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Microscopic origin of non-Gaussian distributions of financial returns

dc.contributor.authorBiro, T. S.
dc.contributor.authorRosenfeld, Rogério [UNESP]
dc.contributor.institutionRMKI
dc.contributor.institutionUniversidade Estadual Paulista (Unesp)
dc.date.accessioned2013-09-30T18:53:39Z
dc.date.accessioned2014-05-20T14:09:30Z
dc.date.available2013-09-30T18:53:39Z
dc.date.available2014-05-20T14:09:30Z
dc.date.issued2008-03-01
dc.description.abstractIn this paper we study the possible microscopic origin of heavy-tailed probability density distributions for the price variation of financial instruments. We extend the standard log-normal process to include another random component in the so-called stochastic volatility models. We study these models under an assumption, akin to the Born-Oppenheimer approximation, in which the volatility has already relaxed to its equilibrium distribution and acts as a background to the evolution of the price process. In this approximation, we show that all models of stochastic volatility should exhibit a scaling relation in the time lag of zero-drift modified log-returns. We verify that the Dow-Jones Industrial Average index indeed follows this scaling. We then focus on two popular stochastic volatility models, the Heston and Hull-White models. In particular, we show that in the Hull-White model the resulting probability distribution of log-returns in this approximation corresponds to the Tsallis (t-Student) distribution. The Tsallis parameters are given in terms of the microscopic stochastic volatility model. Finally, we show that the log-returns for 30 years Dow Jones index data is well fitted by a Tsallis distribution, obtaining the relevant parameters. (c) 2007 Elsevier B.V. All rights reserved.en
dc.description.affiliationRMKI, KFKI, Budapest, Hungary
dc.description.affiliationState Univ São Paulo, Inst Fis Teor, São Paulo, Brazil
dc.description.affiliationUnespState Univ São Paulo, Inst Fis Teor, São Paulo, Brazil
dc.format.extent1603-1612
dc.identifierhttp://dx.doi.org/10.1016/j.physa.2007.10.067
dc.identifier.citationPhysica A-statistical Mechanics and Its Applications. Amsterdam: Elsevier B.V., v. 387, n. 7, p. 1603-1612, 2008.
dc.identifier.doi10.1016/j.physa.2007.10.067
dc.identifier.issn0378-4371
dc.identifier.urihttp://hdl.handle.net/11449/24178
dc.identifier.wosWOS:000253188700018
dc.language.isoeng
dc.publisherElsevier B.V.
dc.relation.ispartofPhysica A: Statistical Mechanics and Its Applications
dc.relation.ispartofjcr2.132
dc.relation.ispartofsjr0,773
dc.rights.accessRightsAcesso restrito
dc.sourceWeb of Science
dc.subjectstochastic volatilityen
dc.subjectBorn-Oppenheimer approximationen
dc.subjectpower-law distribution of returnsen
dc.titleMicroscopic origin of non-Gaussian distributions of financial returnsen
dc.typeArtigo
dcterms.licensehttp://www.elsevier.com/about/open-access/open-access-policies/article-posting-policy
dcterms.rightsHolderElsevier B.V.
dspace.entity.typePublication
unesp.campusUniversidade Estadual Paulista (UNESP), Instituto de Física Teórica (IFT), São Paulopt

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