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AMODEL OF S ECULAR S TAGNATION Gauti B. Eggertsson and Neil R. Mehrotra Brown University BIS Research Meetings March 11, 2015 1/38
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Page 1: Gauti B. Eggertsson and Neil R. Mehrotra · 2015-03-19 · A MODEL OF SECULAR STAGNATION Gauti B. Eggertsson and Neil R. Mehrotra Brown University BIS Research Meetings March 11,

A MODEL OF SECULAR STAGNATION

Gauti B. Eggertsson and Neil R. Mehrotra

Brown University

BIS Research MeetingsMarch 11, 2015

1 / 38

Page 2: Gauti B. Eggertsson and Neil R. Mehrotra · 2015-03-19 · A MODEL OF SECULAR STAGNATION Gauti B. Eggertsson and Neil R. Mehrotra Brown University BIS Research Meetings March 11,

SECULAR STAGNATION HYPOTHESIS

I wonder if a set of older ideas . . . under the phrase secularstagnation are not profoundly important in understanding Japan’sexperience, and may not be without relevance to America’sexperience — Lawrence Summers

Original hypothesis:

I Alvin Hansen (1938)I Reduction in population growth and investment opportunitiesI Concerns about insufficient demand ended with WWII and

subsequent baby boom

Secular stagnation resurrected:

I Lawrence Summers (2013)I Highly persistent decline in the natural rate of interestI Chronically binding zero lower bound

2 / 38

Page 3: Gauti B. Eggertsson and Neil R. Mehrotra · 2015-03-19 · A MODEL OF SECULAR STAGNATION Gauti B. Eggertsson and Neil R. Mehrotra Brown University BIS Research Meetings March 11,

WHY ARE WE SO CONFIDENT INTEREST RATES

WILL RISE SOON?

Interest rates in the US during the Great Depression:

I Started falling in 1929I Reached zero in 1933I Interest rates only started increasing in 1947

Started dropping in Japan in 1994:I Remains at zero today

Why are we so confident interest rates are increasing in the next fewyears?

Interest Rates, 1929-1951

3 / 38

Page 4: Gauti B. Eggertsson and Neil R. Mehrotra · 2015-03-19 · A MODEL OF SECULAR STAGNATION Gauti B. Eggertsson and Neil R. Mehrotra Brown University BIS Research Meetings March 11,

SHORTCOMINGS OF SOME EXISTING MODELS

Representative agent models:

rss =1β

I Real interest rate must be positive in steady stateI Households problem not well defined if β ≥ 1I ZLB driven by temporary shocks to discount rate (Eggertsson

and Woodford (2003))

Patient-impatient agent models:I Steady state typically pinned down by the discount factor of the

representative saver (Eggertsson and Krugman (2012))I Deleveraging only has temporary effect

4 / 38

Page 5: Gauti B. Eggertsson and Neil R. Mehrotra · 2015-03-19 · A MODEL OF SECULAR STAGNATION Gauti B. Eggertsson and Neil R. Mehrotra Brown University BIS Research Meetings March 11,

QUESTION AND APPROACH

QuestionI Can we formalize the idea of secular stagnation?I Is a permanent slump a theoretical possibility?

ElementsI Permanently binding zero lower bound:

I Three-generation OLG model (Samuelson, 1958)

I Natural rate that can be permanently negative

I Permanent slump in output:I Downward nominal wage rigidity with partial adjustment

I Persistent slump in periods of deflation

5 / 38

Page 6: Gauti B. Eggertsson and Neil R. Mehrotra · 2015-03-19 · A MODEL OF SECULAR STAGNATION Gauti B. Eggertsson and Neil R. Mehrotra Brown University BIS Research Meetings March 11,

PREVIEW OF RESULTSNegative natural rate of interest can be triggered by:

I Deleveraging shockI Slowdown in population growthI Increase in income inequalityI Fall in relative price of investment

Stagnation steady state

I Permanently binding zero lower boundI Low inflation or deflationI Permanent shortfall in output from potential

Monetary and fiscal policy responses

I Raising the inflation targetI Increases in public debtI Increases in government purchases

6 / 38

Page 7: Gauti B. Eggertsson and Neil R. Mehrotra · 2015-03-19 · A MODEL OF SECULAR STAGNATION Gauti B. Eggertsson and Neil R. Mehrotra Brown University BIS Research Meetings March 11,

ECONOMIC ENVIRONMENT

ENDOWMENT ECONOMY

I Time: t = 0, 1, 2, ...

