Scholarlink

This chapter discusses a particular early cosmological model in which the source of Einsteinian gravitation is assumed to be a “cold collisionless gas” composed of galactic matter (i.e. a thermodynamically inert, spatially homogeneous medium) with a timelike flow given by the timelike geodesics of the Einstein-de Sitter spacetime metric tensor.

错误：搜索内容不能为空，请输入英文关键词
错误：关键词超出字数限制，请精简
高级检索

The Non-Thermodynamic Self-Gravitating Perfect Fluid in a Dynamic Einstein-de Sitter Metric

  • 章节

  • 发表日期：

    2025年

查看全文
  • Robin W. Tucker,
  • Timothy J. Walton

摘要

This chapter discusses a particular early cosmological model in which the source of Einsteinian gravitation is assumed to be a “cold collisionless gas” composed of galactic matter (i.e. a thermodynamically inert, spatially homogeneous medium) with a timelike flow given by the timelike geodesics of the Einstein-de Sitter spacetime metric tensor.