shadow interest rate - cemla

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Shadow rate Empirical evidence New Keynesian model International evidence Shadow Interest Rate Jing Cynthia Wu Notre Dame and NBER Coauthors: Dora Xia (BIS) and Ji Zhang (Tsinghua) Cynthia Wu (Notre Dame & NBER) 1 / 34

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Page 1: Shadow Interest Rate - CEMLA

Shadow rate Empirical evidence New Keynesian model International evidence

Shadow Interest Rate

Jing Cynthia WuNotre Dame and NBER

Coauthors: Dora Xia (BIS) and Ji Zhang (Tsinghua)

Cynthia Wu (Notre Dame & NBER) 1 / 34

Page 2: Shadow Interest Rate - CEMLA

Shadow rate Empirical evidence New Keynesian model International evidence

ZLB: monetary policy

Before ZLB, policy rates are the tool for monetary policy and its research

I Central banks lower policy rates to stimulate aggregate demand

I Economists rely on them to study monetary policy

Policy rates at ZLB

I Japan, US, EuropeI Unconventional policy tools

I large-scale asset purchases (QE)I lending facilitiesI forward guidanceI negative interest rate policy

Cynthia Wu (Notre Dame & NBER) 2 / 34

Page 3: Shadow Interest Rate - CEMLA

Shadow rate Empirical evidence New Keynesian model International evidence

ZLB: economic models

Term structure models

I Benchmark Gaussian ATSM

I ZLB: Yields are unconstrained in the model, but constrained in the data

I My papers: Wu and Xia (JMCB 2016), Wu and Xia (JAE forthcoming)

I respect the ZLB

New Keynesian models

I Benchmark models: no unconventional monetary policy

I My papers: Wu and Zhang (JEDC 2019), Wu and Zhang (JIE 2019)

I incorporate unconventional monetary policyI Key feature: tractable

Cynthia Wu (Notre Dame & NBER) 3 / 34

Page 4: Shadow Interest Rate - CEMLA

Shadow rate Empirical evidence New Keynesian model International evidence

ZLB: economic models

Term structure models

I Benchmark Gaussian ATSM

I ZLB: Yields are unconstrained in the model, but constrained in the data

I My papers: Wu and Xia (JMCB 2016), Wu and Xia (JAE forthcoming)

I respect the ZLB

New Keynesian models

I Benchmark models: no unconventional monetary policy

I My papers: Wu and Zhang (JEDC 2019), Wu and Zhang (JIE 2019)

I incorporate unconventional monetary policyI Key feature: tractable

Cynthia Wu (Notre Dame & NBER) 3 / 34

Page 5: Shadow Interest Rate - CEMLA

Shadow rate Empirical evidence New Keynesian model International evidence

Common theme: shadow rate

Black (1995)rt = max(st , r)

Sources:BoardofGovernorsoftheFederalReserveSystemandWuandXia(2015)

Wu-XiaShadowFederalFundsRate

Effectivefederalfundsrate,end-of-monthWu-Xiashadowrate

2003 2004 2005 2006 2007 2008 2009 2010 2011 2012 2013 2014 2015 2016-4%

-2%

0%

2%

4%

6%

Cynthia Wu (Notre Dame & NBER) 4 / 34

Page 6: Shadow Interest Rate - CEMLA

Shadow rate Empirical evidence New Keynesian model International evidence

Wu and Xia (JMCB 2016) shadow rate

I Wu-Xia shadow rates for US, Euro area, and UK are available atI Atlanta FedI Haver AnalyticsI Thomson ReutersI Bloomberg

I Wu-Xia shadow rate has been discussed byI Policy makers: then Governor Powell (2013), Altig (2014) of the Atlanta

Fed, Hakkio and Kahn (2014) of the Kansas City FedI Media:Wall Street Journal, Financial Times, The New York Times,

