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P-star model for India: a nonlinear approach

  • Aditi Chaubal ORCID logo EMAIL logo
Published/Copyright: August 18, 2018

Abstract

Inflation in India has been a major cause for concern in the recent past (2008–2012). This study examines the Indian wholesale price index inflation from 1951 to 2012 using P-star (or P*) models after accounting for the nonlinearities in the data by establishing the presence of a nonlinear long-run equilibrium. The paper establishes the presence of a threshold vector error correction model (TVECM) between prices and their long-run equilibrium with three optimal regimes to explain the short-run and long-run dynamics based on an error correcting transition term. Based on these results, the study classifies the various regimes that Indian inflation goes through based on historical economic events. The P* models (price gap, output gap and velocity gap models) were implemented regime-wise. The price gap models (output gap and income velocity gap determine inflation) were found to be optimal in the first and second regimes and consistent with theory. The velocity gap model (which has monetarist foundations) was found to be optimal in the third regime.

JEL Classification: E31; C24; C32; C34

Article Note

This paper was presented at the Financial and Nonlinear Dynamics 2017 conference held in Paris (June 1–2, 2017). The views expressed here do not reflect the views of the Australian Consulate General, Mumbai (my affiliation when this paper was presented and accepted). This paper was part of my PhD thesis submitted and defended at the Indira Gandhi Institute of Development Research, Mumbai.


Acknowledgement

The author is extremely grateful for the valuable comments received from the anonymous referee which led to considerable improvement in the paper. Responsibility for any remaining shortcomings and errors rests solely with the author.

A Appendix

A.1 Data transformations

A.1.1 GDP interpolation method

The quarterly estimates of GDP are available in Khetan, Handa, and Waghmare (1976) and Das (1993) for the periods 1951–1966 and 1970–1990, respectively. Thus, there are gaps in the GDP data from 1967 to 1969 and from 1991 to 1995 (post–1995, quarterly data is available from 1996 onwards).

Suppose the quarterly GDP data points are given as Y(i, t) [e.g. Y(1, 1954), Y(2, 1954), Y(3, 1960), etc.] where i denotes the quarter and t denotes the year.

Then, let P(i, t) denote the proportions of GDP for each quarter (i = 1, …,4) in year t.

(23)P(i,t)=Y(i,t)t=14Y(i,t),t

Collate all the different proportions quarter-wise (set 1, set 2, …, set 4). For each set of quarters (set 1–3), run the following regression:

(24)P(i,t)=αi+βit,t=1,2,3

for the period 1951–1966. The estimates for quarters P(1, t), P(2, t) and P(3, t) for the missing years (1967–1969) are calculated by simple extrapolation of the above equation [equation 24].

The estimates of the fourth quarter proportions (P(4, t)) for the period 1967–1969 are then calculated as given below:

(25)P(4,t)=1P(1,t)P(2,t)P(3,t)

These estimated proportions are then multiplied with the annual GDP (at constant 2004–2005 prices) to get the GDP at constant 2004–2005 prices.

This process is repeated for the 1970–1990 data to obtain the estimates of GDP (at constant 2004–2005 prices) for 1991–1995.

Splicing of GDP

a) The GDP data that has been taken from various data sources needs to be spliced to the same base year prior to using it for further analysis: For e.g.:

YearGDP at new base (2004–2005)QuarterGDP at old base (e.g. 1970–1971)SumProportionSplicing factor (SF)New base (2004–2005) GDP
1970

X1

1975Q1

1975Q2

1975Q3

1975Q4
Y1

Y2

Y3

Y4
S1 = ΣYiZ1 = Y1/S1

Z2 = Y2/S1

Z3 = Y3/S1

Z4 = Y4/S1
SF = X1/S1Z1*SF

(where S is the annual GDP figure at 2004–2005 prices)

Steps: e.g. to splice 1980–1981 to 2004–2005 (no overlapping data exists)

  1. Take sum of each year in quarterly data.

  2. Find splicing factor by using data from (i) and the annual data (at base 2004–2005).

  3. Splice data.

A.2 WPI

1) Monthly data for WPI is available from the DBIE Handbook of Statistics on the Indian economy (with overlapping data given for the different base years).

a) Overlapping data is not available for the WPI at 1980–1981 and 1993–1994 base years.

