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Publicly Available Published by De Gruyter January 22, 2016

Structural changes in inflation dynamics: multiple breaks at different dates for different parameters

  • Yunjong Eo EMAIL logo

Abstract

I consider complicated patterns of structural breaks in postwar quarterly US inflation rates based on the CPI and the GDP deflator over the period from 1953:Q1 to 2013:Q4. Bayesian model selection procedures suggest that the two inflation measures had distinct structural changes in different parameters as well as at different dates. CPI inflation experienced a dramatic drop in persistence around the early 1980s, but GDP deflator inflation remains persistent throughout the postwar sample period. The residual variance for both inflation measures switched from a low volatility regime to a high volatility regime in the early 1970s, but returned to another low volatility regime at different dates: the early 1980s for GDP deflator inflation and the early 1990s for CPI inflation. The residual variance for CPI inflation has increased again since the early 2000s, while GDP deflator inflation has remained less volatile. I do not find evidence of a structural shift in the unconditional mean of either measure of inflation. When reviewing the recent literature, considerable controversy exists over the structural break in inflation persistence around the early 1980s but this appears to be dependent on the measures of inflation, as highlighted by the empirical findings in this paper.

JEL: C11; C22; E31

1 Introduction

In this paper, I make inferences about complicated patterns of structural breaks in inflation dynamics. An autoregressive (AR) model is used for studying structural shifts in three parameter groups: the unconditional mean, a group of autoregressive coefficients, and the residual variance. The choice of parameter groups are potentially related to structural interpretations of changes in inflation dynamics. Some parameters could have a different number of structural breaks and/or at different dates from others. Also, structural breaks are modeled as abrupt changes to identify potential regime shifts in economic structure such as a long-run inflation target, monetary policy, and price-setting behavior.[1]

Changes in the group of AR coefficients, related to inflation persistence, can be understood through shifts in structural parameters in the New Keynesian Phillips curve. Shifts in inflation persistence can be caused by changes in firms’ price setting behavior, marginal cost dynamics, or monetary policy.[2] Shifts in inflation persistence have crucial implications for policymakers. For example, Solow (1968) and Tobin (1968) consider a test for the natural rate hypothesis using a simple Phillips curve with unemployment rate. When inflation is considered to be less persistent, the natural rate hypothesis is likely to be rejected. In such a case, policymakers may feel a strong temptation to exploit an illusory inflation-unemployment trade-off, resulting in high inflation as in the 1970s.[3]

The unconditional mean in AR models is associated with trend inflation, which is potentially set by the cental bank. Thus, one can make inferences about shifts in the central bank’s long-run inflation target when studying structural breaks in the unconditional mean. However, the changes in trend inflation would not be identified if we consider breaks in the intercept because the shifts in the intercept may provide mixed information on breaks in the unconditional mean and persistence.

In addition, Stock and Watson (2003) and Kim, Nelson and Piger (2004) suggest the possibility of structural changes in the volatility of inflation as potentially related to real activity and supply shocks. This shift can be captured when taking into account the change in the residual variance.

In short, these complex patterns of structural breaks in different parameters reflect the possibility that the parameter changes are due to the shifts in structural parameters of macroeconomic models.[4] To understand the structural dynamics of inflation clearly, it is essential above all to investigate whether there have been breaks. If so, which parameters are subject to these shifts? Do they undergo these changes at the same time? To answer these questions, it is important to identify the parameters subject to changes at a particular time and distinguish them from unchanged parameters.

I take a Bayesian approach to estimate and compare the complex structural break models, which are potentially non-nested. However, in the literature all the parameters subject to the changes are assumed to have the structural shifts at the same date either in pure or partial structural change models.[5] For example, Chib (1998) considers single-group changepoint models by interpreting structural changes for all the parameters as regime transitions that follow a first-order Markov processes. Wang and Zivot (2000) treat structural break dates as additional parameters and sample break dates from conditional distributions of break dates with flat priors.

Thus, these approaches in the literature are not suitable for making inferences about the complicated patterns of structural changes considered in this paper. To overcome the limitation I modify Chib’s (1998) approach, augmenting each parameter (group) with its corresponding independent regime indicator variable. Note that it is possible to sort several parameters into a group and make the group of parameters undergo structural changes at the same dates, as in the approach for persistence parameters adopted in this paper. The modified approach allows multiple parameters (groups) to undergo mutually independent structural breaks at different dates with the different number of breaks. This multiple-group changepoint model can explore all the possible patterns of structural breaks efficiently. The number of structural breaks and the form of structural change are determined by a Bayesian model selection procedure using Bayes factors. For robustness, I also calculate marginal probabilities for the number of structural breaks in each individual parameter group because the model selection procedure using the Bayes factors chooses only one model.

I employ the modified approach to an autoregressive model for postwar US GDP deflator inflation and CPI inflation by allowing for shifts in the unconditional mean, a group of persistence parameters, and/or the residual variance. The Bayesian model selection procedure shows distinct patterns of structural changes from two different measures of inflation. CPI inflation experienced a dramatic drop in persistence around the early 1980s, but GDP deflator inflation is still persistent. Also, the residual variance for both inflation measures switched from a low volatility regime to a high volatility regime in the early 1970s, but it returned to another low volatility regime at different dates: the early 1980s for GDP deflator inflation and the early 1990s for CPI inflation. The residual variance for CPI inflation has increased again since the early 2000s, while GDP deflator inflation has remained less volatile. This different pattern of changes in the variance is also confirmed using unobserved components model with stochastic volatility in Stock and Watson (2007). However, I do not find evidence of a structural shift in the unconditional mean. The marginal probability calculations for the number of breaks in each individual parameter group also strongly support the model selection results based on the Bayes factors. The structural breaks at different dates reflect the possibility that parameter shifts might be caused by a variety of factors.

The remainder of this paper describes the methods and then discusses the empirical results and how they compare to existing results in the literature.

2 Model specification and Bayesian inference

2.1 Model specification

I consider a pth-order autoregressive model for an analysis of inflation dynamics and the AR(p) model allows for structural breaks in three parameter groups such as (i) the unconditional mean μ, (ii) persistence (ϕ1, …, ϕt) and (iii) the residual variance σ2. I focus on changes in the unconditional mean rather than the intercept because changes in the intercept may contain mixed information on changes in level and persistence. Sims (2001) and Stock (2001) note that allowing for changes in the residual variance helps avoid any potential distortions of identifying structural breaks in coefficients.[6] The AR(p) model with structural breaks is given by

(1)πt=μS1,t+ϕ1,S2,t(πt1μS1,t1)++ϕp,S2,t(πtpμS1,tp)+et,   etN(0,σS3,t2) (1)

where S1,t∈{1, …, M1+1}, S2,t∈{1, …, M2+1}, and S3,t∈{1, …, M3+1} represent the regimes for the unconditional mean parameter with M1 breaks, the persistence parameter group with M2 breaks and the residual variance with M3 breaks, respectively. The nature of the structural breaks in each parameter group is independent of one another in terms of the number and timing of structural changes.

