Microscopic origin of non-Gaussian distributions of financial returns

被引:19
作者
Biro, T. S. [1 ]
Rosenfeld, R. [2 ]
机构
[1] RMKI, KFKI, Budapest, Hungary
[2] State Univ Sao Paulo, Inst Fis Teor, Sao Paulo, Brazil
基金
匈牙利科学研究基金会;
关键词
stochastic volatility; Born-Oppenheimer approximation; power-law distribution of returns;
D O I
10.1016/j.physa.2007.10.067
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
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. (c) 2007 Elsevier B.V. All rights reserved.
引用
收藏
页码:1603 / 1612
页数:10
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