I Goods: consumption good (c)

I Agents: 3-generations: iε {y, m, o}

I Assets: riskless bonds (Bi)

I Technology: exogenous borrowing constraint D

7 / 38

Page 8: Gauti B. Eggertsson and Neil R. Mehrotra · 2015-03-19 · A MODEL OF SECULAR STAGNATION Gauti B. Eggertsson and Neil R. Mehrotra Brown University BIS Research Meetings March 11,

HOUSEHOLDS

Objective function:

maxCy

t,,Cmt+1,Co

t+2

U = Et

{log(

Cyt

)+ β log

(Cm

t+1)+ β2 log

(Co

t+2)}

Budget constraints:

Cyt = By

t

Cmt+1 = Ym

t+1 − (1 + rt)Byt + Bm

t+1

Cot+2 = Yo

t+2 − (1 + rt+1)Bmt+1

(1 + rt)Bit ≤ Dt

8 / 38

Page 9: Gauti B. Eggertsson and Neil R. Mehrotra · 2015-03-19 · A MODEL OF SECULAR STAGNATION Gauti B. Eggertsson and Neil R. Mehrotra Brown University BIS Research Meetings March 11,

CONSUMPTION AND SAVING

Credit-constrained youngest generation:

Cyt = By

t =Dt

1 + rt

Saving by the middle generation:

1Cm

t= βEt

1 + rt

Cot+1

Spending by the old:

Cot = Yo

t − (1 + rt−1)Bmt−1

9 / 38

Page 10: Gauti B. Eggertsson and Neil R. Mehrotra · 2015-03-19 · A MODEL OF SECULAR STAGNATION Gauti B. Eggertsson and Neil R. Mehrotra Brown University BIS Research Meetings March 11,

DETERMINATION OF THE REAL INTEREST RATE

Asset market equilibrium:

NtByt = −Nt−1Bm

t

(1 + gt)Byt = −Bm

t

Demand and supply of loans:

Ldt =

1 + gt

1 + rtDt

Lst =

β

1 + β(Ym

t −Dt−1)−1

1 + β

Yot+1

1 + rt

10 / 38

Page 11: Gauti B. Eggertsson and Neil R. Mehrotra · 2015-03-19 · A MODEL OF SECULAR STAGNATION Gauti B. Eggertsson and Neil R. Mehrotra Brown University BIS Research Meetings March 11,

DETERMINATION OF THE REAL INTEREST RATE

Expression for the real interest rate (perfect foresight):

1 + rt =1 + β

β

(1 + gt)Dt

Ymt −Dt−1

+1β

Yot+1

Ymt −Dt−1

Determinants of the real interest rate:I Tighter collateral constraint reduces the real interest rateI Lower rate of population growth reduces the real interest rateI Higher middle age income reduces real interest rateI Higher old income increases real interest rate

11 / 38

Page 12: Gauti B. Eggertsson and Neil R. Mehrotra · 2015-03-19 · A MODEL OF SECULAR STAGNATION Gauti B. Eggertsson and Neil R. Mehrotra Brown University BIS Research Meetings March 11,

EFFECT OF A DELEVERAGING SHOCK

0.80  

0.85  

0.90  

0.95  

1.00  

1.05  

1.10  

1.15  

1.20  

0.200   0.220   0.240   0.260   0.280   0.300  

Loans  

Gross  Real  Interest  R

ate  

Loan  Supply  

Loan  Demand  

A  

B  

C  

D  

12 / 38

Page 13: Gauti B. Eggertsson and Neil R. Mehrotra · 2015-03-19 · A MODEL OF SECULAR STAGNATION Gauti B. Eggertsson and Neil R. Mehrotra Brown University BIS Research Meetings March 11,

INCOME INEQUALITY AND REAL INTEREST

RATE

Credit constrained middle income:I Fraction ηs of middle income households are credit constrainedI True for low enough income in middle generation and high

enough income in retirementI Fraction 1− ηs lend to both young and constrained

middle-generation households

Expression for the real interest rate:

1 + rt =1 + β

β

(1 + gt + ηs)Dt

(1− ηs)(

Ym,ht −Dt−1

) +1

β (1− ηs)

Yot+1(

Ym,ht −Dt−1

)