To make inferences about multiple-group changepoint models, I modify Chib’s (1998) approach in which the structural breaks are interpreted as regime transitions. Chib (1998) assumes that all the parameters which undergo the structural changes have the structural shifts at the same dates.[7] Thus, I propose an efficient Bayesian MCMC method that allows for a number of possibilities for the nature of structural breaks. This modified approach is developed to have the following attractive features: (i) model specification of considering multiple structural changes in multiple parameters; (ii) model flexibility in allowing the multiple structural breaks to occur mutually independently at different dates; and (iii) model selection procedure by comparing various potentially non-nested structural break models.

Suppose a multiple-group changepoint model which allows parameters to change at different dates with the different number of breaks.[8] For example, in (1) the model for inflation dynamics may have one break in the unconditional mean, two breaks in persistence, and three breaks in the residual variance. In this case, the modified approach would require only augmentations with three independent latent regime indicator variables (S˜1,T,S˜2,T,S˜3,T), where S˜i,T=[Si,1Si,2Si,T1Si,T] for each parameter group i=1, 2, 3, and three transition probability matrices (P1, P2, P3) corresponding to three parameter groups while the single-group changepoint model is augmented with only one regime indicator variable and one transition probability matrix. Since all the regime indicator variables are mutually independent in the multiple-group changepoint model, the date of regime transition in a parameter is allowed to occur close to that of regime transition in other parameters without any necessary minimum distance unlike the restriction in Levin and Piger (2007).

For a parameter group i, the latent state variable St follows a first-order Markov process with the transition probabilities constrained: for k=1, …, Mt

(2)Pr[Si,t=k|Si,t1=k]=pk,ki and Pr[Si,t=k+1|Si,t1=k]=pk,k+1i=1pk,ki (2)

and

(3)Pr[Si,t=Mi+1|Si,t1=Mi+1]=1   for the last regime Mi+1 (3)

where pk,ki indicates the probability that a regime St for the parameter group i stays in the current regime k. A transition probability matrixPt for the parameter group i can then be formed as a (Mt+1)-by-(Mt+1) matrix with elements containing information about the first-order Markov process in (2) and (3).[9]

A joint posterior density can be obtained as being proportional to a product of a prior density and a likelihood function of Yt=[y1yt]′ such as

π(θ,P|YT)π(θ,P)f(YT|θ,P)

where π(·) denotes a density function; θ=(μ˜,ϕ˜,σ˜2) is a collection of model parameters; μ˜=(μ1,,μM1+1),ϕ˜=(ϕ1,1,,ϕp,1,,ϕ1,M2+1,,ϕp,M2+1), and σ˜2=(σ12,,σM3+12); and P=(P1, P2, P3) is a collection of transition probability matrices. The model parameters, θ=(μ˜,ϕ˜,σ˜2), are then augmented with the transition probability matrices, P=(P1, P2, P3), and the latent regime indicators (S˜1,T,S˜2,T,S˜3,T). The MCMC sampler is developed through a hierarchical specification in which one draws the model parameters conditional on the regime indicators and the observed data; the regime indicators conditional on the model parameters and the observed data; and finally the transition probabilities conditional on the regime indicators via Gibbs sampling. More details for the MCMC sampling algorithm are explained in the Appendix.

2.2 Model selection procedures

I consider two different model selection procedures: (i) the Bayes factor comparison using the marginal likelihoods and (ii) the posterior probability for the number of structural breaks in each individual parameter group by integration. Thus, I find not only the most preferred model based on the Bayes factor but also the marginal probability for the number of breaks in each parameter group for robustness to the model selection results. In this analysis, the maximum number of structural breaks is specified to four for each parameter group and in total, 125 different models for each inflation measure are considered including a model with no break (125=53).

The Bayes factor is presented in favor of the alternative model, M=(M1, M2, M3) versus the most preferred model, =(M1,M2,M3) by

BF=m(YT|=(M1,M2,M3))m(YT|=(M1,M2,M3))

where m(Yt|ℳ=(M1, M2, M3)) is the marginal likelihood for the model with structural breaks of (M1, M2, M3). I calculate the marginal likelihood at the posterior mean. The algorithm to compute the marginal likelihood is described in the Appendix.

I also calculate the posterior probability for the number of structural breaks in each individual parameter group by integrating out the number of breaks in other parameters. For example, the posterior probability for l structural breaks in the parameter μ˜, denoted by M1=l, is given by

(5)Pr(M1=l|YT)=m(YT|M1=l)π(M1=l)i=04m(YT|M1=i)π(M1=i) (5)

where

m(YT|M1=l)=j=04k=04m(YT|M1=l,M2=j,M3=k)π(M2=j,M3=k|M1=l)

is the integrated likelihood when M1=l; π(M1=l) is the prior probability for M1=l; and π(M2=j, M3=k|M1=l) is the joint prior probability for M2=j and M3=k conditional on M1=l. Because all the models are considered a priori equally likely as well as independent, π(M1=l) is equal to 1/5 and π(M2=j, M3=k|M1=l) is equal to 1/25 when the maximum number of structural breaks is specified to four as in this analysis. In fact, the posterior probability of l structural breaks in the parameter μ˜ is simply the sum of posterior probabilities for all the models such that M1=l. For other parameters, ϕ˜ and σ˜2, Pr(M2=j|YT) and Pr(M3=k/Yt) can be easily obtained by using the same approach in (5). Note that all the terms in (5) are readily available when the marginal likelihood calculations are completed.

3 Structural breaks in inflation dynamics

3.1 Data and prior

I consider two different quarterly US inflation measures based on the consumer price index (CPI) and the GDP deflator.[10] Each inflation is defined as 100 times the log change in the corresponding price index for the period of 1953:Q1–2013:Q4.

