Homogeneous Cosmological Models without Shear

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概要

• 論文の詳細を見る

• The paper presents some general differential relations on the dynamics of homogeneous rotating cosmological models with nonvanishing pressure. It appears from these that such models must in general be associated with shear if there be a linear relation between the pressure and the density except perhaps in the case p=ρ/9.

• 理論物理学刊行会の論文
• 1968-02-25

著者

• Banerji S.

  Department Of Physics The University Of Burdwan

関連論文

• Homogeneous Cosmological Models without Shear

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