Learning and Time-Varying Macroeconomic Volatility

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Transcription:

Learning and Time-Varying Macroeconomic Volatility Fabio Milani University of California, Irvine International Research Forum, ECB - June 26, 28

Introduction Strong evidence of changes in macro volatility over time (The Great Moderation) Kim and Nelson (1999), McConnell and Pérez-Quiròs (2), Stock and Watson (22), Blanchard and Simon (21)

Time-Varying Volatility Conditional Standard Deviation (Inflation) 1.6 1.4 1.2 1.8.6.4 196 1965 197 1975 198 1985 199 1995 2 25 2 Conditional Standard Deviation (Output Gap) 1.5 1.5 196 1965 197 1975 198 1985 199 1995 2 25 Figure: Conditional Standard Deviation series for Inflation and Output Gap

Introduction Need to correctly model volatility Sims and Zha (AER 26): BVAR, Regime changes in volatilities of shocks

Introduction In DSGE Models? Exogenous shocks with constant variance (Smets and Wouters JEEA 23, AER 27, An and Schorfheide ER 27) DSGE with Stochastic Volatility Justiniano and Primiceri (AER forth.), Fernandez-Villaverde and Rubio-Ramirez (RES 27) Time variation in the volatility of exogenous shocks

Introduction But what explains the changing volatility?

Scope of the paper Present a simple model with learning The learning speed (gain coefficient) of the agents is endogenous: it responds to previous forecast errors Endogenous Time-Varying Volatility Related: Branch and Evans (RED 27), Lansing (27), Bullard and Singh (27).

Results: 1 The changing gain induces endogenous time variation in the volatilities of the macroeconomic variables the agents try to learn 2 Evidence of time variation in endogenous gain from estimated model 3 The econometrician can spuriously find evidence of stochastic volatility if learning is not taken into account

The Model Stylized New Keynesian Model π t = βêtπ t+1 + κx t + u t (1) x t = Êtx t+1 σ(i t Êtπ t+1 ) + g t (2) i t = ρ t i t 1 + (1 ρ t )(χ π,t π t 1 + χ x,t x t 1 ) + ε t (3) Learning instead of RE TV Monetary Policy

Expectations Formation VAR to form inflation and output expectations Perceived Law of Motion (VAR(1)): Z t = a t + b t Z t 1 + η t (4) where Z t [π t, x t, i t ] Minimum State Variable solution

Learning Coefficient Updating φ t = φ t 1 + g t,y Rt 1 X t (Z t X t φ t 1 ) (5) R t = R t 1 + g t,y (X t 1 X t 1 R t 1 ) (6) where φ t = (a t, vec(b t ) ) and X t {1, Z t 1 } t 1.

Endogenous Time-Varying Gain Decreasing Gain if Forecast Errors are small Switch to Constant Gain if Forecast Errors become large P J t g t,y = 1 j= if ( y t j E t j 1 y t j ) J < υ P t y J j= g y if ( y t j E t j 1 y t j ) J υt y, where y = π, x, i. (Decr. Gain reset to 1 g 1 y +t ) Similar to Marcet-Nicolini (υ t is m.a.d. of forecast errors) Constant Gain is estimated Which situations? (7)

Questions: 1 Does the gain coefficient affect volatility? Can the model generate time-varying volatility in inflation and in the output gap? 2 Does the model fit U.S. data? Is there evidence of changes in the gain over time? 3 Does the omission of learning imply that researchers spuriously find stochastic volatility in the structural shocks? 4 Does the model-implied stochastic volatility resemble the SV estimated from the data? 5 What are the effects of MP on the estimated Volatility?

1. Endogenous Gain and TV Volatility 4.5 4 Std. Infl Std. Output Gap 3.5 3 2.5 2 1.5 1.5.5.1.15 Figure: Volatility of simulated Inflation and Output Gap as a function of the constant gain coefficient.

1. Endogenous Gain and TV Volatility Volatility typically increases in the gain Simulation (1, periods) Gain switches endogenously according to previous forecast errors

1. Endogenous Gain and TV Volatility 5 4 Std. Infl Std. Gap Time Varying Volatility (rolling standard deviation) 3 2 1 1 2 3 4 5 6 7 8 9 1.2.15 TV gain (Infl) TV gain (Gap) Endogenous Time Varying Gain.1.5 1 2 3 4 5 6 7 8 9 1 Figure: Time-Varying Volatility with Time-Varying Endogenous Gain Coefficient.

