Microscopic Origin of Non-Gaussian Distributions of Financial Returns

Details Microscopic Origin of Non-Gaussian Distributions of Financial Returns Microscopic Origin of Non-Gaussian Distributions of Financial Returns

2007-05-29

arxiv.org/abs/0705.4112v2

Economy

Quantitative Finance

Statistical Finance

13 pages, 4 figures. Several clarifying comments, new references and acknowledgments added

Scientific paper

10.1016/j.physa.2007.10.067

In 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.

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