Figure 1 depicts the two inflation series. Both inflation measures appear to be less volatile for the “Great Moderation” period since the early 1980s but CPI inflation has been recently more volatile. Moreover, CPI inflation appears to be less persistent than GDP deflator inflation. Table 1 presents summary statistics over the sample period. CPI inflation has a slightly higher mean, is less persistent, and more volatile than for GDP deflator inflation. In addition, the correlation between the two inflation measures is 0.78. Thus, the timing and the number of structural changes might be different across model parameters such as the unconditional mean, persistence, and the residual variance as well as across the different measures of inflation. In this case, the multiple-group changepoint model can effectively detect the structural changes in individual parameter groups.

Figure 1: US inflation rates: CPI and GDP deflator (quarterly percentage change): 1953:Q1–2013:Q4.
Figure 1:

US inflation rates: CPI and GDP deflator (quarterly percentage change): 1953:Q1–2013:Q4.

Table 1

Summary statistics for inflation series: 1953:Q1–2013:Q4.

SeriesMeanSDFirst order autocorr.
CPI0.890.810.61
GDP0.800.570.86
Corr0.78

CPI refers to CPI inflation and GDP refers to GDP deflator inflation.

In this analysis, the lag order p is set to two for both series by the Bayesian information criterion. The diffuse and same prior distributions across different regimes are chosen in order to avoid any distortions from the choice of specific prior distributions when estimating different structural break models. The priors for regression coefficients are distributed with mean zero and variance one (i.e., μ, ϕt~N(0, 1)) and the priors of variance parameters follow an Inverse Gamma distribution such as σ2IG(5.02,1.52) for CPI inflation and σ2IG(4.22,0.52) for GDP deflator inflation. The priors for the variance parameters are set differently reflecting the fact that GDP deflator inflation is more persistent and less volatile than CPI inflation so that the residual variance for the GDP inflation regression is much smaller than for the CPI inflation regression. See the summary statistics in Table 1. The prior of the transition probability that the current regime k stays in the same regime k in the next period is distributed as pt~Beta(10, 0.1). The prior expected duration of a given regime is about 101 quarters and the prior expected number of breaks is 2.4 given the sample size of 241. All the estimations are based on 3000 Gibbs simulations after discarding 3000 burn-ins.[11]

3.2 Empirical findings for CPI inflation

I first discuss model selection results for CPI inflation. Table 2 presents the ten best models based on marginal likelihood calculations among 125 models. The comparison of the marginal likelihoods shows that the most preferred model has one structural break in persistence, three structural breaks in the residual variance, and no structural break in the unconditional mean. The most preferred model clearly dominates the other models in the sense that the Bayes factor is lower than 1/8 in favor of any alternative model.

Table 2

US CPI inflation: model selection.

Model (# of breaks) ℳ=(M1, M2, M3)Log marginal likelihoodBayes factor
(0, 1, 3)–203.551.0000
(1, 1, 3)–205.660.1206
(0, 1, 4)–206.170.0728
(0, 2, 3)–207.360.0221
(0, 1, 2)–207.460.0200
(0, 0, 3)–207.850.0135
(0, 1, 1)–208.160.0099
(1, 1, 4)–208.350.0082
(2, 1, 3)–208.770.0054
(1, 1, 2)–209.040.0041

M1, M2, and M3 denote the number of breaks in the unconditional mean (μ), the persistence (ϕ1, ϕ2), and the residual variance (σ2), respectively. Bayes factors are calculated in favor of the alternative model: BF=m(YT|A)m(YT|=(0,1,3)).

Table 3 lists the marginal posterior probability of the number of structural breaks in individual parameter groups using (5). The highest probability of the number of breaks for each parameter is calculated as follows: 0.89 for no break in the unconditional mean, 0.97 for one break in persistence, and 0.91 for three breaks in the residual variance. This finding from the marginal probability calculations is completely consistent with the model selection of =(M1=0,M2=1,M3=3) based on the Bayes factors.

Table 3

US CPI inflation: posterior probability of the number of structural breaks in individual parameter group.

Parameter# of breaksPosterior probability
Uncond. mean00.89
10.11
20.00
30.00
40.00
Persistence00.01
10.97
20.02
30.00
40.00
Residual variance00.00
10.01
20.02
30.91
40.06

Bold values indicate the highest posterior probability for individual parameter groups.

Table 4 summarizes the posterior distributions with mean and standard deviation and Figure 2 plots the posterior mean and 90% credible band for each parameter group over the sample period. The sum of autoregressive coefficients is used for the measure of persistence. The posterior distributions clearly show that persistence sharply decreased from 0.89 to 0.10 (posterior mean) in the early 1980s while the residual variance switched from a low volatility regime to a high volatility regime around the early 1970s, returned to another low volatility regime around the early 1990s, and then has increased again since the early 2000s.[12] The changes in the residual variance also appear to be abrupt. It is evident that the break point for persistence is different from the break points for the residual variance. Thus, these structural changes could be caused by different sources.

Table 4

US CPI inflation: posterior distributions for the most preferred model [# of breaks (M1,M2,M3)=(0,1,3)].

ParameterPriorPosterior
Regime1Regime2Regime3Regime4
μ0.0000.686
(1.000)(0.070)
ϕ10.0000.4360.086
(1.000)(0.085)(0.126)
ϕ20.0000.4580.013
(1.000)(0.085)(0.116)
p2,ii0.9900.992
(0.030)(0.008)
σ20.5000.1430.4270.1120.678
(0.707)(0.025)(0.103)(0.036)(0.149)
p3,ii0.9900.9870.9860.981
(0.030)(0.012)(0.014)(0.018)

Standard deviations are reported in parentheses.

Figure 2: US CPI inflation: posterior distribution of parameters over time.(A) Unconditional mean, (B) persistence (sum of AR parameters), (C) residual variance.Posterior mean and 90% band are plotted over time. The estimated break dates (posterior mode) are 1981:Q3 for persistence and 1972:Q4, 1991:Q1, and 2001:Q2 for the residual variance.
Figure 2:

US CPI inflation: posterior distribution of parameters over time.

(A) Unconditional mean, (B) persistence (sum of AR parameters), (C) residual variance.

Posterior mean and 90% band are plotted over time. The estimated break dates (posterior mode) are 1981:Q3 for persistence and 1972:Q4, 1991:Q1, and 2001:Q2 for the residual variance.

