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首页> 外文期刊>The Astrophysical journal >EVOLUTION OF THE CORRELATION FUNCTION FOR A CLASS OF PROCESSES INVOLVING NONLOCAL SELF-REPLICATION
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EVOLUTION OF THE CORRELATION FUNCTION FOR A CLASS OF PROCESSES INVOLVING NONLOCAL SELF-REPLICATION

机译:一类涉及非局部自我复制的过程的相关函数的演化

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摘要

A large class of evolutionary processes can be modeled by a rule that involves self-replication of some physical quantity with a nonlocal rescaling. We show that a class of such models is exactly solvable in the discrete as well as the continuum limit and can represent several physical situations, as varied as from the formation of galaxies in some cosmological models to growth of bacterial cultures. This class of models, in general, has no steady state solution and evolves unstably as t → ∞ for generic initial conditions. The models can, however, exhibit an (unstable) power-law correlation function in the continuum limit, for an intermediate range of times and length scales.
机译:一大类进化过程可以通过一个规则来建模,该规则涉及某些物理量的自我复制和非局部重新定标。我们表明,这类模型在离散极限和连续极限中都是完全可解决的,并且可以表示几种物理情况,从某些宇宙学模型中的星系形成到细菌培养的生长不等。通常,此类模型没有稳态解,并且对于一般初始条件,其演化为t→∞。但是,对于时间和长度范围的中间范围,模型可以在连续极限中显示(不稳定的)幂律相关函数。

著录项

  • 来源
    《The Astrophysical journal》 |2002年第1期|p.10-15|共6页
  • 作者

    T. PADMANABHAN;

  • 作者单位

    Inter-University Centre for Astronomy and Astrophysics, Post Bag 4, Ganeshkhind, Pune 411 007, India;

  • 收录信息
  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类 天文学;
  • 关键词

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