2. Bayesian Estimation Gain switches from decreasing to constant Constant Gain jointly estimated in the system Metropolis-Hastings Quarterly U.S. data, 196:I-26:I, data from 1954 to 1959 to initialize learning algorithm Uniform priors for gains

2. Bayesian Estimation: Priors Prior Distribution Description Param. Range Distr. Mean 95% Int. Inverse IES σ 1 R + G 1 [.12, 2.78] Slope PC κ R + G.25 [.3,.7] Discount Rate β.99.99 Interest-Rate Smooth ρ pre79 [, 1] B.8 [.46,.99] Feedback to Infl. χ π,pre79 R N 1.5 [.51, 2.48] Feedback to Output χ x,pre79 R N.5 [.1,.99] Interest-Rate Smooth ρ post79 [, 1] B.8 [.46,.99] Feedback to Infl. χ π,post79 R N 1.5 [.51, 2.48] Feedback to Output χ x,post79 R N.5 [.1,.99] Std. MP shock σ ε R + IG 1 [.34, 2.81] Std. g t σ g R + IG 1 [.34, 2.81] Std. u t σ u R + IG 1 [.34, 2.81] Constant Gain infl. g π [,.3] U.15 [.7,.294] Constant Gain gap g x [,.3] U.15 [.7,.294] Constant Gain FFR g i [,.3] U.15 [.7,.294] Table 1 - Prior Distributions.

2. Bayesian Estimation: Results Posterior Distribution Description Parameter Mean 95% Post. Prob. Int. Inverse IES σ 1 6.4 [4.17-9.14] Slope PC κ.21 [.26-.54] Discount Factor β.99 - IRS pre-79 ρ pre79.937 [.85-.99] Feedback Infl. pre79 χ π,pre 79 1.3 [.83-1.81] Feedback Gap pre79 χ x,pre 79.66 [.29-1.13] IRS post-79 ρ post79.93 [.88-.97] Feedback Infl. post79 χ π,post 79 1.66 [1.19-2.11] Feedback Gap post79 χ x,post 79.48 [.7-.85] Autoregr. Cost-push shock ρ u.39 [.27-.49] Autoregr. Demand shock ρ g.85 [.78-.92] Std. Cost-push shock σ u.89 [.81-.98] Std. Demand shock σ g.65 [.59-.72] Std. MP shock σ ε.97 [.88-1.7] Constant gain (Infl.) g π.82 [.78-.9] Decreasing gain (Infl.) t 1 - - Constant gain (Gap) g x.73 [.6-.82] Decreasing gain (Gap) t 1 - - Constant gain (FFR) g i.3 [,.23] Decreasing gain (FFR) t 1 - - Table 2 - Posterior Distributions: baseline case with J = 4.

2. Bayesian Estimation: Time-Varying Gain Endogenous Time Varying Gain Inflation.8.6.4.2 196 1965 197 1975 198 1985 199 1995 2 25.8 Endogenous Time Varying Gain Output Gap.6.4.2 196 1965 197 1975 198 1985 199 1995 2 25 Figure: Endogenous Time-Varying Gain Coefficients (estimated constant gain). Baseline Case

Is it a good idea to use this learning rule? Is it dominated by alternatives? Endogenous TV Gain Decreasing Gain Constant Gain Inflation.94.97.98 Output Gap.88 1..91 Table 6 - RMSEs. Optimality Tests. I t+1,t 1(Y t+1,t < Ŷt+1,t) = α + βŷt+1,t + u t+1 (8) Back out Loss Function

2. Bayesian Estimation: Time-Varying Gain.8 Endogenous Time Varying Gain Inflation.6.4.2 196 1965 197 1975 198 1985 199 1995 2 25.8 Endogenous Time Varying Gain Output Gap.6.4.2 196 1965 197 1975 198 1985 199 1995 2 25 Figure: Endogenous Time-Varying Gain Coefficients (estimated constant gain). Case with J = 2

2. Bayesian Estimation: Time-Varying Gain.35.3.25 Posterior Distribution g π Prior Distribution.2.15.1.5.5.6.7.8.9.1.2.15 Posterior Distribution g x Prior Distribution.1.5.5.6.7.8.9.1 Figure: Constant Gain Coefficients: Prior and Posterior Distributions.

2. Bayesian Estimation: Time-Varying Gain.1 Endogenous Time Varying Gain Inflation.8.6.4.2 196 1965 197 1975 198 1985 199 1995 2 25.6 Endogenous Time Varying Gain Output Gap.5.4.3.2.1 196 1965 197 1975 198 1985 199 1995 2 25 Figure: Endogenous Time-Varying Gain Coefficients (Case with low and high constant gain coefficients only).

