Finiteness of Multi-Body Neutrino Exchange Potential Energy in Neutron Stars

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概要

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• The multi-body neutrino potential energy is analytically estimated for a spherical neutron star with a vector potential model for neutrinos. We show that the self-energy and the neutrino number of the neutron star coincide with the semi-classical values in the large volume limit, and confirm that there is no catastrophe in neutron stars with massless neutrinos.

• 理論物理学刊行会の論文
• 1998-11-25

著者

• Arafune J

  Univ. Tokyo Tanashi Jpn

• Arafune Jiro

  Department Of Physics Faculty Of Science Tokyo Institute Of Technology:institute For Cosmic Ray Rese

• Arafune Jiro

  Institute For Cosmic Ray Research University Of Tokyo

• MIMURA Yukihiro

  Institute of Cosmic Ray Research,University of Tokyo

• Nimura Yukihiro

  Institute of Cosmic Ray Research,University of Tokyo

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