Pion condensed matter at high densities - Equation of state and stellar models

Details Pion condensed matter at high densities - Equation of state and stellar models Pion condensed matter at high densities - Equation of state and stellar models

Jul 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975apj...199..471h&link_type=abstract

Astrophysical Journal, vol. 199, July 15, 1975, pt. 1, p. 471-481. NSF-supported research.

Physics

Condensed Matter

49

Astronomical Models, Equations Of State, Neutron Stars, Pions, Stellar Structure, Condensed Matter Physics, Cosmic Dust, Density (Mass/Volume), Ground State, Nuclear Reactions, Nucleon-Nucleon Interactions, Stellar Rotation

Scientific paper

Equations of state for the ground state of matter at nuclear densities
and above are derived, including the effects of a condensed charged pion
wave. Nonrotating neutron star models are constructed using these
equations of state, and their observational significance is discussed.

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