3.3 Empirical findings for GDP deflator inflation

Now, I apply the modified approach to an AR(2) model for GDP deflator inflation. Table 5 presents calculations for the marginal likelihood and Bayes factor. The marginal likelihood calculations select the model with two breaks in the residual variance only. The Bayes factor between ℳ*=(0, 0, 2) and ℳ=(0, 0, 1), the second preferred model, is 0.61. Table 6 shows the marginal probability for the number of breaks in each parameter group. The posterior probability for two breaks in the residual variance (σ2) is 0.60 and for one break is 0.37 while the posterior probabilities for no break in the unconditional mean (μ) and in persistence (ϕ) are 0.99 and 0.95, respectively. Thus, not only the marginal likelihood comparisons but also the posterior probability calculations produce very strong evidence that the autoregressive model for GDP deflator inflation has no break in the unconditional mean and persistence but the specification for two breaks in the residual variance is slightly more preferred than for one break.[13] This result is also consistent with the finding that evidence for shifts in persistence for GDP deflator inflation is not statistically significant, particularly once allowing for shifts in the residual variance as in Pivetta and Reis (2007) and Stock (2002).

Table 5

US GDP deflator inflation: model selection.

Model (# of breaks) ℳ=(M1, M2, M3)Log marginal likelihoodBayes factor
(0, 0, 2)–23.301.0000
(0, 0, 1)–23.800.6105
(0, 1, 2)–26.180.0561
(0, 0, 3)–26.420.0441
(0, 1, 1)–26.770.0311
(1, 0, 1)–27.880.0103
(1, 0, 2)–27.980.0093
(0, 1, 3)–29.140.0029
(0, 0, 4)–29.730.0016
(0, 2, 2)–30.020.0012

For the proposed approach, M1, M2, and M3 denote the number of breaks in the unconditional mean (μ), the persistence (ϕ1,ϕ2), and the residual variance (σ2), respectively. Bayes factors are calculated in favor of the alternative model: BF=m(YT|A)m(YT|=(0,0,2)).

Table 6

US GDP deflator inflation: posterior probability of the number of structural breaks in individual parameters.

Parameter# of breaksPosterior probability
Uncond. mean00.99
10.01
20.00
30.00
40.00
Persistence00.95
10.05
20.00
30.00
40.00
Residual variance00.00
10.37
20.60
30.03
40.00

Bold values indicate the highest posterior probability for individual parameter groups.

Table 7 summarizes posterior distributions for the parameters in the most preferred model and Figure 3 plots posterior mean and 90% credible band for each parameter group. The residual variance switched from a low volatility regime to a high volatility regime around the early 1970s and then returned to another low volatility regime around the early 1980s. In addition, the residual variance for the first regime appears to be bigger than that for the third regime. The changes in the residual variance are also abrupt and this implies that the multiple-group changepoint model provides precise information about the timing of the structural breaks in the residual variance. Note also that GDP deflator inflation is highly persistent in the sense that the sum of the autoregressive coefficients (posterior mean) is 0.88. This finding on high inflation persistence is consistent with that in the literature (e.g. Fuhrer and Moore (1995)). However, the 90% credible band does not cover the unit root.[14]

Table 7

US GDP deflator inflation: posterior distributions for the most preferred model [# of breaks (M1,M2,M3)=(0,0,2)].

ParameterPriorPosterior
Regime 1Regime 2Regime 3
μ0.0000.611
(1.000)(0.205)
ϕ10.0000.494
(1.000)(0.064)
ϕ10.0000.387
(1.000)(0.062)
σ20.2270.0780.1740.038
(0.719)(0.014)(0.041)(0.005)
p3,ii0.9900.9850.980
(0.030)(0.013)(0.017)

Standard deviations are reported in parentheses.

Figure 3: GDP deflator inflation: posterior distribution of parameters over time.(A) Unconditional mean, (B) persistence (Sum of AR parameters), (C) residual variance.Posterior mean and 90% band are plotted over time. The estimated break dates (posterior mode) are 1970:Q2 and 1981:Q2 for the residual variance.
Figure 3:

GDP deflator inflation: posterior distribution of parameters over time.

(A) Unconditional mean, (B) persistence (Sum of AR parameters), (C) residual variance.

Posterior mean and 90% band are plotted over time. The estimated break dates (posterior mode) are 1970:Q2 and 1981:Q2 for the residual variance.

4 Robustness

4.1 Comparison with Chib’s (1998) approach

For robustness, I consider Chib’s approach, a single-group changepoint model, in which all the parameters including the residual variance undergo breaks at the same time. The models are estimated using the same priors as in the multiple-group changepoint models. The results for the Bayes factor calculations are summarized for both measures of inflation in Table 8. Based on Chib’s approach, the values of the highest (log) marginal likelihood are equal to –208.54 (three breaks) for CPI inflation and –31.43 (one break) for GDP deflator inflation, respectively. However, these marginal likelihood values are significantly lower than those based on the multiple-group changepoint approach.

Table 8

Comparison to Chib’s (1998) approach: model selection.

Model (# of breaks)Log marginal likelihoodBayes factor
(a) CPI inflation
0–233.430.0000
1–212.130.0002
2–211.670.0003
3–208.540.0068
4–215.940.0000
(b) GDP deflator inflation
0–34.610.0000
1–31.430.0003
2–32.550.0001
3–39.220.0000
4–49.250.0000

Bayes factors are calculated in favor of the alternative model: BF=m(YT|A)m(YT|) for each measure of inflation. m(YT|ℳ*) is the most preferred model based on the multiple-group changepoint approach for each measure of inflation.

I also consider another modified approach in which the unconditional mean and persistence parameters (i.e. conditional mean) undergo co-breaks at the same time, which are independent of the breaks in the residual variance. I estimate the model with one break in the conditional mean and three breaks in the residual variance in accordance with the empirical finding in the previous section. The log marginal likelihood for this modified model is calculated to be –204.81, which is lower than that for the most preferred model (–203.55) based on the multiple-group changepoint approach. The Bayes factor is then equal to 0.28 (alternatively 3.53 in favor of the most preferred model, ℳ*=(0, 1, 3)), which shows substantial evidence for one break in persistence and three breaks in the residual variance when adopting Jeffreys’s (1961) interpretation.[15] Note that the most preferred model for GDP deflator inflation has no break in the unconditional mean and persistence. Therefore it is not required to estimate the modified model additionally.

