grow in the future as the U.S. terms of trade improve, so the desire to smooth consumption dominates the effects of precautionary saving and the collateral constraint. Intertemporal smoothing and precautionary saving also affect E.U. interest rates, but here the wealth effects dominate by pushing E.U. households further away from their collateral constraint.

Variance Decompositions

Figures 3 and 4 showed how endowment and risk shocks were transmitted to exchange rates and other marco variables in environments with different degrees of risk sharing. I now examine the relative importance of risk and endowment shocks as drivers of exchange-rate variations and the dynamics of macro variables. For this purpose I calculate the variance ratios 𝕍(xt|σe2=0)/𝕍(xt), where 𝕍(xt|σe2=0) denotes the unconditional variance of variable xt computed from the equilibrium of the model in the absence of endowment shocks (i.e., in an equilibrium when their variance, σe2, is zero), and 𝕍(xt) denotes the variance when both endowment and risk shocks are present. This variance ratio measures the fraction of the variability in xt that can be attributable to risk shocks.

Column (a) of Table 6 reports the variance ratios for the variables listed in the left-hand column computed from the equilibrium with incomplete markets and collateral constraints. The variance ratios in the other columns are computed from equilibria that use the benchmark values for all the parameters (from Table 4) except the parameter shown at the head of each column. A comparison of the ratios in column (a) with those in columns (b) -(h) reveals the degree to which the variance contribution of risk-shocks is robust across alternative parameterizations. In particular, there is full risk-sharing when μ = 0, so column (b) shows the contribution of risk-shocks when markets are complete. Columns (c) and (d) show the effects of reducing the values of the barrier and collateral parameters from their benchmark levels of μ = 0.03 and χ = 0.3, while columns (e) and (f) show the effect of different specifications for households preferences. Finally, columns (g) and (f) report the variance ratios computed in equilibria with different specifications for the endowment processes. In column (g) I report the effect of raising the AR coefficient, ρ, to 0.95 from its benchmark level of 0.77. This change makes endowment shocks more persistent that risk shocks. In column (h) I show the effect of doubling the standard deviation of endowment stocks.

Table 6:

Variance Decompositions

article image
Notes: The table reports the fraction of the unconditional variance attributable to risk shocks for each of the variables listed in the left-hand column: 𝕍(x|σe2=0)/𝕍(x). The variance ratios reported in column (a) are computed from the incomplete markets equilibrium with collateral constraints using the benchmark parameter values reported in Table 4. The ratios in columns (b) - (h) are computed from the equilibrium with benchmark values for the parameters except the one shown at the head of each column. ct – 𝔗t denotes the cyclical component of U.S. aggregate consumption.

Three key features of the table stand out. First, risk shocks are the overwhelmingly dominant driver of real change rate variations across all variants of the model. In all but two cases, the variance ratios reported in row (i) are very close to one. The two exceptions occur in columns (d) and (h). The ratio in column (d) shows that risk shocks play a somewhat reduced role when foreign bonds are less valuable as collateral (i.e., when χ is smaller). In this case, risk shocks have smaller direct effects on the risk premia as households respond to capital gains and loss on the equity holdings, so their ultimate impact on the real exchange rate is reduced. Increasing the variance of the endowment shocks reduces the contribution of risk shocks to the volatility of depreciation rates for obvious reasons. Nevertheless, the ratio in column (h) shows that the variance of endowments shocks would have to be a great deal larger than in the benchmark parameterization before risk shocks cease to be the dominate driver of the deprecation rate.

The second feature concerns the contribution of risk shocks to the variability of real trade flows. In row (ii) we see that risk shocks are the dominant driver of variations in the log ratio of exports to imports across all the model variants. To a first-order approximation,

ln (𝔛t/𝔐t) = [1 – 2φ(1 – θ)]εt – (ctĉt),

so trade flows reflect variations in the real exchange rate (terms of trade) and the consumption differential. If real exchange rates are much more volatile than relative consumption (as they are in the data and the model variants), and risk-shocks account for most exchange rate volatility, then they must also be the dominant driver of trade flows.

Finally, rows (iii) - (vi) of Table 6 show that the risk shocks have substantial macroeconomic effects, they are the dominant drives of the consumption growth and real interest differentials, real interest rates and the cyclical component of U.S. consumption, ct – 𝔗t, across most model variants. Again, the notable exception appears in column (d). When foreign bonds are less valuable as collateral the international transmission of risk shocks via the risk premia is dampened, so the effects are absorbed by interest rates rather than domestic consumption and the consumption differential.

5 Conclusion

The main message of this paper is very simple. Variations in current and expected future real interest differentials have played a very minor role as the proximate determinant of the changes in real exchange rates for major currencies over short- and medium-term horizons in the post-Bretton Woods era. Instead, exchange-rate dark matter has been the dominate driver of real depreciation rates through its affects on expected excess returns and/or the expected long-run real exchange rate. To understand the nature of this dark matter, I developed a novel open-economy DSGE model in which the risk shocks driving households’ habits worked in conjunction with collateral constraints and incomplete markets. The model not only shows that risk shocks can account for the role of dark matter in real exchange-rate dynamics, but also that these same shocks have significant macroeconomic implications. This analysis suggests that exchange rates appear disconnected from traditional fundamentals because they are particularly susceptible to risk shocks that play an important role in international macroeconomics.

Finally, let me offer a some perspective on these results. First, my empirical analysis in Section 1 used VARs to estimate variations in expected future real rate differentials, rather than data on agents’ forecasts. Thus, it is possible that my analysis over-estimates the contribution of dark matter because agents’ actual forecasts for future real interest differentials were varying far more than one could identify from any VAR. However, if this were really the explanation for my empirical results, we would be left to wonder what was making agents’ interest-rate forecasts so volatile. Remember that according to my calculations dark matter accounts for approximately 90 percent of the variance in real depreciation rates at a five-year horizon, so adding a little more volatility to agents’ interest-rate forecasts will not eliminate the role of dark matter.

