Neutrino Cooling of Neutron Stars in Pion-Condensed Phase

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概要

• 論文の詳細を見る

• Neutrino energy loss rates of neutron stars in the pion-condensed phase are calculated. The studied processes are the decay of thermally excited pions and the nucleon URCA process. The nucleon URCA process makes a major contribution to the cooling rate. The expected neutrino luminosity is about 7.6×10^<44> ergs/sec(T/10^9K)^6 for 1M_⨀ neutron stars. This luminosity is 10^7 times as high as the standard value.

• 理論物理学刊行会の論文
• 1977-12-25

著者

• KIGUCHI Masayoshi

  Research Institute for Science and Technology, Kinki University

• Kiguchi Masayoshi

  Research Institute For Fundamental Physics Kyoto University

• KIGUCHI Masayoshi

  Research Institute for Science and Technology Kinki University

• KIGUCHI Masayoshi

  Research Institute for Fundamental Physics, Kyoto University

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• Chapter 5 Collapse and Fragmentation of Isothermal Clouds : Part II Formation Processes of Protostars : Origin of the Solar System
• Chapter 4 The Equilibrium and the Stability of Rotating Isothermal Clouds : Part II Formation Processes of Protostars : Origin of the Solar System
• Hot Dense Matter and Stellar Collapse
• The Quantum Chromodynamic Black Body Radiation and the Universe
• Neutrino Cooling of Neutron Stars in Pion-Condensed Phase

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