Bloomberg news, Bloomberg Businessweek, Forbes, Business Insider, VOX

Cynthia Wu (Notre Dame & NBER) 5 / 34

Page 7: Shadow Interest Rate - CEMLA

Shadow rate Empirical evidence New Keynesian model International evidence

Outline

1. Wu-Xia shadow rate: Wu and Xia (JMCB 2016)

2. Empirical evidence: Wu and Xia (JMCB 2016), Wu and Zhang (JEDC 2019)

3. New Keynesian model: Wu and Zhang (JEDC 2019), Wu and Zhang (JIE 2019)

4. International evidence: Wu and Zhang (JIE 2019)

Cynthia Wu (Notre Dame & NBER) 6 / 34

Page 8: Shadow Interest Rate - CEMLA

Shadow rate Empirical evidence New Keynesian model International evidence

Shadow rate

Black (1995):

rt = max(st , r)

The shadow rate is affine

st = δ0 + δ′1Xt

I Xt : 3 factors

Cynthia Wu (Notre Dame & NBER) 7 / 34

Page 9: Shadow Interest Rate - CEMLA

Shadow rate Empirical evidence New Keynesian model International evidence

Bond pricing

Physical dynamics:

Xt+1 = µ + ρXt + Σεt+1, εt+1 ∼ N(0, I ).

Risk-neutral Q dynamics:

Xt+1 = µQ + ρQXt + ΣεQt+1, εQt+1Q∼ N(0, I ).

Pricing equation

Pnt = EQt [exp(−rt)Pn−1,t+1]

Yield

ynt = −1

nlog(Pnt)

Forward rate from t + n to t + n + 1

fnt = (n + 1)yn+1,t − nynt

Cynthia Wu (Notre Dame & NBER) 8 / 34

Page 10: Shadow Interest Rate - CEMLA

Shadow rate Empirical evidence New Keynesian model International evidence

Forward rates

Our approximation

fnt ≈ r + σQn g

(an + b′nXt − r

σQn

)where g(z) = zΦ(z) + φ(z).

Details

Forward rate in GATSM

fnt = an + b′nXt .

Cynthia Wu (Notre Dame & NBER) 9 / 34

Page 11: Shadow Interest Rate - CEMLA

Shadow rate Empirical evidence New Keynesian model International evidence

Property of g(.)

−5 −4 −3 −2 −1 0 1 2 3 4 50

1

2

3

4

5

z

y

y = g(z)y = z

f SRnt

≈ r , at the ZLB

≈ an + b′nXt = f Gnt , when interest rates are high

Cynthia Wu (Notre Dame & NBER) 10 / 34

Page 12: Shadow Interest Rate - CEMLA

Shadow rate Empirical evidence New Keynesian model International evidence

State space form

State equation

Xt+1 = µ+ ρXt + Σεt+1, εt+1 ∼ N(0, I )

Observation equation

f ont = r + σQn g

(an + b′nXt − r

σQn

)+ ηnt , ηnt ∼ N(0, ω)

We apply extended Kalman filter for estimation

Cynthia Wu (Notre Dame & NBER) 11 / 34

Page 13: Shadow Interest Rate - CEMLA

Shadow rate Empirical evidence New Keynesian model International evidence

Model fit

Figure: Average forward curve in 2012

1 2 5 7 100

0.5

1

1.5

2

2.5

3

3.5

4SRTSM

fittedobserved

1 2 5 7 100

0.5

1

1.5

2

2.5

3

3.5

4GATSM

fittedobserved

Log likelihood values

I SRTSM: 850; GATSM: 750

Cynthia Wu (Notre Dame & NBER) 12 / 34

Page 14: Shadow Interest Rate - CEMLA

Shadow rate Empirical evidence New Keynesian model International evidence

Approximation error

Average absolute approximation error between 1990M1 and 2013M1 (in basis points)

3M 6M 1Y 2Y 5Y 7Y 10Y

forward rate error 0.01 0.02 0.04 0.13 0.69 1.14 2.29forward rate level 346 357 384 435 551 600 636yield error 0.00 0.01 0.01 0.04 0.24 0.42 0.78