The second perspective concerns the structure of the DSGE model. Following CC, the model is reversed-engineered to surmount some of the known pitfalls of existing open-economy models, such as their failure to replicate the Backus-Smith and Real UIP Puzzles. A model that could not account for these long-standing exchange-rate puzzles would be of little use in understanding the forces driving exchanges rates and macroeconomic variables. At the same time, the model does not provide any micro foundations for the assumption that all households within a country are subject to the same risk shock. This modeling approach is very much in line with the asset-pricing literature, but clearly there is more work to be done here. The model also abstracts from many other features; such as production, price-setting, nontraded goods, a government or financial institutions. Adding these features to the model is conceptually straightforward, but they would have obscured my purpose here. More importantly, adding these features to the model would give greater scope for risk shocks to affect real macroeconomics activity via channels like the financial accelerator. Such a model would also provide some entirely new conceptual space for analyzing macro-prudential risk management, capital controls and international macroeconomic policies.

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Appendix.

This appendix describes the procedure I use to compute the equilibrium process for the real exchange rate and other variables. The procedure adapts the two-step solution method in Lombardo and Sutherland (2007) to the set of second-order and continuous-time approximations of the model’s equilibrium conditions. First I summarize these equations. I then present the approximations and describe the solution method.

Equilibrium Conditions

The model’s equilibrium conditions comprise the households’ first-order conditions, the market clearing conditions and the exogenous processes for the endowments and consumption surplus ratios. The first-order conditions for the U.S. and E.U. households are:

1 = β 𝔼 t [ ( C t + 1 C t ) γ ( S t + 1 S t ) γ R t + 1 EQ ] , ( 52 a )
1 = β 𝔼 t [ ( C t + 1 C t ) γ ( S t + 1 S t ) γ t + 1 R ^ t t ] + ( 1 + χ ) t ( 52 b )
1 = β 𝔼 t [ ( C t + 1 C t ) γ ( S t + 1 S t ) γ R t ] + t , ( 52 c )
1 = β 𝔼 t [ ( C ^ t + 1 C ^ t ) γ ( S ^ t + 1 S ^ t ) γ R ^ t + 1 EQ ] ( 53 a )
1 = β 𝔼 t [ ( C ^ t + 1 C ^ t ) γ ( S ^ t + 1 S ^ t ) γ t R t t + 1 ] + ( 1 + χ ) ^ t and ( 53 b )
1 = β 𝔼 t [ ( C ^ t + 1 C ^ t ) γ ( S ^ t + 1 S ^ t ) γ R ^ t ] + ^ t . ( 53 c )

where

t = μ ( C t S t C ¯ t S ¯ ) γ { N ¯ t N t 1 } and ^ t = μ ( C ^ t S ^ t C ¯ t S ¯ ) γ { N ¯ t N ^ t 1 } .

I use (52a) and (53a) to identify the ratios of equity prices to dividends, ΛtQ=Qt/Dt and Λ^tQ=Q^t/D^t:

Λ t Q = β 𝔼 t [ ( C t + 1 C t ) γ ( S t + 1 S t ) γ ( Λ t + 1 Q + 1 ) D t + 1 D t ] and ( 54 a )
Λ ^ t Q = β 𝔼 t [ ( C ^ t + 1 C ^ t ) γ ( S ^ t + 1 S ^ t ) γ ( Λ ^ t + 1 Q + 1 ) D ^ t + 1 D ^ t ] . ( 54 b )

The savings-to-consumption ratios, Λtw=(WtCt)/Ct and Λ^tw=(W^tC^t)/C^t, are determined by

Λ t W = β 𝔼 t [ ( C t + 1 C t ) 1 γ ( S t + 1 S t ) γ ( Λ t + 1 W + 1 ) ] + t N t / C t and ( 55 a )
Λ ^ t W = β 𝔼 t [ ( C ^ t + 1 C ^ t ) 1 γ ( S ^ t + 1 S ^ t ) γ ( Λ ^ t + 1 W + 1 ) ] + ^ t N ^ t / C ^ t . ( 55 b )

Goods market clearing requires that

Y t = η ( η + ( 1 η ) 𝒯 t 1 θ ) θ 1 θ C t + ( 1 η ) ( η 𝒯 t 1 θ + ( 1 η ) ) θ 1 θ C ^ t , and ( 56 a )
Y ^ t = ( 1 η ) ( η 𝒯 t θ 1 + ( 1 η ) ) θ 1 θ C t η ( η + ( 1 η ) 𝒯 t θ 1 ) θ 1 θ C ^ t , ( 56 b )

while market clearing in the equity and bond markets requires that

α t Q = Q t / ( W t C t ) , α ^ t Q = Q ^ t / ( W ^ t C ^ t ) , B t US + B ^ t US = 0 and B t EU + B ^ t EU = 0. ( 57 )

Goods market clearing also implies that real dividends are related to aggregate consumption and the trade flows by

D t = C t + 𝒳 t 𝔐 t , and D ^ t = C ^ t + ( 𝒳 t 𝔐 t ) / t , ( 58 )

where

𝒳 t = ( 1 η ) ( η 𝒯 t 1 θ + ( 1 η ) ) 1 t C ^ t and 𝔐 t = ( 1 η ) ( η 𝒯 t θ 1 + ( 1 η ) ) 1 C t . ( 59 )

Combining the bond and equity market clearing conditions in (21) and (22) with the aggregated budget constraint for U.S. households in (19) and the equation for dividends in (58) gives the following expression for the consolidated U.S. budget constraint:

FA t FL t = X t M t R t FL FL t 1 + R t FA FA t 1 , ( 60 )

where tBtEU=FAt, and B^tUS=FLt, and where RtFA=tR^t1/t1 and RtFL=Rt1. In equilibrium households hold long positions in foreign bonds so (i.e., BtEU>0andB^tUS>0) so FAt and FLt denote the real value of U.S. foreign assets and liabilities.