13 / 38

Page 14: Gauti B. Eggertsson and Neil R. Mehrotra · 2015-03-19 · A MODEL OF SECULAR STAGNATION Gauti B. Eggertsson and Neil R. Mehrotra Brown University BIS Research Meetings March 11,

PRICE LEVEL DETERMINATION

Euler equation for nominal bonds:

1Cm

t= βEt

1Co

t+1(1 + it)

Pt

Pt+1

it ≥ 0

Bound on steady state inflation:

Π̄ ≥ 11 + r

I If steady state real rate is negative, steady state inflation must bepositive

I No equilibrium with stable inflationI But what happens when prices are NOT flexible and the central

bank does not tolerate inflation?

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Page 15: Gauti B. Eggertsson and Neil R. Mehrotra · 2015-03-19 · A MODEL OF SECULAR STAGNATION Gauti B. Eggertsson and Neil R. Mehrotra Brown University BIS Research Meetings March 11,

AGGREGATE SUPPLY

Output and labor demand:

Yt = Lαt

Wt

Pt= αLα−1

t

Labor supply:I Middle-generation households supply a constant level of labor L̄I Implies a constant market clearing real wage W̄ = αL̄α−1

I Implies a constant full-employment level of output: Yfe = L̄α

15 / 38

Page 16: Gauti B. Eggertsson and Neil R. Mehrotra · 2015-03-19 · A MODEL OF SECULAR STAGNATION Gauti B. Eggertsson and Neil R. Mehrotra Brown University BIS Research Meetings March 11,

DOWNWARD NOMINAL WAGE RIGIDITY

Partial wage adjustment:

Wt = max{

W̃t, PtαL̄α−1}

where W̃t = γWt−1 + (1− γ)PtαL̄α−1

Wage rigidity and unemployment:

I W̃t is a wage normI If real wages exceed market clearing level, employment is

rationedI Unemployment: Ut = L̄− Lt

I Similar assumption in Kocherlakota (2013) and Schmitt-Groheand Uribe (2013)

16 / 38

Page 17: Gauti B. Eggertsson and Neil R. Mehrotra · 2015-03-19 · A MODEL OF SECULAR STAGNATION Gauti B. Eggertsson and Neil R. Mehrotra Brown University BIS Research Meetings March 11,

DERIVATION OF AGGREGATE SUPPLY

With inflation:

wt = W̄ = αL̄(α−1)

Yt = Yfe

With deflation:

wt = γwt−1

Πt+ (1− γ) W̄

wt = αLα−1t

Yt = Lαt

17 / 38

Page 18: Gauti B. Eggertsson and Neil R. Mehrotra · 2015-03-19 · A MODEL OF SECULAR STAGNATION Gauti B. Eggertsson and Neil R. Mehrotra Brown University BIS Research Meetings March 11,

AGGREGATE SUPPLY RELATION

0.80  

0.85  

0.90  

0.95  

1.00  

1.05  

1.10  

1.15  

1.20  

0.80   0.85   0.90   0.95   1.00   1.05   1.10  

Output  

Gross  Infla5o

n  Ra

te  

Aggregate  Supply  

18 / 38

Page 19: Gauti B. Eggertsson and Neil R. Mehrotra · 2015-03-19 · A MODEL OF SECULAR STAGNATION Gauti B. Eggertsson and Neil R. Mehrotra Brown University BIS Research Meetings March 11,

DERIVATION OF AGGREGATE DEMAND

Monetary policy rule:

1 + it = max

(1, (1 + i∗)

(Πt

Π∗

)φπ)

Above binding ZLB:

1 + i∗

Πt+1

(Πt

Π∗

)φπ

=1 + β

β

(1 + gt)Dt

Yt −Dt−1

Binding ZLB:

1Πt+1

=1 + β

β

(1 + gt)Dt

Yt −Dt−1

19 / 38

Page 20: Gauti B. Eggertsson and Neil R. Mehrotra · 2015-03-19 · A MODEL OF SECULAR STAGNATION Gauti B. Eggertsson and Neil R. Mehrotra Brown University BIS Research Meetings March 11,