4.2 Unobserved components models with stochastic volatility

The empirical results reported in Section 3 show that there have been large changes in the variance, but two measures of inflation exhibit the different evolution of the residual variance in terms of the number and timing of the breaks. Following Stock and Watson (2007), I consider an unobserved components model with stochastic volatility (UC-SV) and further examine whether these empirical findings on the shifts in the residual variance are robust.[16]

Stock and Watson (2007) estimate an UC-SV model for GDP deflator inflation from 1953:Q1 to 2004:Q4. They find that there have been substantial movements over time in the standard deviation of the permanent component while there is little change in the standard deviation of the transitory innovation. I examine CPI inflation in addition to GDP deflator inflation using the longer sample period of 1953:Q1–2013:Q4, which is used in Section 3, in comparison to Stock and Watson (2007). The UC-SV model specification is exactly the same as in Stock and Watson (2007):

πt=τt+ηt, where ηt=ση,tξη,tτt=τt1+ϵt, where ϵt=σϵ,tξϵ,tlnση,t2=lnση,t12+vη,tlnσϵ,t2=lnσϵ,t12+vϵ,t

where ξt=(ξt, ξε,t)′ is i.i.d. N(0, I2); vt=(vη,t, vε,t)′ is i.i.d. N(0, γI2); ξt and vt are independently distributed; and γ determines the smoothness of the stochastic volatility process. The scalar parameter γ is set to 0.2 as in Stock and Watson (2007) and the posterior distributions of stochastic volatility are estimated by MCMC. Figures 4 and 5 plot the smoothed estimates (posterior mean and 67% band) of σϵ,t2 and ση,t2 from the UC-SV models for GDP deflator inflation and CPI inflation, respectively. The empirical results for GDP deflator inflation are similar to Stock and Watson’s (2007) results. The standard deviation of the permanent disturbance was moderate from the mid 1950s through the early 1970s, it was large during the 1970s through the mid 1980s, and it declined sharply in the mid-1980s, whereas the volatility of the transitory disturbance appears to have remained stable. This low-high-low volatility pattern on the permanent innovations is consistent with the regime changes in the residual variance based on the multiple-group changepoint model in Section 3. Note also that the changepoint model analysis finds that GDP inflation has been highly persistent for the whole sample period and this high persistence for GDP deflator inflation implies that the evolution of inflation volatility would be mostly attributed to the permanent innovations. This conjecture is confirmed by the substantial changes in the standard deviations of the permanent innovations and the relatively stable volatility of the transitory innovations. In contrast to GDP deflator inflation, the volatility of the transitory innovations for CPI inflation shows substantial movements while the permanent innovations for CPI inflation exhibit a similar pattern of the low-high-low volatility shifts for GDP deflator inflation. The high volatility of the transitory innovations appears to contribute to the large fluctuations since the early 2000s because the volatility of the permanent innovations is moderate during this period. This empirical finding is consistent with the result based on the multi-group changepoint model in the sense that CPI inflation experienced a dramatic drop in persistence around the early 1980s and the permanent innovations would not play an important role in generating high levels of CPI inflation volatility since the early 2000s.

Figure 4: CPI inflation: stochastic volatility in UC-SV model.(A) Permanent innovations, (B) transitory innovations.Posterior mean and 67% band are plotted over time.
Figure 4:

CPI inflation: stochastic volatility in UC-SV model.

(A) Permanent innovations, (B) transitory innovations.

Posterior mean and 67% band are plotted over time.

Figure 5: GDP deflator inflation: stochastic volatility in UC-SV model.(A) Permanent innovations, (B) transitory innovations.Posterior mean and 67% band are plotted over time.
Figure 5:

GDP deflator inflation: stochastic volatility in UC-SV model.

(A) Permanent innovations, (B) transitory innovations.

Posterior mean and 67% band are plotted over time.

5 Summary and comparison with the literature

To summarize, two different measures of inflation undergo distinct structural changes in different parameters as well as at different dates. Both measures of inflation switched from a low volatility regime to a high volatility regime in the early 1970s but switched to another low volatility regime at different dates: the early 1980s for GDP deflator inflation and the early 1990s for CPI inflation. Moreover, the residual variance for CPI inflation has increased again since the early 2000s but GDP deflator inflation has remained less volatile. The empirical results on the changes in volatility for two measures of inflation are robust to the alternative specification of stochastic volatility. CPI inflation experienced a dramatic drop in persistence around the early 1980s but GDP deflator inflation is still persistent. The correlations between CPI inflation and GDP deflator inflation are calculated for the periods before and after 1981:Q3, which is the break date (posterior mode) for persistence of CPI inflation. The correlation has dropped substantially from 0.88 to 0.44 and this decrease also supports the different dynamics of the two inflation measures since the early 1980s. These findings about the complex patterns of structural changes reflect the possibility that the parameter shifts are caused by a variety of sources.

When reviewing recent findings in the literature,[17] there appears to be controversy surrounding changes in inflation persistence. The mixed statistical evidence on inflation persistence in this paper seems to be along the lines of the disagreement in the literature. However, there seems to be an interesting pattern of results in reading recent studies in the literature regardless of persistence measures and econometric models. That is, whether there was a change in persistence around the early 1980s depends on the measure of inflation used in the analysis.

For example, Pivetta and Reis (2007) use GDP deflator inflation and conclude that inflation persistence has been roughly constant and high over the past 40 years, which is the same as the empirical finding in this paper.[18]Pivetta and Reis (2007) conduct extensive research and robustness checks to support their findings. They first consider a Bayesian time-varying parameter model which allows for time-varying intercept and persistence parameters. They then calculate median unbiased estimates using local-to-unity asymptotics for different measures of persistence. Based on the various empirical models and estimates, they conclude that there has been no evidence of a change in persistence since 1965. For CPI inflation, Kim, Nelson and Piger (2004) find a persistence fall in 1979:Q2 and Leybourne et al. (2003) detected a change in inflation dynamics from I(1) to I(0) in 1982:Q2.

While most studies focus on only a particular measure of inflation, some papers examine multiple measures of inflation.[19]Stock (2002) finds no evidence of a structural break for GDP deflator inflation but detects a single structural break in the regression coefficients for CPI inflation around 1981 using the Quandt likelihood ratio test at a 10% level. This break date is consistent with the estimated (posterior mode) break date based on the multiple-group changepoint approach. Benati (2008) and Fuhrer (2010) consider a broad range of inflation measures for various subsamples, which are determined by monetary regimes and the so-called “Great Moderation” break, respectively. Benati (2008) documents that there was a fall in persistence for CPI inflation during the post-Volcker stabilization period since 1982:Q4, while other measures of inflation including GDP deflator inflation continued to be persistent. Finally, Fuhrer (2010) finds that since the early 1980s CPI inflation has very different dynamics from other inflation measures such as the GNP deflator, the GDP deflator, the PCE deflator, the core CPI, and the core PCE deflator. He confirms this difference by considering “grid-bootstrap” median-unbiased estimates of persistence, results for structural break test in persistence, first-order autocorrelation, and LAR estimates.