The exogenous processes for the log surplus ratios follow

s t + 1 = ( 1 Φ ) s ¯ + Φ s t + ω ( s t ) v t + 1 and s ^ t + 1 = ( 1 Φ ) s ¯ + Φ s ^ t + ω ( s ^ t ) v ^ t + 1 ( 61 )

where vt and v^t are mean-zero, unit variance i.i.d. shocks, and

ω ( s ) = { ω ( s max s ) s s max 0 s > s max .

The log endowments follow

y t = 𝔗 t + z t and y ^ t = 𝔗 t + z ^ t , ( 62 )

with

𝔗 t = 𝔗 t 1 + g + u t , z t = ρ z t + 1 + e t and z ^ = ρ z ^ t 1 + e ^ t ,

where ut, et and êt are mean-zero i.i.d. shocks with variances σu2 and σe2, respectively.

The Steady State

To determine the steady state, I first write the goods market clearing conditions in (56) as

cy t = ( τ t , ξ t ) and cy ^ t = ( τ t , ξ t ) ( 63 )

where ξt=cytcy^t+ztz^t and

( τ , ξ ) = In { [ η ( η + ( 1 η ) exp ( τ ) 1 θ ] θ 1 θ + ( 1 η ) [ ηexp ( τ ) 1 θ + ( 1 η ) ] θ 1 θ exp ( ξ ) } .

Let τ¯ and ξ¯ denote the steady state values of τt and ξt that are to be determined. Taking a first-order approximation to (63) around τ¯ and ξ¯ produces

[ cy t cy ¯ cy t cy ^ ¯ t ] = 1 Ξ [ 1 ξ ( τ ¯ , ξ ¯ ) ξ ( τ ¯ , ξ ¯ ) ξ ( τ ¯ , ξ ¯ ) 1 ξ ( τ ¯ , ξ ¯ ) ] [ ξ ( τ ¯ , ξ ¯ ) ξ ( τ ¯ , ξ ¯ ) ] ( z t z ^ t ) + 1 Ξ [ 1 ξ ( τ ¯ , ξ ¯ ) ξ ( τ ¯ , ξ ¯ ) ξ ( τ ¯ , ξ ¯ ) 1 ξ ( τ ¯ , ξ ¯ ) ] [ ξ ( τ ¯ , ξ ¯ ) ξ ( τ ¯ , ξ ¯ ) ] ( z t z ^ t ) , ( 64 )

where

Ξ = ( 1 ξ ( τ ¯ , ξ ¯ ) ) ( 1 ξ ( τ ¯ , ξ ¯ ) ) ξ ( τ ¯ , ξ ¯ ) ξ ( τ ¯ , ξ ¯ ) .

I also use log-normal approximations to the first-order conditions determining bond holdings.

r t = lnβ + γ 𝔼 t ( Δ c t + 1 + Δ s t + 1 ) 1 2 γ 2 𝕍 t ( c t + 1 + s t + 1 ) , r ^ t = lnβ + γ 𝔼 t ( Δ c ^ t + 1 + Δ s ^ t + 1 ) 1 2 γ 2 𝕍 t ( c ^ t + 1 + s ^ t + 1 ) , 𝔼 t Δ ε t + 1 + r ^ t = lnβ + γ 𝔼 t ( Δ c t + 1 + Δ s t + 1 ) 1 2 𝕍 t ( ε t + 1 γ ( c t + 1 + s t + 1 ) ) and 𝔼 t Δ ε t + 1 r t = lnβ γ 𝔼 t ( Δ c ^ t + 1 + Δ s ^ t + 1 ) + 1 2 𝕍 t ( ε t + 1 + γ ( c t + 1 + s t + 1 ) ) .

Rewriting these equations in terms of cyt and cy^t and simplifying gives

δ t = 1 2 γℂ 𝕍 t ( ε t + 1 , z t + 1 + z ^ t + 1 ) + 1 2 γℂ 𝕍 t ( ε t + 1 , c y t + 1 + cy ^ t + 1 ) + 1 2 γℂ 𝕍 t ( ε t + 1 , s t + 1 + s ^ t + 1 ) ( 65 a )
r t r ^ t = γ 𝔼 t ( Δc y t + 1 + Δ z t + 1 + Δ s t + 1 ) γ 𝔼 t ( Δ cy ^ t + 1 + Δ z ^ t + 1 + Δ s ^ t + 1 ) + 1 2 γ 2 { 𝕍 t ( cy ^ t + 1 + z ^ t + 1 + s ^ t + 1 ) 𝕍 t ( c y t + 1 + z t + 1 + s t + 1 ) } ( 65 b )

Combining these expressions with the identity 𝔼tΔεt+1=rtr^t+δt produces the approximate counterpart to (33). The link between this international asset market condition and the market clearing approximations in (63) is provided by the log terms of trade in (34c): τt = 𝒥 (εt), which I approximate as

τ t = τ ¯ + 𝒥 ε ( ε ¯ ) ( ε t ε ¯ ) . ( 66 )

In the steady state, zt = ẑt = 0, so (63) implies that ξ¯=(τ¯,ξ¯)(τ¯,ξ¯). Rearranging this expression, produces ξ¯=𝒢t(τ¯) where 𝒢 (τ) = ℋ(–τ, 0) – ℋ(τ, 0). Furthermore, 𝒢τ (τ) < 0 when there is consumption home bias.

To show that ε¯=0 is a candidate value for the steady state real exchange rate, I verify that

ε t = π z ( z t z ^ t ) + π s ( s t s ^ t ) ( 67 )

solves (64), (65) and (66) when ε¯=τ¯=0 and ξ¯=𝒢(0)=0. The values for πz and πs are determined by applying the method of undetermined coefficients as

π z = ( 2 φ 1 ) γ ( 1 ρ ) ( 1 ρ ) + 4 θ ( 1 η ) ( 1 ρ ) φ 2 / η and π s = γ ( 1 Φ 1 2 γω ) [ 1 + 4 θγ ( 1 η ) φ 2 / η ] ( 1 Φ 1 2 γω ) .