FULL EMPLOYMENT STEADY STATE

0.80  

0.85  

0.90  

0.95  

1.00  

1.05  

1.10  

1.15  

1.20  

0.80   0.85   0.90   0.95   1.00   1.05   1.10  

Output  

Gross  Infla5o

n  Ra

te  

Aggregate  Supply  

FE  Steady  State   Aggregate  

Demand  

Parameter Values

20 / 38

Page 21: Gauti B. Eggertsson and Neil R. Mehrotra · 2015-03-19 · A MODEL OF SECULAR STAGNATION Gauti B. Eggertsson and Neil R. Mehrotra Brown University BIS Research Meetings March 11,

EFFECT OF A COLLATERAL SHOCK

0.80  

0.85  

0.90  

0.95  

1.00  

1.05  

1.10  

1.15  

1.20  

0.80   0.85   0.90   0.95   1.00   1.05   1.10  

Output  

Gross  Infla5o

n  Ra

te  

Aggregate  Supply  

Defla5on  Steady  State  

AD1  

AD2  

21 / 38

Page 22: Gauti B. Eggertsson and Neil R. Mehrotra · 2015-03-19 · A MODEL OF SECULAR STAGNATION Gauti B. Eggertsson and Neil R. Mehrotra Brown University BIS Research Meetings March 11,

PROPERTIES OF THE STAGNATION STEADY

STATE

Long slump:I Binding zero lower bound so long as natural rate is negativeI Deflation raises real wages above market-clearing levelI Output persistently below full-employment level

Existence and stability:I Secular stagnation steady state exists so long as γ > 0I If Π∗ = 1, secular stagnation steady state is unique and

determinateI Contrast to deflation steady state emphasized in Benhabib,

Schmitt-Grohe and Uribe (2001)

Linearized Conditions

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Page 23: Gauti B. Eggertsson and Neil R. Mehrotra · 2015-03-19 · A MODEL OF SECULAR STAGNATION Gauti B. Eggertsson and Neil R. Mehrotra Brown University BIS Research Meetings March 11,

MONETARY POLICY RESPONSES

Forward guidance:I Extended commitment to keep nominal rates low?I Ineffective if households/firms expect rates to remain low

indefinitelyI IS curve not forward-looking in the same manner as New

Keynesian IS curve

Raising the inflation target:I For sufficiently high inflation target, full employment steady

state exists.I Timidity trap (Krugman (2014))I Multiple determinate steady states

23 / 38

Page 24: Gauti B. Eggertsson and Neil R. Mehrotra · 2015-03-19 · A MODEL OF SECULAR STAGNATION Gauti B. Eggertsson and Neil R. Mehrotra Brown University BIS Research Meetings March 11,

RAISING THE INFLATION TARGET

0.80  

0.85  

0.90  

0.95  

1.00  

1.05  

1.10  

1.15  

1.20  

0.80   0.85   0.90   0.95   1.00   1.05   1.10  

Output  

Gross  Infla5o

n  Ra

te  

Aggregate  Supply  

Full  Employment  Steady  State  

AD2   AD3  

Defla5on  Steady  State  

AD1  

24 / 38

Page 25: Gauti B. Eggertsson and Neil R. Mehrotra · 2015-03-19 · A MODEL OF SECULAR STAGNATION Gauti B. Eggertsson and Neil R. Mehrotra Brown University BIS Research Meetings March 11,

FISCAL POLICY

Fiscal policy and the real interest rate:

Ldt =

1 + gt

1 + rtDt + Bg

t

Lst =

β

1 + β(Ym

t −Dt−1 − Tmt )−

11 + β

Yot+1 − To

t+11 + rt

Government budget constraint:

Bgt + Ty

t (1 + gt) + Tmt +

11 + gt−1

Tot = Gt +

1 + rt

1 + gt−1Bg

t−1

Fiscal instruments:

Gt, Bgt , Ty

t , Tmt , To

t

25 / 38

Page 26: Gauti B. Eggertsson and Neil R. Mehrotra · 2015-03-19 · A MODEL OF SECULAR STAGNATION Gauti B. Eggertsson and Neil R. Mehrotra Brown University BIS Research Meetings March 11,

TEMPORARY INCREASE IN PUBLIC DEBT

Under constant population and set Gt = Tyt = Bg

t−1 = 0:

