Gravitational Collapse of Cold Dark Matter in Early Universe using Schrodinger Equation

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概要

• 論文の詳細を見る

• 本文データはCiNiiから複製したものである。We have numerically solved a non-linear Schrodinger equation which describes the growth of the density perturbation in an expanding universe. We have explored the characteristics of this Schrodiger equation method because this method has numerous advantage over N-body simulation method for the study of gravitational collapse of Cold dark matter.

• 近畿大学の論文
• 2006-02-28

著者

• Kiguchi Masayoshi

  RIST, Kinki University

• Kiguchi Masayoshi

  Kinki Univ. Osaka Jpn

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