Cynthia Wu (Notre Dame & NBER) 13 / 34

Page 15: Shadow Interest Rate - CEMLA

Shadow rate Empirical evidence New Keynesian model International evidence

Outline

1. Wu-Xia shadow rate: Wu and Xia (JMCB 2016)

2. Empirical evidence: Wu and Xia (JMCB 2016), Wu and Zhang (JEDC 2019)

3. New Keynesian model: Wu and Zhang (JEDC 2019), Wu and Zhang (JIE 2019)

4. International evidence: Wu and Zhang (JIE 2019)

Cynthia Wu (Notre Dame & NBER) 14 / 34

Page 16: Shadow Interest Rate - CEMLA

Shadow rate Empirical evidence New Keynesian model International evidence

Evidence 1: taper tantrum

3M 1Y 3Y 5Y 7Y 10Y0

1

2

Maturity

May 21, 2013May 22, 2013

−3

−2

−1

0

1

2

3

4

5Expected short rate

Apr 2013Apr 2014

Apr 2015Apr 2016

Apr 2017Apr 2018

Apr 2019Apr 2020

Apr 2021Apr 2022

Apr 2023

Apr 2013May 2013

−3

−2

−1

0

1

2

3

4

5Expected shadow rate

Apr 2013Apr 2014

Apr 2015Apr 2016

Apr 2017Apr 2018

Apr 2019Apr 2020

Apr 2021Apr 2022

Apr 2023

Apr 2013May 2013

I May 22, 2013: Bernanke told Congress Fed may decrease the size of QE

Shift in shadow rate summarizes this effect

Cynthia Wu (Notre Dame & NBER) 15 / 34

Page 17: Shadow Interest Rate - CEMLA

Shadow rate Empirical evidence New Keynesian model International evidence

Evidence 2: shadow rate and Fed’s balance sheet

2009 2010 2011 2012 2013 2014−3

−2.5

−2

−1.5

−1

−0.5

0

0.5

1

Per

cent

age

poin

ts

QE1

QE2

OT

QE3

−4.5

−4

−3.5

−3

−2.5

−2

−1.5

−1

Tril

lions

of D

olla

rs

Wu−Xia shadow rate− Fed balance sheet

Correlation

I QE1 - QE3: -0.94

Cynthia Wu (Notre Dame & NBER) 16 / 34

Page 18: Shadow Interest Rate - CEMLA

Shadow rate Empirical evidence New Keynesian model International evidence

Evidence 3: structural break test in VAR

Wu and Xia (JMCB 2016): structural break test

I p = 0.29 for stI p = 0.0007 for EFFR

model details robustness

Cynthia Wu (Notre Dame & NBER) 17 / 34

Page 19: Shadow Interest Rate - CEMLA

Shadow rate Empirical evidence New Keynesian model International evidence

Evidence 4: shadow rate Taylor rule

st = β0 + β1st−1 + β2(yt − ynt ) + β3πt + εt

Full sample

1955 1970 1985 2000 2015-5

0

5

10

15

20

fed funds rate & shadow rateTaylor rule implied

1955 1970 1985 2000 2015-10

-5

0

5

10

Post-85 sample

1985 1991 1997 2003 2009 2015−5

0

5

10

15

fed funds rate & shadow rateTaylor rule implied

1985 1991 1997 2003 2009 2015−5

0

5

No structural breakI F statistics: 0.48 & 1.42I Critical values: 2.64 & 2.68

Cynthia Wu (Notre Dame & NBER) 18 / 34

Page 20: Shadow Interest Rate - CEMLA

Shadow rate Empirical evidence New Keynesian model International evidence

Evidence 5: shadow rate and private rates

2009 2011 2013 2015-5

0

5

10

15

20

Inte

rest

rat

es

Wu-Xia shadow rateGSFCIhigh yield effective yieldBBB effective yieldGZ credit spreadfed funds rate

94

96

98

100

102

104

106

108

110

Gol

dman

Sac

hs F

CI

I private rates are the relevant rates for agents and the economyI correlation with SR: 0.8I private rate = st + rp