Tmt = −Bg

t

Tot+1 = (1 + rt)Bg

t

Implications for natural rate:I Loan demand and loan supply effects cancel outI Temporary increases in public debt ineffective in raising real rateI Temporary monetary expansion equivalent to temporary

expansion in public debt at the zero lower boundI Effect of an increase in public debt depends on beliefs about

future fiscal policy

26 / 38

Page 27: Gauti B. Eggertsson and Neil R. Mehrotra · 2015-03-19 · A MODEL OF SECULAR STAGNATION Gauti B. Eggertsson and Neil R. Mehrotra Brown University BIS Research Meetings March 11,

PERMANENT INCREASE IN PUBLIC DEBT

Consider steady state following fiscal rule:

To = β (1 + r)Tm

Ld =1 + g1 + r

D + Bg

Ls =β

1 + β(Ym −D)− 1

1 + β

Yo

1 + r

Implications for natural rate:I Changes in taxation have no effects on loan supplyI Permanent rise in public debt always raises the real rateI Equivalent to helicopter drop at the zero lower boundI Public debt circumvents the tightening credit friction (Woodford

(1990))

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Page 28: Gauti B. Eggertsson and Neil R. Mehrotra · 2015-03-19 · A MODEL OF SECULAR STAGNATION Gauti B. Eggertsson and Neil R. Mehrotra Brown University BIS Research Meetings March 11,

GOVERNMENT PURCHASES MULTIPLIER

Slope of the AD and AS curves:

ψ =1 + β

β(1 + g)D

κ =1− α

α

1− γ

γ

Purchases multiplier at the zero lower bound:

Financing Multiplier Value

Increase in public debt 1+ββ

11−κψ > 2

Tax on young generation 0 0

Tax on middle generation 11−κψ > 1

Tax on old generation − 1+gβ

11−κψ < 0

28 / 38

Page 29: Gauti B. Eggertsson and Neil R. Mehrotra · 2015-03-19 · A MODEL OF SECULAR STAGNATION Gauti B. Eggertsson and Neil R. Mehrotra Brown University BIS Research Meetings March 11,

EXPANSIONARY FISCAL POLICY

0.80  

0.85  

0.90  

0.95  

1.00  

1.05  

1.10  

1.15  

1.20  

0.80   0.85   0.90   0.95   1.00   1.05   1.10  

Output  

Gross  Infla5o

n  Ra

te  

Aggregate  Supply  

Full  Employment  Steady  State  

AD2   AD3  

Defla5on  Steady  State  

29 / 38

Page 30: Gauti B. Eggertsson and Neil R. Mehrotra · 2015-03-19 · A MODEL OF SECULAR STAGNATION Gauti B. Eggertsson and Neil R. Mehrotra Brown University BIS Research Meetings March 11,

CAPITAL AND SECULAR STAGNATION

Rental rate and real interest rate:

rkt = pk

t − pkt+1

1− δ

1 + rt≥ 0

rss ≥ −δ

I Negative real rate now constrained by fact that rental rate mustbe positive

Relative price of capital goods:I Decline in relative price of capital goodsI Need less savings to build the same capital stockI Global decline in price of capital goods (Karabarbounis and

Neiman, 2014)

Land

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Page 31: Gauti B. Eggertsson and Neil R. Mehrotra · 2015-03-19 · A MODEL OF SECULAR STAGNATION Gauti B. Eggertsson and Neil R. Mehrotra Brown University BIS Research Meetings March 11,

GOING FORWARD: FINANCIAL STABILITY

Low equilibrium rates:I Possibility of rational asset price bubblesI Dynamic inefficiencyI Future dividends relatively more important than current

dividendsI Bubbles may be welfare-enhancing

Policy responses:I Higher inflation target leaves natural rate unchangedI Favor fiscal policy responses that raise natural rate of interest

rather than accommodate lower natural rates

31 / 38

Page 32: Gauti B. Eggertsson and Neil R. Mehrotra · 2015-03-19 · A MODEL OF SECULAR STAGNATION Gauti B. Eggertsson and Neil R. Mehrotra Brown University BIS Research Meetings March 11,

CONCLUSIONS

Policy implications:I Higher inflation target neededI Limits to forward guidanceI Role for fiscal policyI Possible implications for financial stability

Key takeaway:I NOT that we will stay in a slump foreverI Slump of arbitrary durationI OLG framework to model interest rates

32 / 38

Page 33: Gauti B. Eggertsson and Neil R. Mehrotra · 2015-03-19 · A MODEL OF SECULAR STAGNATION Gauti B. Eggertsson and Neil R. Mehrotra Brown University BIS Research Meetings March 11,

Additional Slides

33 / 38

Page 34: Gauti B. Eggertsson and Neil R. Mehrotra · 2015-03-19 · A MODEL OF SECULAR STAGNATION Gauti B. Eggertsson and Neil R. Mehrotra Brown University BIS Research Meetings March 11,

US INTEREST RATES, 1929-1951INTEREST RATE ON 3-MONTH TREASURY BILLS

-1!

