Time evolution of stochastic processes with correlations in the variance: stability in power-law tails of distributions

被引:23
作者
Podobnik, B [1 ]
Matia, K
Chessa, A
Ivanov, PC
Lee, Y
Stanley, HE
机构
[1] Univ Zagreb, Fac Sci, Dept Phys, Zagreb 41000, Croatia
[2] Boston Univ, Ctr Polymer Studies, Boston, MA 02215 USA
[3] Boston Univ, Dept Phys, Boston, MA 02215 USA
[4] Univ Cagliari, Dipartimento Fis, I-09124 Cagliari, Italy
[5] Univ Cagliari, Unita INFM, I-09124 Cagliari, Italy
[6] Yanbian Univ Sci & Technol, Yanji 133000, Jilin, Peoples R China
来源
PHYSICA A | 2001年 / 300卷 / 1-2期
关键词
random walks; stochastic processes; fluctuation phenomena; central limit theory;
D O I
10.1016/S0378-4371(01)00390-9
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
We model the time series of the S&P500 index by a combined process, the AR+GARCH process, where AR denotes the autoregressive process which we use to account for the short-range correlations in the index changes and GARCH denotes the generalized autoregressive conditional heteroskedastic process which takes into account the long-range correlations in the variance. We study the AR+GARCH process with an initial distribution of truncated Levy form. We find that this process generates a new probability distribution with a crossover from a Levy stable power law to a power law with an exponent outside the Levy range, beyond the truncation cutoff, We analyze the sum of n variables of the AR+GARCH process, and find that due to the correlations the AR+GARCH process generates a probability distribution which exhibits stable behavior in the tails for a broad range of values n-a feature which is observed in the probability distribution of the S&P500 index. We find that this power-law stability depends on the characteristic scale in the correlations. We also find that inclusion of short-range correlations through the AR process is needed to obtain convergence to a limiting Gaussian distribution for large it as observed in the data. (C) 2001 Elsevier Science B.V. All rights reserved.
引用
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页码:300 / 309
页数:10
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