The corresponding approximations for the log consumption-output ratios are found by combining (64), (66) and (67).

Now suppose that

( . ) = ε ˜ + π z ( z t z ^ t ) + π s ( s t s ^ t ) , ( 68 )

for some value ε¯ close to zero. If the economy is in the steady state at t, (65a) simplifies to

δ t = 1 2 γ ℂ𝕍 t ( ε t + 1 , cy t + 1 + cy ^ t + 1 ) and ( 69 a )
r t r ^ t = 1 2 γ 2 { 𝕍 t ( cy ^ t + 1 + z ^ t + 1 + s ^ t + 1 ) 𝕍 t ( cy t + 1 + z t + 1 + s t + 1 ) } , ( 69 b )

because (64) and (66) imply that 𝔼tΔcyt+1=𝔼tΔcy^t+1 for any value of τ¯ and ξ¯. In a symmetric steady state, the variance terms in (69b) are equal, so rtr^t and 𝔼t Δεt+1 = σt. Since the approximation in (68) implies that 𝔼tΔεt+1 = 0, ε˜ can differ from zero if and only if there are non-zero values for τ¯ and ξ¯ such that (64) and (68) together imply that ℂ𝕍t(εt+1,cyt+1+cy^t+1)=0. Inspection of (64) reveals that this will be true when

1 2 ξ ( τ ¯ , ξ ¯ ) 1 2 ξ ( τ ¯ , ξ ¯ ) = ξ ( τ ¯ , ξ ¯ ) ξ ( τ ¯ , ξ ¯ ) .

Combining this expression with ξ¯=𝒢(τ¯) and approximating both the numerator and denominators around τ¯=0 produces

1 2 ( 1 η ) 2 η ( 1 η ) [ θ ( 2 η 1 ) + 4 ( 1 η ) θ η ( 2 η 1 ) ] τ ¯ 1 2 ( 1 η ) + 2 η ( 1 η ) [ θ ( 2 η 1 ) + 4 ( 1 η ) θ η ( 2 η 1 ) ] τ ¯ = 2 η θ ( 1 η ) + η θ ( 1 η ) τ ¯ 2 η θ ( 1 η ) η θ ( 1 η ) τ ¯ .

It is easy to check that the only solution to this equation is τ¯=0 when the parameters of the model are set to their calibrated values, so the corresponding value for ε˜ must be zero.

Let 𝒳t = [1, zt, ẑt, st, ŝt, 𝔗t]’ denote the vector of exogenous variables which follows 𝒳t+1 = 𝒜 𝒳t + ζt+1 with vec (𝕍tt+1)) = Ω𝒳t. The solutions to (64), (65) and (66) when ε¯=0 can be written as εt = lε 𝒳t, cyt = lcy𝒳t, and cy^t=lcy^𝒳t, so equilibrium consumption is approximated by ct = cyt + zt + 𝔗t = 1c𝒳t and c^t=cy^t+z^t+𝔗t=lc^𝒳t. The steady state value for the saving-to-consumption ratio, Λ¯W, is computed from the log normal approximation to (36) with tNt = 0:

λ t w = In β ( 1 κ w ) In ( 1 κ w ) + ( 1 γ ) 𝔼 t [ Δ c t + 1 γ Δ s t + 1 + κ w λ t + 1 w ] + 1 2 𝕍 t ( ( 1 γ ) c t + 1 γ s t + 1 + κ w λ t + 1 w ) , ( 70 )

where κw=Λ¯w/(1+Λ¯w). In particular, let λtw=lλw𝒳t, for some unknown vector of coefficients, lλW. Then (70) implies that

l λ w = [ In β ( 1 k ) In ( 1 k ) k In k ] l 1 + [ ( 1 γ ) l c γ l s ] ( 𝒜 1 ) + k w l λ w 𝒜 + 1 2 ( l λλ w l λλ w ) Ω ,

where lλλw=(1γ)lcγls+kwlλw and the vectors l1, lz and ls pick out 1, zt and st from 𝒳t, respectively. The first element in lλW identifies the steady state value of ln ΛtW.

The steady state value for the equity price-to-dividend ratio, Λ¯Q, is computed in a similar manner from the log normal approximation to (37):

λ t Q = In β ( 1 κ Q ) In ( 1 κ Q ) + ( 1 γ ) 𝔼 t [ Δ c t + 1 γ Δ s t + 1 + Δ dc t + 1 + κ Q λ t + 1 Q ] + 1 2 𝕍 t ( ( 1 γ ) c t + 1 γ s t + 1 + dc t + 1 + κ Q λ t + 1 Q ) , ( 71 )

where κQ=Λ¯Q/(1+Λ¯Q). Approximating (38) and (39) around the steady state produces

dc t = ( 1 η ) ( ε t + cy ^ t cy t + z t z ^ t ) 2 φ ( 1 η ) ( 1 θ ) ε t = l dc 𝒳 t ,

so (71) implies that λtQ=lλQ𝒳t where

l λ Q = [ In β ( 1 κ Q ) In ( 1 κ Q ) κ Q In κ Q ] l 1 + [ ( 1 γ ) l c γ l s + l dc ] ( 𝒜 1 ) + κ Q l λ Q 𝒜 + 1 2 ( l λλ Q l λλ Q )

and

l λλ Q = ( 1 γ ) l c γ l s + l dc + κ Q l λ Q .

The first element in lλQ identifies the steady state value of ln ΛtQ. The steady state values of ln Λ^tW and ln Λ^tQ are computed in an analogous manner.

