An Equation of State of Cold Dense Matter

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概要

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• In order to discuss the cold dense star such as neutron stars, an equation of state at high density is necessary. When phenomenological baryon-baryon forces are adopted to derive it, an equation of state is very hard to be consistent with causality, that is, a velocity of sound which is derived from the equation of state exceeds the velocity of light. In this paper we present a simple example of the equation of state at zero temperature.

• 理論物理学刊行会の論文
• 1975-03-25

著者

• Akitoshi NlSHlMURA

  Department of Physics, University of Tokyo

関連論文

• An Equation of State of Cold Dense Matter

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