6 Conclusion

In this paper, I employ a Bayesian approach to making inferences about complicated patterns of structural breaks in inflation dynamics. I modify Chib’s (1998) approach by allowing multiple parameters to undergo mutually independent structural breaks at different dates with the different number of breaks. Structural breaks are modeled as abrupt changes to identify potential regime shifts in economic structure such as a long-run inflation target, monetary policy, and price-setting behavior. I examine postwar quarterly US inflation rates based on the CPI and the GDP deflator. Both inflation measures show multiple structural breaks in the residual variance but they show quite distinctive patterns in terms of timing and the number of breaks, which are confirmed by the empirical results based on the UC-SV model.

Another interesting finding is that CPI inflation experienced a dramatic drop in persistence around the early 1980s, but GDP deflator inflation is still persistent. However, I do not find evidence of a structural shift in the unconditional mean for both measures of inflation. The marginal probability calculations for the number of breaks in each individual parameter group also strongly support the model selection results based on the Bayes factors.

When reviewing the recent literature, considerable controversy exists over the structural break in inflation persistence around the early 1980s but the existence of the structural break appears to be dependent on the measures of inflation, as highlighted by the empirical findings in this paper. The structural breaks at different dates reflect the possibility that the parameter shifts are caused by a variety of factors.


Corresponding author: Yunjong Eo, School of Economics, University of Sydney, Sydney 2006, Australia, Phone: +612 9351 3075, Fax: +612 9351 4341, e-mail:

Acknowledgments

I am very grateful to James Morley for his constructive discussion and comments. I also thank the editor and two anonymous referees, Kyu Ho Kang, Jeremy Piger, Anastasia Zervou, and participants at the Midwest Econometrics Group meeting and the Annual Symposium of the Society for Nonlinear Dynamics and Econometrics for helpful comments and suggestions. I acknowledge the use of GAUSS code written by James Stock and Mark Watson for unobserved components model with stochastic volatility. An earlier version of this paper was circulated under the title “Bayesian Inference about the Types of Structural Breaks When There Are Different Breaks in Many Parameters.”

A. Appendix

A.1 Sampling posteriors

I describe how to sample the latent regime indicators, (S˜1,T,S˜2,T,S˜3,T) and the posterior of model parameters conditional on the regime transition probabilities, P=(P1, P2, P3) in the case of three parameter groups based on MCMC sampling algorithm in Section 2.

A.1.1 Simulation of latent regime indicatorS˜g,Tforg=1, 2, 3

The discrete latent regime indicators {Sg,t} for t=1, …, T and g=1, 2, 3 are simulated in each step. The objective is to sample the indicators from the mass discrete function p(S˜g,T|θ,S˜g,T,P,YT) where p(·) denotes a discrete mass function and S˜g,T=(S˜1,T,,S˜g1,T,S˜g+1,T,,S˜G,T). The mass function can be expressed as a joint density in reverse time order as follows.

(A.1)p(S˜g,T|θ,S˜g,T,P,YT)=p(Sg,T|θ,S˜g,T,P,YT)×p(Sg,T1|Sg,T,θ,S˜g,T,P,YT)××p(Sg,t|Sgt+1,θ,S˜g,T,P,YT)××p(Sg,1|Sg2,θ,S˜g,T,P,YT) (A.1)

where Sgt+1=[Sg,t+1Sg,T]. Notice that the first regime and the last regime are always one and Mg+1, respectively. These imply that for g=1, 2, 3

p(Sg,T=Mg+1|θ,S˜g,T,P,YT)=1   and   p(Sg,1=1|θ,S˜g,T,P,YT)=1.

Thus, the regimes Sg,t for t=2, …, t−1 are recursively simulated from t=T−1 to t=2 in reverse time order.

As discussed in Section 2, the regime transition follows a first order Markov process. It is also independent of its own parameter as well as both other parameters and their latent regime indicators, as shown in Chib (1996). Thus, a term in (A.1) can be written that for g=1, 2, 3

p(Sg,t|YT,Sgt+1,S˜g,T,θ,P)p(Sg,t|Yt,S˜g,T,θ,P)×p(Sg,t+1|Sg,t,Pg).

The first term in the proportion of the regime distribution is calculated recursively. Suppose p(Sg,t1|Yt1,S˜g,T,θ,P) is known. Then, Bayes’ rule can be applied for k=1, …, Mg+1 regimes,

p(Sg,t=k|Yt,S˜g,T,θ,P)=p(Sg,t=k|Yt1,S˜g,T,θ,P)×f(yt|Yt1,θg,k,θg)l=1Mg+1p(Sg,t=l|Yt1,S˜g,T,θ,P)×f(yt|Yt1,θg,l,θg)

where

p(Sg,t=k|Yt1,S˜g,T,θ,P)=l=k1kp(Sg,t=k|Sg,t1=l,Pg)×p(Sg,t1=l|Yt1,S˜g,T,θ,P)

and p(Sg,t=k|Sg,t−1=l, Pg) is the (l, k)th entry of the transition matrix Pg.

In sum, the probabilities of the regimes over dates are sampled through MCMC simulations:

Pr(Sg,t=k|YT)=p(Sg,t=k|YT,θ,P)π(θ,P|YT)d(θ,P)

and in practice with J simulations

Pr(Sg,t=k|YT)=1Jj=1Jp(Sg,t(j)=k|YT,θ(j),P(j)).

A.1.2 Simulation of transition probability matrixPg

The transition probability matrices (P1, P2, P3) are sampled only conditional on their regime indicators (S˜1,T,S˜2,T,S˜3,T), respectively. The reason is that the full conditional distribution Pg|θ,S˜g,T,S˜g,T,Pg,YT is independent of (θ,S˜g,T,Pg,YT) where Pg=(P1, …, Pg−1, Pg+1, …, PG) for g=1, 2, 3. Thus, it can be shown that

π(Pg|θ,S˜g,T,S˜g,T,Pg,YT)=π(Pg|S˜g,T).

