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Multiscaling and nonextensivity of large-scale structures in the Universe

机译:宇宙中大型结构的多尺度和非扩展性

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摘要

There has been a trend in the past decade to describe the large-scale structures in the Universe as a (multi)fractal set. However, one of the main objections raised by the opponents of this approach deals with the transition to homogeneity. Moreover, they claim there is not enough sampling space to determine a scaling index which characterizes a (multi)fractal set. In this work we propose an alternative solution to this problem, using the generalized thermostatistics formalism. We show that applying the idea of nonextensivity, intrinsic to this approach, it is possible to derive an expression for the correlation function, describing the scaling properties of large-scale structures in the Universe and the transition to homogeneity, which is in good agreement with observational data. (C) 2002 Elsevier Science B.V. All rights reserved. [References: 24]
机译:在过去的十年中,有一种趋势将宇宙中的大型结构描述为(多重)分形集。但是,这种方法的反对者提出的主要反对意见之一涉及向同质性的过渡。此外,他们声称没有足够的采样空间来确定表征(多)分形集的缩放指数。在这项工作中,我们使用广义温度统计形式主义提出了解决该问题的另一种方法。我们证明,应用这种方法固有的非扩展性思想,可以导出相关函数的表达式,描述宇宙中大型结构的缩放性质以及向均质的过渡,这与观测数据。 (C)2002 Elsevier Science B.V.保留所有权利。 [参考:24]

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