๐”– Bobbio Scriptorium
โœฆ   LIBER   โœฆ

On the non-existence of a Bartlett correction for unit root tests

โœ Scribed by J.L. Jensen; Andrew T.A. Wood


Publisher
Elsevier Science
Year
1997
Tongue
English
Weight
358 KB
Volume
35
Category
Article
ISSN
0167-7152

No coin nor oath required. For personal study only.

โœฆ Synopsis


There has been considerable recent interest in testing for a unit root in autoregressive models, especially in the context of cointegration models in econometrics. The likelihood ratio test for a unit root has non-standard asymptotic behaviour. In particular, when the errors are Gaussian, the limiting null distribution of the likelihood ratio statistic, W, is a certain functional of Brownian motion, rather than chi-squared. Moreover, numerical work has shown that the limiting distribution of W is not always a good approximation to the actual distribution. Consequently, there is a need for improved distributional approximations, and the question of whether W admits a Bartlett correction is of interest. In this note we establish that a Bartlett correction does not exist in the simplest unit root model. (~) 1997 Elsevier Science B.V.


๐Ÿ“œ SIMILAR VOLUMES


Testing for a unit root in the volatilit
โœ Jonathan H. Wright ๐Ÿ“‚ Article ๐Ÿ“… 1999 ๐Ÿ› John Wiley and Sons ๐ŸŒ English โš– 168 KB ๐Ÿ‘ 2 views

It is now well established that the volatility of asset returns is time varying and highly persistent. One leading model that is used to represent these features of the data is the stochastic volatility model. The researcher may test for non-stationarity of the volatility process by testing for a un

Instability conditions for a non-linear
โœ A. Kh. Gelig; A.N. Churilov ๐Ÿ“‚ Article ๐Ÿ“… 2009 ๐Ÿ› Elsevier Science ๐ŸŒ English โš– 135 KB

A class of non-linear discrete second-order systems is considered in the critical case when two roots of the characteristic polynomial of the linearized system are equal to unity. Sufficient conditions for the instability of the equilibrium are obtained.