2. Bayesian Estimation: Forecast Errors 4 Forecast Errors Inflation 3 2 1 196 1965 197 1975 198 1985 199 1995 2 25 Forecast Errors Output Gap 4 3 2 1 196 1965 197 1975 198 1985 199 1995 2 25 Forecast Errors FFR 1 5 196 1965 197 1975 198 1985 199 1995 2 25 Figure: Forecast errors for inflation, output gap, and federal funds rate (absolute values).

2. Bayesian Estimation: Forecast Errors 3 2 Inflation Mean Absolute Forecast Error ν t π 1 196 1965 197 1975 198 1985 199 1995 2 25 Output Gap 3 2 Mean Absolute Forecast Error ν t x 1 196 1965 197 1975 198 1985 199 1995 2 25 FFR 6 4 Mean Absolute Forecast Error ν t i 2 196 1965 197 1975 198 1985 199 1995 2 25 Figure: Rolling Mean Absolute Forecast errors vs. Updated ν t for inflation, output gap, and federal funds rate series.

3. If learning is neglected: The volatility of shocks may be overestimated Possible to spuriously find Stochastic Volatility

3. Test for ARCH/GARCH Effects Endogenous TV Gain No Learning J = 4 J = 2 ARCH(1) GARCH(1,1) ARCH(1) GARCH(1,1) ARCH(1) GARCH(1,1) Inflation.517.61.48.56.5.6 Output Gap.785.89.85.9.45.5 Table 7 - Test for the existence of ARCH/GARCH effects (5% significance): proportion of rejections of the null hypothesis of no ARCH/GARCH effects.

4. Volatility.12.1 Max. Std. Inflation eq. Residuals.8.6.4.2 196 1965 197 1975 198 1985 199 1995 2 25.12.1 Max. Std. Output Gap eq. Residuals.8.6.4.2 196 1965 197 1975 198 1985 199 1995 2 25 Figure: Maximum rolling Standard Deviation of residuals across simulations: Kernel Density Estimation.

4. The Great Moderation Ratio Ratio Endogenous TV Gain No Learning Data Baseline J = 2 CG Std. Infl. 1985 26 Std. Infl. 196 1984.39.42.43 1..35 (Std. OutputGap 1985 26) (Std. Output Gap 196 1984).42.52.54 1..5 Table 8 - The Great Moderation: ratio of standard deviations for inflation and output gap in the second versus the first part of the simulated samples (median across simulations).

5. Monetary Policy, Learning, and Volatility Simulation for χ π = [,..., 5]: Related: Benati-Surico (27) 1.8 Fraction of Switches to a Constant Gain.6.4.2 χ.5 1 1.5 2 2.5 3 3.5 4 4.5 5 π.8.7 Average Gain in Sample.6.5.4 χ.5 1 1.5 2 2.5 3 3.5 4 4.5 5 π.9.8 % Rejections no ARCH Effects.7.6.5 χ π.5 1 1.5 2 2.5 3 3.5 4 4.5 5 Figure: Effects of Monetary Policy on Volatility.

5. Bernanke - Great Moderation Speech I am not convinced that the decline in macroeconomic volatility of the past two decades was primarily the result of good luck. changes in monetary policy could conceivably affect the size and frequency of shocks hitting the economy, at least as an econometrician would measure those shocks changes in inflation expectations, which are ultimately the product of the monetary policy regime, can also be confused with truly exogenous shocks in conventional econometric analyses. some of the effects of improved monetary policies may have been misidentified as exogenous changes in economic structure or in the distribution of economic shocks.

6. TV Volatility: Learning or Exogenous Shocks? Test ARCH/GARCH in DSGE Model Innovations now Output Gap Inflation DSGE-RE ARCH ARCH DSGE-TV Gain ARCH No ARCH

6. TV Volatility: Learning or Exogenous Shocks? 2 1.5 Innovation in Inflation Equation: Rolling Std. Under Learning/TV Gain Under RE 1.5 196 1965 197 1975 198 1985 199 1995 2 25 1.4 1.2 1 Innovation in Output Gap Equation: Rolling Std. Under Learning/TV Gain Under RE.8.6.4.2 196 1965 197 1975 198 1985 199 1995 2 25 Figure: Rolling Std. estimated innovations under RE and Learning

Conclusions Strong Evidence of Stochastic Volatility in the economy Usually Exogenous Learning with endogenous TV gain (depends on previous forecast errors) Endogenous Stochastic Volatility Gain often larger in pre-1984 sample Overestimation of TV in volatility of exogenous shocks.

Future Directions How much volatility can learning explain? (estimate DSGE model with learning and TV volatility). More serious attempt to match volatility series in the data. Different ways to model endogenous gain/ Optimality Interactions Policy/Learning/Volatility