Approximations

To approximate the first-order conditions associated by bond holdings, I rewrite (52b), (52c), (53b) and (53c) as

β 𝔼 t [ ( C t + 1 C t ) γ ( S t + 1 S t ) γ R t ] = 1 μ ( C ¯ t S ¯ C t S t ) γ [ exp ( n ¯ t n t ) 1 ] , β 𝔼 t [ ( C t + 1 C t ) γ ( S t + 1 S t ) γ t + 1 R ^ t t ] = 1 μ ( 1 + χ ) ( C ¯ t S ¯ C t S t ) γ [ exp ( n ¯ t n t ) 1 ] β 𝔼 t [ ( C ^ t + 1 C ^ t ) γ ( S ^ t + 1 S ^ t ) γ R ^ t ] = 1 μ ( C ¯ t S ¯ C ^ t S ^ t ) γ [ exp ( n ¯ t n ^ t ) 1 ] and β 𝔼 t [ ( C ^ t + 1 C ^ t ) γ ( S ^ t + 1 S ^ t ) γ t + 1 R t t + 1 ] = 1 μ ( 1 + χ ) ( C ¯ t S ¯ C ^ t S ^ t ) γ [ exp ( n ¯ t n ^ t ) 1 ] .

I take a standard log-normal approximation to the terms on the left-hand-side, and a second-order approximation to the natural log of the terms on the right-hand-side around the steady state. After some simplification, this produces

r t = In β + γ 𝒳 t ( Δ c t + 1 + Δ s t + 1 ) 1 2 γ 2 𝕍 t ( c t + 1 + s t + 1 ) + μ ( n t n ¯ t ) 1 2 μ ( μ + 1 ) ( n t n ¯ t ) 2 , ( 72 a )
r ^ t = In β + γ 𝔼 t ( Δ c ^ t + 1 + Δ s ^ t + 1 ) 1 2 γ 2 𝕍 t ( c ^ t + 1 + s ^ t + 1 ) + μ ( n ^ t n ¯ t ) 1 2 μ ( μ + 1 ) ( n ^ t n ¯ t ) 2 , ( 72 b )
𝔼 t Δ ε t + 1 + r ^ t = In β + γ 𝔼 t ( Δ c t + 1 + Δ s t + 1 ) 1 2 𝕍 t ( ε t + 1 γ ( c t + 1 + s t + 1 ) ) + μ ( χ + 1 ) ( n t n ¯ t ) 1 2 μ ( χ + 1 ) ( μ ( χ + 1 ) + 1 ) ( n t n ¯ t ) 2 and ( 72 c )
𝔼 t Δ ε t + 1 r t = In β γ 𝔼 t ( Δ c ^ t + 1 + Δ s ^ t + 1 ) + 1 2 𝕍 t ( ε t + 1 + γ ( c t + 1 + s t + 1 ) ) μ ( χ + 1 ) ( n ^ t n ¯ t ) + 1 2 μ ( χ + 1 ) ( μ ( χ + 1 ) + 1 ) ( n ^ t n ¯ t ) 2 . ( 72 d )

Together, these equations imply that

δ t = 1 2 γ ℂ𝕍 t ( ε t + 1 , c t + 1 + s t + 1 ) + 1 2 γ ℂ𝕍 t ( ε t + 1 , c ^ t + 1 + s ^ t + 1 ) + 1 2 μ χ ( n t n ^ t ) + 1 4 μ χ [ 1 + μ ( 2 + χ ) ] [ ( n ^ t n ¯ t ) 2 ( n t n ¯ t ) 2 ] and ( 73 a )
r t r ^ t = γ 𝔼 t ( Δ c t + 1 + Δ s t + 1 ) + γ 𝔼 t ( Δ c ^ t + 1 + Δ s ^ t + 1 ) + 1 2 γ 2 { 𝕍 t ( c ^ t + 1 + s ^ t + 1 ) 𝕍 t ( c t + 1 + s t + 1 ) } + μ ( n t n ^ t ) + 1 2 μ ( μ + 1 ) [ ( n ^ t n ¯ t ) 2 ( n t n ¯ t ) 2 ] . ( 73 b )

Equations (46) and (47) in the text reproduce these expressions without the terms involving (n^tn¯t)2 and (ntn¯t)2.

I approximate the equations determining the logs of ΛtQ, Λ^tQ, ΛtW and ΛtW in an analogous fashion from (54) and (55) as

λ t Q = In β ( 1 κ Q ) In ( 1 κ Q ) + ( 1 γ ) 𝔼 t [ Δ c t + 1 γ Δ s t + 1 + Δ dc t + 1 + κ Q λ t + 1 Q ] + 1 2 𝕍 t ( ( 1 γ ) c t + 1 γ s t + 1 + dc t + 1 + κ Q λ t + 1 Q ) , ( 74 a )
λ ^ t Q = In β ( 1 κ Q ) In ( 1 κ Q ) + ( 1 γ ) 𝔼 t [ Δ c ^ t + 1 γ Δ s ^ t + 1 + Δ d ^ c t + 1 + κ Q λ ^ t + 1 Q ] + 1 2 𝕍 t ( ( 1 γ ) c ^ t + 1 γ s ^ t + 1 + d ^ c t + 1 + κ Q λ ^ t + 1 Q ) , ( 74 b )
λ t W = In β ( 1 κ W ) In ( 1 κ W ) + ( 1 γ ) 𝔼 t [ Δ c t + 1 γ Δ s t + 1 + κ W λ t + 1 W ] + 1 2 𝕍 t ( ( 1 γ ) c t + 1 γ s t + 1 + κ W λ t + 1 W ) 1 2 χ ( 1 η ) [ 1 χ ( 1 η ) ] ( n t n ¯ t ) 2 χ ( 1 η ) ( n t n ¯ t ) [ 1 + γ ( s t s ¯ ) ( λ t W λ ) ( 1 γ ) ( c t c ¯ t ) ] and ( 74 c )
λ ^ t W = In β ( 1 κ W ) In ( 1 κ W ) + ( 1 γ ) 𝔼 t [ Δ c ^ t + 1 γ Δ s ^ t + 1 + κ W λ ^ t + 1 W ] + 1 2 𝕍 t ( ( 1 γ ) c ^ t + 1 γ s ^ t + 1 + κ W λ ^ t + 1 W ) 1 2 χ ( 1 η ) [ 1 χ ( 1 η ) ] ( n ^ t n ¯ t ) 2 χ ( 1 η ) ( n ^ t n ¯ t ) [ 1 + γ ( s ^ t s ¯ ) ( λ ^ t W λ ) ( 1 γ ) ( c ^ t c ¯ t ) ] . ( 74 d )

Here κQ=Λ¯Q/(1+Λ¯Q) and κQ=Λ¯W/(1+Λ¯W) where Λ¯W and Λ¯Q are the steady state values for ΛtW and ΛtQ, identified above.