If Beta priors for pi,i, i=1, …, Mg, are employed as

pi,iBeta(ui,i,ui,i+1)

where ui,i and ui,i+1 are the hyper-parameters, the posterior distribution can be derived as

pi,i|S˜g,TBeta(ui,i+ni,i,ui,i+1+ni,i+1)

where ni,j refers to the total number of transitions from regime i to regime j. Note that ni,i+1, for i=1, …, Mg, is always equal to one since every regime never comes back to the previous regimes and moves to the next regime only once. For details, see Albert and Chib (1993).

A.1.3 Sampling of the unconditional meanμ

Consider an AR(2) model with structural breaks in the unconditional mean, persistence coefficients, and the residual variance independently as follows:

πtμS1,t=ϕ1,S2,t(πt1μS1,t1)+ϕ2,S2,t2(πt2μS1,t2)+et,   etN(0,σs3,t2).

Conditional on (S˜1,T,S˜2,T,S˜3,T),ϕ˜=(ϕ1,1,ϕ2,1,,ϕ1,M2+1,ϕ2,M2+1), and σ˜2=(σ12,,σM3+12), the unconditional mean for the regime j, μj, for j=1, …, (M1+1) can be sampled as follows.

(a) Prior

μjN(μ_jj,D_μj)

(b) Posterior

μj|μ˜j,ϕ˜,σ˜2,S˜1,T,S˜2,T,S˜3,TN(μ¯j,D¯μj)

where μ˜j=(μ1,,μj1,μj+1,,μM1+1),

μ¯jj=(D_μj1+{S1,t=j,S1,t1=j,S1,t2=j}x1,tx1,t/σS3,t2)1(D_μj1μ_j+{S1,t=j,S1,t1=j,S1,t2=j}x1,ty1,t/σS3,t2),D¯μj=(D_μj1+{S1,t=j,S1,t1=j,S1,t2=j}x1,tx1,t/σS3,t2)1,

y1,t=πtϕ1,S2,tπt1ϕ2,S2,tπt2μS1,t1(S1,tj)+ϕ1,S2,tμS1,t11(S1,t1j)+ϕ2,S2,tμS1,t21(S1,t2j),

and

x1,t=1(S1,t=j)ϕ1,S2,t1(S1,t1=j)ϕ2,S2,t1(S1,t2=j).

A.1.4 Sampling of persistence coefficientsϕ

Conditional on (S˜1,T,S˜2,T,S˜3,T),μ˜, and σ˜2, persistence parameters for regime j, ϕj=(ϕ1,j, ϕ2,j)′, for j=1, …, (M2+1) can be sampled as follows.

(a) Prior

ϕjN(ϕ_jj,D_ϕj)

(b) Posterior

ϕj|μ˜,σ˜2,S˜1,T,S˜2,T,S˜3,TN(ϕ¯j,D¯ϕj)

where

ϕ¯j=(D_ϕj1+{S2,t=j}x2,tx2,t/σS3,t2)1(D_ϕj1ϕ_j+{S2,t=j}x2,ty2,t/σS3,t2),D¯ϕj=(D_ϕj1+{S2,t=j}x2,tx2,t/σS3,t2)1,y2,t=πtμS1,t,

and

x2,t=[(πt1μS1,t1)(πt2μS1,t2)].

A.1.5 Sampling of the residual varianceσ2

Conditional on (S˜1,T,S˜2,T,S˜3,T),μ˜, and ϕ˜, residual variance for regime j,σj2, for j=1, …, (M3+1) can be sampled as follows.

(a) Prior

σj2IG(νj2,δj2)

(b) Posterior

σj2|μ˜,ϕ˜,S˜1,T,S˜2,T,S˜3,TIG(νj+nj2,δj+{S3,t=j}et22)

where nj=t=1T1(S3,t=j).

A.2 Marginal likelihood calculation

Let m(YT|ℳ) is the marginal likelihood or the marginal density of the data YT under model ℳ. The marginal likelihood of model ℳ can be easily calculated through the method of Chib (1995) for Gibbs sampling based on the Bayes rule identity:

(A.2)m(YT|)=f(YT|ψ,)π(ψ|)π(ψ|YT,) (A.2)

where ψ=(θ, P). The above identity holds for any point ψ in the parameter space since the left hand side is free of ψ. Taking the logarithm of the marginal likelihood for computational convenience, the estimate of the marginal density at any particular point ψ* is given by

(A.3)lnm^(YT|)=lnf(YT|θ,P,)+lnπ(θ,P|)lnπ(θ,P|YT,). (A.3)

I explain all the terms in equation (A.3) in the following subsections. For simplicity, I drop the model indicator ℳ from now on.

A.2.1 Likelihood function

The logarithm of likelihood function is given by

ln f(YT|ψ)=t=1Tlnf(yt|Yt1,ψ)

where

f(yt|Yt1,ψ)=S1,t=1M1+1S2,t=1M2+1S3,t=1M3+1f(yt|Yt1,S1,t,S2,t,S3,t,ψ)×p(S1,t,S2,t,S3,t|Yt1,ψ)

is the one-step ahead prediction density and f(yt|Yt−1, S1,t, S2,t, S3,t, ψ*) is the conditional density of yt given the composite of regimes (S1,t, S2,t, S3,t) as well as the posterior mean ψ*. Define a composite of regimes for all the parameters by St=(S1,t, S2,t, S3,t). Then, p(S1,t, S2,t, S3,t|Yt−1, ψ*) is the joint discrete mass function of the composite St=(S1,t, S2,t, S3,t) and the transition probability matrix for the composite of regimes St is given by P1P2P3 where ⊗ indicates the Kronecker product, P is a m-by-m square matrix, and the number of the composite of regimes St is given by m=(M1+1)×(M2+1)×(M3+1). For more details, see Kim and Nelson (1999).

A.2.2 Prior density

All the parameters are a priori assumed to be independent of one another and the logarithm of prior density is given by

lnπ(ψ|M)=lnπ(μ˜)+lnπ(ϕ˜)+lnπ(σ˜2)+lnπ(P1)+lnπ(P2)+lnπ(P3).

A.2.3 Posterior density

In order to estimate the posterior ordinate π(θ*, P*|YT), I consider the conditional decomposition of the posterior density as in Chib (1998). Note that the latent variables (S˜1,T,S˜2,T,S˜3,T) are integrated out in the calculation of the posterior density in each step and throughout this reduced Gibbs run, μ˜,ϕ˜,σ˜2,P1, and P2 are set equal to their posterior mean.