Cynthia Wu (Notre Dame & NBER) 19 / 34

Page 21: Shadow Interest Rate - CEMLA

Shadow rate Empirical evidence New Keynesian model International evidence

Summary

Shadow rate summarizes unconventional monetary policy

I Taper tantrum

I Fed’s balance sheet

There is no structural break in

I VAR

I shadow rate Taylor rule

Private rates

I are the relevant interest rates for economic agents

I respond to unconventional monetary policy

I the shadow rate is a sensible summary

Cynthia Wu (Notre Dame & NBER) 20 / 34

Page 22: Shadow Interest Rate - CEMLA

Shadow rate Empirical evidence New Keynesian model International evidence

Outline

1. Wu-Xia shadow rate: Wu and Xia (JMCB 2016)

2. Empirical evidence: Wu and Xia (JMCB 2016), Wu and Zhang (JEDC 2019)

3. New Keynesian model: Wu and Zhang (JEDC 2019), Wu and Zhang (JIE 2019)

4. International evidence: Wu and Zhang (JIE 2019)

Cynthia Wu (Notre Dame & NBER) 21 / 34

Page 23: Shadow Interest Rate - CEMLA

Shadow rate Empirical evidence New Keynesian model International evidence

Shadow rate New Keynesian model

Definition 1

The shadow rate New Keynesian model consists of the shadow rate IScurve

yt = − 1

σ(st − Etπt+1 − s) + Etyt+1,

New Keynesian Phillips curve

πt = βEtπt+1 + κ(yt − ynt ),

and shadow rate Taylor rule

st = φsst−1 + (1 − φs) [φy (yt − ynt ) + φππt + s] .

QE

Cynthia Wu (Notre Dame & NBER) 22 / 34

Page 24: Shadow Interest Rate - CEMLA

Shadow rate Empirical evidence New Keynesian model International evidence

Outline

1. Wu-Xia shadow rate: Wu and Xia (JMCB 2016)

2. Empirical evidence: Wu and Xia (JMCB 2016), Wu and Zhang (JEDC 2019)

3. New Keynesian model: Wu and Zhang (JEDC 2019), Wu and Zhang (JIE 2019)

4. International evidence: Wu and Zhang (JIE 2019)

Cynthia Wu (Notre Dame & NBER) 23 / 34

Page 25: Shadow Interest Rate - CEMLA

Shadow rate Empirical evidence New Keynesian model International evidence

Taylor rule

Definition

I rt : observed policy rate

I st : Taylor rule implied

Cases

I Normal times: rt = stI ELB:

rt = λst

I λ = 0: Standard modelI λ = 1: UMP behaves the same as normal times; Wu and Zhang (2017)I 0 < λ < 1: partially active UMPI λ > 1: hyper active UMP

Cynthia Wu (Notre Dame & NBER) 24 / 34

Page 26: Shadow Interest Rate - CEMLA

Shadow rate Empirical evidence New Keynesian model International evidence

VAR: how large is λ?

Model implication for a negative TFP shock

0 20 40

−0.3

−0.2

−0.1

0

0.1

0.2

0.3

0.4

y%

ELB + UMPELBnormal times

Cynthia Wu (Notre Dame & NBER) 25 / 34

Page 27: Shadow Interest Rate - CEMLA

Shadow rate Empirical evidence New Keynesian model International evidence

VAR: how large is λ?

I 2 variables: growth rate of labor productivity and per-capita hourssimilar to Debortoli, Galı, and Gambetti (2016)

I Identification: Cholesky decomposition

I quarterly VAR(1)

Benefits of the VAR

I Simple and robust

I Does not depend on any one shadow rate

Samples

Cynthia Wu (Notre Dame & NBER) 26 / 34

Page 28: Shadow Interest Rate - CEMLA

Shadow rate Empirical evidence New Keynesian model International evidence

IRF of output to a productivity shock: US

1 5 10 15−0.8

−0.6

−0.4

−0.2

0US

normal timesELB

Conclusion: λ ≈ 1Cynthia Wu (Notre Dame & NBER) 27 / 34

Page 29: Shadow Interest Rate - CEMLA

Shadow rate Empirical evidence New Keynesian model International evidence

IRF of output to a productivity shock: Euro area

1 5 10 15−0.6

−0.4

−0.2

0

0.2

0.4Euro area

Conclusion: 0 < λ < 1Cynthia Wu (Notre Dame & NBER) 28 / 34

Page 30: Shadow Interest Rate - CEMLA

Shadow rate Empirical evidence New Keynesian model International evidence

IRF of output to a productivity shock: UK

1 5 10 15−1

−0.8

−0.6

−0.4

−0.2

0UK

Conclusion: λUS ≈ 1 > λEuro > λUK > 0Cynthia Wu (Notre Dame & NBER) 29 / 34

Page 31: Shadow Interest Rate - CEMLA

Shadow rate Empirical evidence New Keynesian model International evidence

Taylor rule: quantify λ

Why Taylor rule? It gives us a quantitative value of λ

Basic idea: compare what has been done at the ELB with the interest rateimplied by the historical Taylor rule

