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Pions in Neutron Star Matter
Published online by Cambridge University Press: 14 August 2015
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.
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