π(θ,P|YT)=π(μ˜|YT)×π(P1|μ˜,YT)×π(ϕ˜|μ˜,P1,YT)×π(P2|μ˜,ϕ˜,P1,YT)×π(σ˜2|μ˜,ϕ˜,P1,P2,YT)π(P3|μ˜,ϕ˜,σ˜2,P1,P2,YT)

where

π(μ˜|YT)=π(μ˜|ϕ˜,σ˜2,P1,P2,P3,S˜1,T,S˜2,T,S˜3,T,YT)×π(ϕ˜,σ˜2,P1,P2,P3,S˜1,T,S˜2,T,S˜3,T|YT)dϕ˜dσ˜2dP1dP2dP3dS˜1,TdS˜2,TdS˜3,T,

π(P1|μ˜,YT)=π(P1|μ˜,ϕ˜,σ˜2,P2,P3,S˜1,T,S˜2,T,S˜3,T,YT)×π(ϕ˜,σ˜2,P2,P3,S˜1,T,S˜2,T,S˜3,T|μ˜,YT)dϕ˜dσ˜2dP2dP3dS˜1,TdS˜2,TdS˜3,T,

π(ϕ˜|μ˜,P1,YT)=π(ϕ˜|μ˜,P1,ϕ˜,σ˜2,P2,P3,S˜1,T,S˜2,T,S˜3,T,YT)×π(σ˜2,P2,P3,S˜1,T,S˜2,T,S˜3,T|μ˜,P1,YT)dσ˜2dP2dP3dS˜1,TdS˜2,TdS˜3,T,

π(P2|μ˜,ϕ˜,P1,YT)=π(P2|μ˜,ϕ˜,P1,σ˜2,P3,S˜1,T,S˜2,T,S˜3,T,YT)×π(σ˜2,P3,S˜1,T,S˜2,T,S˜3,T|μ˜,ϕ˜,P1,YT)dσ˜2dP3dS˜1,TdS˜2,TdS˜3,T,

π(σ˜2|μ˜,ϕ˜,P1,P2,YT)=π(σ˜2|μ˜,ϕ˜,P1,P2,P3,S˜1,T,S˜2,T,S˜3,T,YT)×π(P3,S˜1,T,S˜2,T,S˜3,T|μ˜,ϕ˜,P1,P2,YT)dP3dS˜1,TdS˜2,TdS˜3,T,

and

π(P3|μ˜,ϕ˜,σ˜2,P1,P2,YT)=π(P3|μ˜,ϕ˜,σ˜2,P1,P2,S˜1,T,S˜2,T,S˜3,T,YT)×π(S˜1,T,S˜2,T,S˜3,T|μ˜,ϕ˜,σ˜2,P1,P2,YT)dS˜1,TdS˜2,TdS˜3,T.

The decomposition of the posterior density shows that the first ordinate π(μ˜|YT) can be calculated based on draws from the full Gibbs run, and π(P1|μ˜,YT),π(ϕ˜|μ˜,P1,YT),π(P2|μ˜,ϕ˜,P1,YT),π(σ˜2|μ˜,ϕ˜,P1,P2,YT), and π(P3|μ˜,ϕ˜,σ˜2,P1,P2,YT) can be calculated from appropriate reduced Gibbs runs. The Monte Carlo estimate of each decomposition component based on draws from each Gibbs run is calculated as follows.

π(μ˜|YT)=1Jj=1Jπ(μ˜|ϕ˜(j),σ˜2(j),P1(j),P2(j),P3(j),S˜1,T(j),S˜2,T(j),S˜3,T(j),YT),

π(P1|μ˜,YT)=1Jj1=1Jπ(P1|μ˜,ϕ˜(j1),σ˜2(j1),P2(j1),P3(j1),YT),

π(ϕ˜|μ˜,P1,YT)=1Jj2=1Jπ(ϕ˜|μ˜,P1,ϕ˜(j2),σ˜2(j2),S˜1,T(j2),S˜2,T(j2),S˜3,T(j2),YT),

π(P2|μ˜,ϕ˜,P1,YT)=1Jj3=1Jπ(P2|μ˜,ϕ˜,P1,σ˜2(j3),P3(j3),S˜1,T(j3),S˜2,T(j3),S˜3,T(j3),YT),

π(σ˜2|μ˜,ϕ˜,P1,P2,YT)=1Jj4=1Jπ(σ˜2|μ˜,ϕ˜,P1,P2,P3(j4),S˜1,T(j4),S˜2,T(j4),S˜3,T(j4),YT),

and

π(P3|μ˜,ϕ˜,σ˜2,P1,P2,YT)=1Jj5=1Jπ(P3|μ˜,ϕ˜,σ˜2,P1,P2,S˜1,T(j5),S˜2,T(j5),S˜3,T(j5),YT)

where the superscript (j) refers to the jth draw of the full Gibbs run and the superscript (ji), i=1, …, 5, refers to the jith draw from the appropriate reduced Gibbs run. Thus, in addition to the full Gibbs run for the usual estimation of parameters, it is required to have five additional Gibbs runs (5×J iterations). For example, π(σ˜2|μ˜,ϕ˜,P1,P2,YT) is calculated by additional J iterations from the following reduced j4th Gibbs run.

Algorithm forπ(σ˜2|μ˜,ϕ˜,P1,P2,YT)

  1. Generate σ˜2(j4) from π(σ˜2|μ˜,ϕ˜,P1,P2,P3(j41),S1,T(j41),S2,T(j41),S3,T(j41),YT)

  2. Generate P3(j4) from π(P3|μ˜,ϕ˜,P1,P2,σ˜2(j4),S1,T(j41),S2,T(j41),S3,T(j41),YT)

  3. Generate S˜1,T(j4) from π(S1,T|μ˜,ϕ˜,P1,P2,σ˜2(j4),P3(j4),S2,T(j41),S3,T(j41),YT)

  4. Generate S˜2,T(j4) from π(S2,T|μ˜,ϕ˜,P1,P2,σ˜2(j4),P3(j4),S1,T(j4),S3,T(j41),YT)

  5. Generate S˜3,T(j4) from π(S3,T|μ˜,ϕ˜,P1,P2,σ˜2(j4),P3(j4),S1,T(j4),S2,T(j4),YT)

  6. Evaluate π(σ˜2|μ˜,ϕ˜,P1,P2,P3(j4),S1,T(j4),S2,T(j4),S˜3,T(j4),YT)

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Supplemental Material:

The online version of this article (DOI: 10.1515/snde-2015-0041) offers supplementary material, available to authorized users.


Published Online: 2016-1-22
Published in Print: 2016-6-1

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