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arXiv 0705.4112q-fin.STcond-mat.otherphysics.soc-ph
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金融收益率非高斯分布的微观成因

Microscopic Origin of Non-Gaussian Distributions of Financial Returns

T. S. Biro, R. Rosenfeld

摘要:

本文研究了金融工具价格变动的重尾概率密度分布的可能微观起源。我们扩展了标准的对数正态过程,在所谓的随机波动率模型中包括另一个随机成分。我们研究这些模型的假设下,类似于波恩-奥本海默近似,其中的波动性已经放松到其均衡分布,并作为一个背景的价格过程的演变。在这种近似下,我们证明了所有的随机波动率模型在零漂移修正的对数收益的时滞中应该表现出一个标度关系。我们验证了道琼斯工业平均指数确实遵循这种缩放。然后,我们专注于两个流行的随机波动率模型,赫斯顿和赫尔怀特模型。特别是,我们表明,在赫尔-怀特模型中,由此产生的概率分布的对数回报率在这种近似对应于Tsallis(t-学生)分布。根据微观随机波动率模型给出了Tsallis参数。最后,我们证明了30年道琼斯指数的对数收益率很好地拟合了Tsallis分布,获得了相关参数。

英文摘要:

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.

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