Primordial Black Holes and Super-Massive Star

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概要

• 論文の詳細を見る

• We study the evolution of a Super-Massive Star (SMS) in a dense stellar and primordial black holes system. The dissipation of kinetic energy of the holes via gravitational interaction in the SMS becomes greater than the critical luminosity. This quasi pile stage continues for about 1×10^4 years.

• 理論物理学刊行会の論文
• 1981-10-25

著者

• HAGIO Fumihiko

  Department of General Education Kumamoto Institute of Technology

関連論文

• Growth of Black Holes in Dense Stellar Systems with Evaporation of Stars
• Primordial Black Holes and Super-Massive Star

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