Neutron star evolutionary sequences

We present detailed numerical calculations of the evolution of neutron stars that are cooling through the range of central temperatures from about 10/sup 10/ to 10/sup 7/ K. The calculations are solutions of the full set of central relativistic equations that describe the evolution of a spherical st...

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Veröffentlicht in:	Astrophys. J.; (United States) 1982-04, Vol.255, p.624
Hauptverfasser:	Richardson, M. B., van Horn, H. M., Ratcliff, K. F., Malone, R. C.
Format:	Artikel
Sprache:	eng
Schlagworte:	640102 - Astrophysics & Cosmology- Stars & Quasi-Stellar, Radio & X-Ray Sources BOSONS CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS COOLING CRYSTALLIZATION ELEMENTARY PARTICLES EMISSIVITY EQUATIONS EQUATIONS OF STATE FERMIONS FIELD THEORIES GENERAL RELATIVITY THEORY HADRONS LEPTONS MASSLESS PARTICLES MATHEMATICAL MODELS MESONS NEUTRINOS NEUTRON STARS NUCLEAR REACTIONS NUMERICAL SOLUTION OPACITY OPTICAL PROPERTIES PHASE TRANSFORMATIONS PHYSICAL PROPERTIES PION CONDENSATION PIONS PSEUDOSCALAR MESONS STAR EVOLUTION STAR MODELS STARS SUPERFLUIDITY SURFACE PROPERTIES TRANSPORT THEORY
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