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arXiv · hep-ph/9805395

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

Jiro Arafune·Yukihiro Mimura
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Abstract

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.

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Jiro Arafune, Yukihiro Mimura. 1998-10-14. Finiteness of Multi-body Neutrino Exchange Potential Energy in Neutron Stars. https://doi.org/10.1143/ptp.100.1083

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