  1. But, the Economic Affairs Ministry has released the linking factor to convert 1993–1994 base to 1980–1981 base. Thus, the inverse of the linking factor gives (equals) the splicing factor to convert 1993–1994 base to 1980–1981 base.

  2. Thus, the 1980–1981 base data can be converted to 1993–1994 base data using the splicing factor derived in i).

  3. Since overlapping data exists for 1993–1994 and 2003–2004, the splicing factor can be found for converting the former to the latter base.

This in turn can now be used to splice the “new spliced” data (from 1980–1981 to 1993–1994) from ii) to 2003–2004 base.

A.3 Income velocity of money, V

1) Estimation of quarterly income velocity:

The quarterly income velocity of money is calculated as per the RBI definition:

Income velocity of broad money = [GDP (at current market prices)/M3] where M3 is the average broad money supply.

  1. The GDP at current market prices that is used is calculated in the same manner as given above (Appendix A.1.1) for the GDP at constant prices. These figures are also given at a base year of 2004–2005 and hence have been spliced to the same year.

  2. These quarterly estimates are used along with the aggregated M3 figures (which are the simple averages of the monthly broad money M3, for each quarter).

2) Aggregation from monthly to quarterly:

Once all the data is spliced to the same base (2003–2004), it needs to be aggregated to quarterly data. Compute the simple arithmetic mean across quarters for each year.[29] The quarterly WPI dataset is thus, the requisite price data for the P* model.

B Technical appendix: Why BK filter vs. HP filter?

The Baxter-King (BK) filter is chosen to calculate the potential output and potential velocity of money. The advantage of using this filter over the Hodrick-Prescott (HP) filter is that it minimizes the possibility of identifying a spurious cyclical structure in the series. The BK filter filters low frequency and high frequency cycles which enables retaining periodic fluctuations (cycles) between the low and high frequencies (Woitek, 1998; Baum, 2006).

The BK filter can be implemented on raw data, xt, to isolate the component of xt with period of oscillation between pl and pu (where 2 ≤ plpu ≤ ∞) as follows (Christiano & Fitzgerald, 1999):

y^t=B0xt+B1xt+1++BTtixT1+B~TtxT+B1xt1++Bt2x2+B~t1x1,

where t = 3, 4, …, T−2 where y^ approximates yt (where yt is the data generated by applying the ideal band pass filter to xt); Bj=sin(jb)sin(ja)πj,j1,B0=baπ,b=2πpu,a=2πpl and B~Tt,B~t1 are simple linear functions of Bj s.

The HP filter computes the smoothed series st of the raw data xt by minimizing the variance of xt around st subject to a constraint on the second difference of st. The HP filter minimizes:

t=1T(xtst)2+λt=2T1((st+1st)(stst1))2

where λ is the smoothing parameter.

C Model Evaluation

Optimal SARIMA Models across regimes (Model E)

RegimesRegime 1Regime 2Regime 3
CoefficientsConstant0.0733**Constant0.0835**Constant0.0428**
AR(1)0.5201**MA(1)−0.1604MA(1)0.5994**
MA(4)−0.2142**SMA(4)−0.1918SMA(4)−0.2080
Modelsy(t) = 0.07 + 0.5y(t–1) + e(t) – 0.2e(t–4)y(t) = 0.08 + (1 – 0.16L)(1 – 0.19L4)e(t)y(t) = 0.04 + (1 + 0.599L)(1 – 0.21L4)e(t)

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Supplementary Material

The online version of this article offers supplementary material (DOI: https://doi.org/10.1515/snde-2017-0067).


Published Online: 2018-08-18

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