I approximate the other equilibrium conditions in a straightforward manner around the steady state real exchange rate rate. Using the definition in (18) we can approximate the log real exchange to second order by

ε t = ( 2 η 1 ) τ t . ( 75 )

To approximate the goods market clearing conditions, I use (56) to compute ln(Yt/Ct) and ln(Ŷtt) and then take second-order approximations around the steady state of the resulting expressions. Simplifying the result using (75) produces

[ c t c ^ t ] = [ φ 1 φ 1 φ φ ] [ y t y ^ t ] + [ 2 θ φ 2 ( 1 η ) / η 2 θ φ 2 ( 1 η ) / η ] ε t ( 76 )
[ 1 2 ( 4 θ η 2 4 θ η + 1 ) ( η 1 ) θ φ 2 / η 1 2 η ( η 1 ) η θ ( 1 η ) ( 2 φ 1 ) 1 2 ( 4 θ η 2 4 θ η + 1 ) ( η 1 ) θ φ 2 / η 1 2 η ( η 1 ) η θ ( 1 η ) ( 2 φ 1 ) ] [ ε t 2 ( c t c ^ t ) 2 ε t ( c t c ^ t ) ] ,

where φ = η/(2η – 1) > 0. Approximations for dividends and trade flows are derived in an analogous manner from (58) and (59) as

d t c t = ( 1 η ) nx t + 1 2 η ( 1 η ) nx t 2 + φ ( 1 θ ) ( 1 η ) ε t nx t , ( 77 a )
d ^ t c ^ t = ( 1 η ) nx t + 1 2 η ( 1 η ) nx t 2 + φ ( 1 θ ) ( 1 η ) ε t nx t , ( 77 b )
x t = In ( 1 η ) + [ 1 φ ( 1 θ ) ] ε + c ^ t and ( 77 c )
m t = In ( 1 η ) + φ ( 1 θ ) ε t + c t , ( 77 d )

where nxt = xt – mt. Market clearing in the bond markets implies that Nt=(1+𝓍)tB^tUS and N^t=(1+𝓍)B^tUStBtEU. We can use these two expressions to approximate the logs of Nt and N^t by

n t = In χ 1 χ nfl t 1 2 1 + χ χ 2 nfl t 2 + fa t and n ^ t = In χ 1 χ nfl t 1 2 1 + χ χ 2 nfl t 2 + fl t , ( 78 )

where nflt = flt – fat. Notice that ntn^t=2xnflt and

δt=12γℂ𝕍t(εt+1,ct+i+st+1)+12γℂ𝕍t(εt+1,c^t+1+s^t+1)+12μχ(ntn^t) to first order, so the value for μ determines the semi-elasticity of the risk premium with respect to variations in the log ratio of foreign liabilities to assets.

Finally, the consolidated budget constraint in (60) implies that

FA t R t FA FA t 1 1 + 𝔐 t R t 1 FA FA t 1 = FL t R t FA FA t 1 + 𝔛 t R t FA FA t 1 R t FA FL t 1 R t FA FA t 1 .

Taking second-order approximations to the terms on the left- and right-hand-sides, simplifying and taking conditional expectations produces

fl t fa t = ( 1 κ ) 𝔼 t nx t + 1 + 𝔼 t [ r t + 1 FA r t + 1 FA ] + κ 𝔼 t ( fl t + 1 fa t + 1 ) + 1 2 κ 2 𝔼 t [ ( Δ fl t + 1 r t + 1 FL ln κ ) 2 ( Δ fa t + 1 r t + 1 FA ln k ) 2 ] ( 79 ) + 1 2 ( 1 κ ) 𝔼 t [ ( x t + 1 r t + 1 FL fl t ln ( 1 κ ) ) 2 ( m t + 1 r t + 1 FA fa t ln ( 1 κ ) ) 2 ] .
Solution Method

The solution produces vectors of coefficients, πa and π˜a, that link the equilibrium behavior of any endogenous variable at to the exogenous variables by

a t = a ¯ t + π a 𝒵 t + π ˜ a 𝒵 ˜ t ( 80 )

where 𝒵t=[zt,z^t,sts¯,s^ts]ʹ and 𝒵˜t=vec(𝒵). āt identifies the steady state value of stationary variables and the trend, 𝔗t, in non-stationary variables. The exogenous processes for the endowments and log surplus ratios imply that

𝒵 t + 1 = 𝒜 𝒵 t + 𝒱 t + 1 with vec ( V t ( 𝒱 t + 1 ) ) = Σ 0 + Σ 𝒵 t , ( 81 )

and

𝔼 t 𝒵 t + 1 = ( 𝒜 𝒜 ) 𝒵 t + Σ 0 + Σ 𝒵 t . ( 82 )

In principle, the πa and π˜a vectors for each endogenous variable could be found by applying the method of undetermined coefficients to the set of second-order approximations presented above, but in practice it is more computationally efficient to use an iterative procedure based on Lombardo and Sutherland (2007).

