|
||||
|
||||
Stable Mixture GARCH ModelsSimon A. BrodaUniversity of Amsterdam - Amsterdam School of Economics (ASE) Markus HaasLudwig-Maximilians-Universität Munich - Department of Statistics Jochen KrauseUniversity of Zurich - Department of Banking and Finance Marc S. PaolellaUniversity of Zurich ; Swiss Finance Institute Sven C. SteudeUniversity of Zurich - Department of Banking and Finance October 18, 2011 Swiss Finance Institute Research Paper No. 11-39 Abstract: A new model class for univariate asset returns is proposed which involves the use of mixtures of stable Paretian distributions, and readily lends itself to use in a multivariate context for portfolio selection. The model nests numerous ones currently in use, and is shown to outperform all its special cases. In particular, an extensive out-of-sample risk forecasting exercise for seven major FX and equity indices confirms the superiority of the general model compared to its special cases and other competitors. An improved method (in terms of speed and accuracy) is developed for the computation of the stable Paretian density. Estimation issues related to problems associated with mixture models are discussed, and a new, general, method is proposed to successfully circumvent these. The model is straightforwardly extended to the multivariate setting by using an independent component analysis framework. The tractability of the relevant characteristic function then facilitates portfolio optimization using expected shortfall as the downside risk measure.
Number of Pages in PDF File: 38 Keywords: Density Forecasting, Expected Shortfall, Fat Tails, ICA, GARCH, Mixtures, Portfolio Selection, Stable Paretian Distribution, Value-at-Risk JEL Classification: C13, C16, C22, C32, G17 working papers seriesDate posted: September 23, 2011 ; Last revised: October 18, 2011Suggested CitationContact Information
|
|
||||||||||||||||||||||
© 2013 Social Science Electronic Publishing, Inc. All Rights Reserved.
FAQ
Terms of Use
Privacy Policy
Copyright
This page was processed by apollo6 in 0.718 seconds