0!

1!

2!

3!

4!

5!

6!1929!

1930!

1931!

1932!

1933!

1934!

1935!

1936!

1937!

1938!

1939!

1940!

1941!

1942!

1943!

1944!

1945!

1946!

1947!

1948!

1949!

1950!

1951!

Source: NBER Macrohistory Database

Back

34 / 38

Page 35: Gauti B. Eggertsson and Neil R. Mehrotra · 2015-03-19 · A MODEL OF SECULAR STAGNATION Gauti B. Eggertsson and Neil R. Mehrotra Brown University BIS Research Meetings March 11,

PARAMETER VALUES IN NUMERICAL

EXAMPLES

Description Parameter Value

Population growth g 0.2

Collateral constraint D 0.28

Discount rate β 0.77

Labor share α 0.7

Wage adjustment γ 0.3

Taylor coefficient φπ 2

Gross inflation target Π∗ 1.01

Labor supply L 1

Depreciation δ 0.79

Back

35 / 38

Page 36: Gauti B. Eggertsson and Neil R. Mehrotra · 2015-03-19 · A MODEL OF SECULAR STAGNATION Gauti B. Eggertsson and Neil R. Mehrotra Brown University BIS Research Meetings March 11,

DYNAMIC EFFICIENCY

Planner’s optimality conditions:

Co

Cm= β (1 + g)

(1− α)K−α = 1− 1− δ

1 + g

D (1 + g) + Cm +1

1 + gCo = K1−αL̄α − K

(1− 1− δ

1 + g

)Implications:

I Competitive equilibrium does not necessarily coincide with constrainedoptimal allocation

I If r > g, steady state of our model with capital is dynamically efficient

I Negative natural rate only implies dynamic inefficiency if populationgrowth rate is negative

36 / 38

Page 37: Gauti B. Eggertsson and Neil R. Mehrotra · 2015-03-19 · A MODEL OF SECULAR STAGNATION Gauti B. Eggertsson and Neil R. Mehrotra Brown University BIS Research Meetings March 11,

DYNAMIC EFFICIENCY

Is dynamic efficiency empirically plausible?

I Classic study in Abel, Mankiw, Summers and Zeckhauser (1989) says no

I Revisited in Geerolf (2013) and cannot reject condition for dynamicinefficiency in developed economies today

Absence of risk premia:

I No risk premia on capital in our model

I Negative short-term natural rate but positive net return on capital

I Abel et al. (2013) emphasize that low real interest rates not inconsistentwith dynamic efficiency

Back

37 / 38

Page 38: Gauti B. Eggertsson and Neil R. Mehrotra · 2015-03-19 · A MODEL OF SECULAR STAGNATION Gauti B. Eggertsson and Neil R. Mehrotra Brown University BIS Research Meetings March 11,

LAND

Land with dividends:

plandt = Dt +

plandt+1

1 + rt

I Land that pays a real dividend rules out a secular stagnation

Land without dividends:I If r > 0, price of land equals its fundamental value

I If r < 0, price of land is indeterminate and land offers a negative return r

Absence of risk premia:I No risk premia on land

I Negative short-term natural rate but positive net return on capital

Back

38 / 38

Page 39: Gauti B. Eggertsson and Neil R. Mehrotra · 2015-03-19 · A MODEL OF SECULAR STAGNATION Gauti B. Eggertsson and Neil R. Mehrotra Brown University BIS Research Meetings March 11,

LINEARIZED EQUILIBRIUM CONDITIONS

Linearized AS and AD curves:

it = Etπt+1 − sy (yt − gt) + (1− sw)Et (yt+1 − gt+1) + swdt + sddt−1

yt = γwyt−1 + γwα

1− απt

Elements:

I Exogenous shocks: gt, dt

I Retains forward-looking intertemporal IS curve of New Keynesianmodel

I IS curve is "less" forward-looking" than New Keynesian version

Back

39 / 38


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