The first step in this procedure is to find initial values for the πa vectors. For this purpose, I combine (73) with (76), (77) and (79) ignoring all the second-order terms. This produces the following system:

𝔼 t Δ ε t + 1 = δ t + r t r ^ t , ( 83 a )
r t r ^ t = γ 𝔼 t ( Δ c t + 1 + Δ s t + 1 ) γ 𝔼 t ( Δ c ^ t + 1 + Δ s ^ t + 1 ) ( 83 b )
1 2 γ 𝕍 t 2 ( c t + 1 + s t + 1 ) + 1 2 γ 𝕍 t 2 ( c ^ t + 1 + s ^ t + 1 ) μ ( χ + 2 χ ) nfl t , ( 83 c )
δ t = 1 2 γ ℂ𝕍 t ( c t + 1 + c ^ t + 1 , ε t + 1 ) + 1 2 γ 𝕍 t ( s t + 1 + s ^ t + 1 , ε t + 1 ) μ ( χ + 2 2 ) nfl t , ( 83 d )
nfl t = ( 1 κ ) 𝔼 t [ ( ε t + 1 + c ^ t + 1 c t + 1 ) 2 φ ( 1 θ ) ε t + 1 ] + δ t + κ 𝔼 t nfl t + 1 , ( 83 e )
c t = φ y t + ( 1 φ ) y ^ t [ 2 θ φ 2 ( 1 η ) / η ] ε t and ( 83 f )
c ^ t = ( 1 φ ) y t + φ y ^ t + [ 2 θ φ 2 ( 1 η ) / η ] ε t . ( 83 g )

Applying the method of undetermined coefficients to these equations using (80) produces

a t = a ¯ t + π a ( 1 ) 𝒵 t for a t = { ε t , r t r ^ t , δ t , nfl t , c t , c ^ t } . ( 84 )

Combing these expressions with (72), (74) and (77) produces

a t = a ¯ t + π a ( 1 ) 𝒵 t for a t = { r t , r ^ t , n t , n ^ t , λ t Q , λ ^ t Q , λ t W , λ ^ t W , x t , m t , d t , d ^ t , fa t , fl t } . ( 85 )

The second step uses (84) and (85) to compute the second-order terms in (72), (74), (76), (77), (78) and (79). Notice that all of these terms in this system involve deviations from steady-state values, i.e., (ata¯t)(btb¯t). They are computed as

( a t a ¯ t ) ( b t b ¯ t ) = ( π a ( 1 ) 𝒵 t ) ( π b ( 1 ) 𝒵 t ) = ( π b ( 1 ) π a ( 1 ) ) 𝒵 t and 𝔼 t ( a t + 1 a ¯ t + 1 ) ( b t + 1 b ¯ t + 1 ) = ( π b ( 1 ) π a ( 1 ) ) ( Σ 0 + Σ 𝒵 t ) ,

using the coefficient vectors πa(1) and πb(1) from the first step. The other terms in the system are assumed to take the form of

a t = a ¯ t + π a ( 2 ) 𝒵 t + π ˜ a ( 2 ) 𝒵 ˜ t ,

where πa(2) and π˜a(2) are unknown coefficient vectors. Making these substitutions produces a system of linear equations in 𝒵t and 𝒵˜t, so πa(2) and π˜a(2) can be determined by the method of undetermined coefficients. For example, from equation (76), we obtain

c ¯ t + π c ( 2 ) 𝒵 t + π ˜ c ( 2 ) 𝒵 ˜ t = z t + [ φ π z + ( 1 φ ) π z ^ ] 𝒵 t [ 2 θ φ 2 ( 1 η ) / η ] ( π ε ( 2 ) 𝒵 t + π ˜ ε ( 2 ) 𝒵 ˜ t ) + [ 1 2 θ φ 2 ( 4 θ η 2 4 θη + 1 ) ( η 1 ) / η ] ( π ε ( 1 ) π ε ( 1 ) ) 𝒵 ˜ t + 1 2 η ( η 1 ) ( ( π c ( 1 ) π c ^ ( 1 ) ) ( π c ( 1 ) π c ^ ( 1 ) ) ) 𝒵 ˜ t ηθ ( 1 η ) ( 2 φ 1 ) ( ( π ( π c ( 1 ) π c ^ ( 1 ) ) ) 𝒵 ˜ t .

where ztC=πz𝒵1 and ẑt = π𝒵t. Hence, equating coefficients gives

π c ( 2 ) = φ π z + ( 1 φ ) π z ^ [ 2 θ φ 2 ( 1 η ) / η ] π ε ( 2 ) and ( 86 a )
π ˜ c ( 2 ) = [ 2 θ φ 2 ( 1 η ) / η ] π ˜ ε ( 2 ) + [ 1 2 θ φ 2 ( 4 θ η 2 4 θη + 1 ) ( η 1 ) / η ] ( π ε ( 1 ) π ε ( 1 ) ) + 1 2 η ( η 1 ) ( ( π c ( 1 ) π c ^ ( 1 ) ) ( π c ( 1 ) π c ^ ( 1 ) ) ηθ ( 1 η ) ( 2 φ 1 ) ( ( π ( π c ( 1 ) π c ^ ( 1 ) ) ) ( 86 b )

Notice that equation (86b) involves only π˜(2) and the π(1) vectors. This pattern applies across the system, so the π˜(2) vectors can be computed using the first-step estimates, π(1). The π(2) coefficients are determined by (86a) and similar equations derived from the system. This set of equations is similar to those determining π(1) except that it also involves terms like (πb(1)πa(1))Σ because 𝒵t affects 𝔼t(at+1a¯t+1)(bt+1b¯t+1). Consequently, the π(2) coefficients will generally differ from π(1). If the log surplus ratios were homoskedastic, Σ would equal the null matrix, and π(2) would equal π(1) so only two steps would be necessary, as in Lombardo and Sutherland (2007)

To summarize, the solution procedure involves: (i) solving for π(1) from (83); (ii) solving for π(2) and π˜c(2) using π(1) and the second-order approximations to the model’s equilibrium conditions; and (iii) repeating step (ii) solving for π(j) and π˜c(j) using π(J-1) until π(j) = π(J-1). In practice, I find that π(j) – π(J-1) is very close to a vector of zeros for all the variables when j = 3, so only one iteration is necessary.

