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The Effects of Nuclear Forces on the Maximum Mass Limit of Neutron Stars

Published online by Cambridge University Press:  07 February 2017

Sachiko Tsuruta
Sachiko Tsuruta*
Affiliation:
Goddard Space Flight Center, Greenbelt, Md., U.S.A.

Abstract

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The original models of neutron stars must be improved by including effects of nuclear interaction. This paper compares the models reached by various groups, and presents an improved model by the Kyoto group. The maximum mass varies between 0.2 M⊙ and 3 M⊙ in the various models. The Vγ model is recommended for use in the absence of further information on the equation of state at high densities.

Type
Session 6
Information
Symposium - International Astronomical Union , Volume 46: The Crab Nebula , 1971 , pp. 352 - 355
Copyright
Copyright © Reidel 1971 

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