Abstract
view Abstract Citations (15) References (8) Co-Reads Similar Papers Volume Content Graphics Metrics Export Citation NASA/ADS Hagedorn Equation of State in Neutron Stars Rhoades, Clifford E., Jr. ; Ruffini, Remo Abstract At a density of 5 X 1 g neutron-star matter can be described (Harrison and Wheeler) by a system of three noninteracting degenerate gases-namely, electrons, protons, and neutrons. At a density of 10' g , strong interactions between particles can give a significant contribution (Cameron, Cohen, Langer, and Rosen). At densities of > 10' g , production of new particles has to be taken into account. Hagedom has recently giv%n an analytic equation of state for this regime. We have explored the effect of this new equation of state for supranuclear densities on the equilibrium conflgnrations of neutron stars. Publication: The Astrophysical Journal Pub Date: January 1971 DOI: 10.1086/180672 Bibcode: 1971ApJ...163L..83R full text sources ADS |
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