dc.contributorRMKI
dc.contributorUniversidade 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.created2013-09-30T18:53:39Z
dc.date.created2014-05-20T14:09:30Z
dc.date.issued2008-03-01
dc.identifierPhysica A-statistical Mechanics and Its Applications. Amsterdam: Elsevier B.V., v. 387, n. 7, p. 1603-1612, 2008.
dc.identifier0378-4371
dc.identifierhttp://hdl.handle.net/11449/24178
dc.identifier10.1016/j.physa.2007.10.067
dc.identifierWOS:000253188700018
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.
dc.languageeng
dc.publisherElsevier B.V.
dc.relationPhysica A: Statistical Mechanics and Its Applications
dc.relation2.132
dc.relation0,773
dc.rightsAcesso restrito
dc.sourceWeb of Science
dc.subjectstochastic volatility
dc.subjectBorn-Oppenheimer approximation
dc.subjectpower-law distribution of returns
dc.titleMicroscopic origin of non-Gaussian distributions of financial returns
dc.typeArtículos de revistas


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