shadow interest rate - cemla
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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
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
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
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
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%
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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
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
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
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
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 .
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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
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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
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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
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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
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
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
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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
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
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
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
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
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
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
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
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
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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
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
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
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
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
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
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
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
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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
Shadow rate Empirical evidence New Keynesian model International evidence
Cynthia Wu (Notre Dame & NBER) 34 / 34
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
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
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
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