Cynthia Wu (Notre Dame & NBER) 30 / 34

Page 32: Shadow Interest Rate - CEMLA

Shadow rate Empirical evidence New Keynesian model International evidence

United States

I pre-ELB: 1985Q2 - 2007Q4, ELB: 2009Q1 - 2015Q4

I Simple method: 1.02I Iterative method: 1.12

Vary pre-ELB sample: t0 ∈ 1982Q1 : 1990Q1, t1 ∈ 2003Q1 : 2008Q4

0.9 1 1.1 1.2 1.3 1.40

50

100

150

200

250

300

350

400simple

0 0.5 1 1.5 2 2.5 30

50

100

150

200

250

300iterative

Median (std): simple 1.03 (0.065), iterative 1.19 (0.45)Cynthia Wu (Notre Dame & NBER) 31 / 34

Page 33: Shadow Interest Rate - CEMLA

Shadow rate Empirical evidence New Keynesian model International evidence

Euro area and UK

I Euro area: simple 0.998(0.031), iterative 0.63(1.07)

I UK: simple 0.98(0.10), iterative 0.39(4.10)

Again, we conclude λUS ≈ 1 > λEuro > λUK > 0

Cynthia Wu (Notre Dame & NBER) 32 / 34

Page 34: Shadow Interest Rate - CEMLA

Shadow rate Empirical evidence New Keynesian model International evidence

Conclusion

Empirically, we find

I λUS ≈ 1 > λEuro > λUK > 0

Cynthia Wu (Notre Dame & NBER) 33 / 34

Page 35: Shadow Interest Rate - CEMLA

Shadow rate Empirical evidence New Keynesian model International evidence

Cynthia Wu (Notre Dame & NBER) 34 / 34

Page 36: Shadow Interest Rate - CEMLA

Shadow rate

FAVAR

Replace the fed funds rate with st in Bernanke, Boivin, and Eliasz (2005)

Y mt = am + bxx

mt + bsst + ηmt , ηmt ∼ N(0,Ω)

I Y mt : 97 economic variables from 1960 to 2013

I xmt : 3 underlying macro factors

Factor dynamics:

xmt = µx + ρxxXm

t−1 + uxt

+ 1(t<December 2007)ρxs1 St−1 + 1(December 2007≤t≤June 2009)ρ

xs2 St−1 + 1(t>June 2009)ρ

xs3 St−1

I monthly VAR(13)

Null hypothesisH0 : ρxs1 = ρxs3

back

Cynthia Wu (Notre Dame & NBER) 35 / 34

Page 37: Shadow Interest Rate - CEMLA

Shadow rate

Robustness

p-value for ρxs1 = ρxs3 p-value for ρsx1 = ρsx3

Baseline 0.29 1.00A1 estimate r 0.18 1.00A2 2-factor SRTSM 0.13 0.97A3 Fama-Bliss 0.38 1.00A4 5-factor FAVAR 0.70 1.00A5 6-lag FAVAR 0.09 0.98

7-lag FAVAR 0.19 0.9712-lag FAVAR 0.22 1.00

back

Cynthia Wu (Notre Dame & NBER) 36 / 34

Page 38: Shadow Interest Rate - CEMLA

Shadow rate

Samples

pre-ELB and ELB samples

I US: 1985Q2 - 2007Q4 and 2009Q1 - 2015Q4

I Euro area: 1999Q1 - 2009Q1 and 2009Q2 - 2017Q4

I UK: 1993Q1 - 2009Q1 and 2009Q2 - 2017Q4

Back

Cynthia Wu (Notre Dame & NBER) 37 / 34