Finally, applying the method of undetermined coefficients to the system in (83) when μ = 0, gives solutions in (84) such that εt = γ(ct – ct) + γ(st – ŝt), so the this version of the model produces equilibrium under complete markets.

1

The consumption surplus ratio is defined as the difference between the level of current consumption and habit divided by current consumption: (CtHt)/Ct.

2

Consumption baskets differ across countries because households’ preferences are biased towards the consumption of the domestically endowed goods. Consequently, the real bonds are imperfect substitutes in households’ portfolios. Domestic bonds offer a risk-free real return to domestic households but a risky return to foreign households because variations in the real exchange rate affect the return measured in terms of foreign consumption.

3

Verdelhan (2010) uses the CC habit specification in a two-country model to account for the forward premium puzzle. He assumes that markets are complete and that households only consume domestically produced goods. This extreme form of home bias allows him to circumvent the problems induced by variations in the terms of trade under complete risk-sharing but at the cost of eliminating international trade. Bansal and Shaliastovich (2010) also assume an extreme form of home bias to avoid a similar problem in their adaption of the long-run risk framework proposed by Bansal and Yaron (2004). In more recent research, Moore and Roche (2010) use a model with habits and complete markets to account for the forward premium anomaly. They assume that habits are relate to the consumption of individual goods (sometime called deep-habits) and are driven by endowment shocks. This means that the habit level for each good is perfectly correlate across countries without regard to the international differences in consumption. Jonen and Scheuring (2011) propose a habit-based model that is more closely related to the CC specification in which habits respond to consumption that is determined endogenously. This model assumes that households consume a basket comprising a single traded and nontraded good so variations in the terms of trade cannot cause any problems. Of course this also means that all the variations in real exchange rates reflect changes the relative prices of nontraded to traded goods, an implication that is at odds with the empirical evidence; see, e.g., Engel (1999).

4

Following Pagan (1984), I use an IV procedure akin to 2SLS to estimate (9) that accounts for sampling error in iti^t𝔼˜[Δpt+1Δp^t+1|Xt]. This procedure replaces iti^t𝔼˜[Δpt+1Δp^t+1|Xt] by iti^t[Δpt+1Δp^t+1] in (9) and then uses iti^t𝔼˜[Δpt+1Δp^t+1|Xt] as an instrument for iti^t[Δpt+1Δp^t+1]. The resulting coefficient estimates are identical to OLS. The standard errors are computed from the IV procedure with the White (1980) covariance estimator that allows for the presence of heteroskedasticity.

5

In equilibrium households borrow by selling domestic bonds, so Bi,tUS<0andB^i,tEU<0.

7

Embellishments for inducing stationarity include the introduction of endogenous discounting in households’ preferences, asset-holding costs and (ad hoc) debt-elastic interest rates, as discussed in Schmitt-Grohe and Uribe (2003).

8

The log ratios of U.S. and E.U. consumption to output are ctyt+11θln(η+(1η)𝒯t1θ) and c^ty^t+11θln(η+(1η)𝒯t1θ) when measured in terms of the domestic consumption baskets. Consequently, cyt and cy^t should really be thought of as the adjusted log ratios that value endowments when the terms of trade are one.

9

If the economy is at the steady state in period t, Δzt+1=et+1,Δz^t+1=e^t+1,Δst+1=ω(s¯)vt+1andΔs^t+1=ω(s¯)v^t+1 so (33) show that ε¯ depends on the uncertainty households′ face concerning period-t + 1 shocks.

10

When the first-order conditions are computed from the original optimization problem, tNt = 0 by complimentary slackness. This is not guaranteed when the first-order conditions are computed from the modified optimization problem, but in practice the tNt/Ct term has a negligible impact on the values of ΛtW I compute.

11

This is not a standard second-order approximation to the log of the return on wealth in (28). Campbell and Viceira (2002) derive the approximation by applying Ito’s lemma to the log return on wealth when the prices of individual assets follow continuous-time diffusion processes. Notice that the vector of portfolio shares αt appears multiplicatively, and not in deviations from its steady state value.

12

The variance of endowment growth, σu2, governs the long run correlation between consumption growth in each country. I set the value of σu2 so that this correlation in the model matches the sample correlation in US and Euro-area data. The value of this parameter does not affect the dynamics discussed below.

13

Obviously, this is a very reduced-form approach of capturing the low rate of exchange-rate pass-through we observe empirically (see, e.g., Campa and Goldberg, 2008) For a recent discussion of the possible reasons for low pass-through, see Devereux and Yetman (2010).

14

It is worth noting that the discrepancy between the coefficient estimate in Table 3 and the model-implied value is not statistically significant: a t-test for the null that the coefficient equals -1.424 is not significant at the 5 percent level.

15

Since the solution method incorporates second-order approximations, the effects of a shock depend on the initial state of the economy. The impulse responses shown in Figures 3 and 4 are computed under the assumption that the economy is initially in the steady-state. Note, also, that each plot shows the response per one percent of the shock, not the actual response.

16

The small effects of market incompleteness are reminiscent of the results obtained by Cole and Obstfeld (1991) but the mechanism is different. In their model variations in the terms of trade exactly offset changes in the endowments to keep households’ wealth constant. Here wealth changes but this does not materially affect the sharing of risks among households.

17

Risk-shocks have very small effects on αtFB, so the fall in Nt closely matches the fall in Qt.

18

Expectations concerning future consumption and dividend growth also influence ΛtQ, ΛtW and their E.U. counterparts, but the effects are very small and so can safely be ignored for the purpose of this discussion.

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Exchange-Rate Dark Matter
Author:
Mr. Martin D Evans