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Pions in Neutron Star Matter

Published online by Cambridge University Press:  14 August 2015

Raymond F. Sawyer
Raymond F. Sawyer*
Affiliation:
Dept. of Physics, University of California, Santa Barbara, Calif. 93106, U.S.A.

Abstract

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Arguments are given for pions becoming an important constituent of neutron star matter at densities greater than a critical density lying between 5 × 1014 and 1015 g cm−3. It is anticipated that this will lead to a substantial softening of the equation of state.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 53: Physics of Dense Matter , 1974 , pp. 105 - 110
Copyright
Copyright © Reidel 1974 

References

Auerbach, E. H., Fleming, D. M., and Sternheim, M. M.: 1967, Phys. Rev. 162, 1683.CrossRefGoogle Scholar
Bethe, H. A.: 1971, Ann. Rev. Nuclear Sci. 21, 93.CrossRefGoogle Scholar
Weinberg, S.: 1966, Phys. Rev. Letters 17, 168.Google Scholar