Published February 1983 | Version v1
Journal article Metadata-only

Temperature effect on the dynamics of neutron stars with pion condensation

Creators

  • 1. AN SSSR, Novosibirsk. Inst. Teoreticheskoj i Prikladnoj Mekhaniki

Description

The accounting of finite temperature of neutron star with pion condensation results in increasing of a star radius, and decreasing of core mass, core radius, central density and density discontinuity

Additional details

Additional titles

Original title (Russian)
Влияние температуры на динамику нейтронных звезд с пионной конденсацией

Publishing Information

Journal Title
Pis'ma Astron. Zh.
Journal Volume
9
Journal Issue
2
Series
Pis'ma Astron. Zh.
Journal Page Range
116-119
ISSN
0320-0108

INIS

Country of Publication
Russian Federation
Country of Input or Organization
USSR
INIS RN
14785270
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Descriptors DEI
EQUATIONS OF STATE; HYDRODYNAMICS; MASS; NEUTRON STARS; NUCLEAR MATTER; PION CONDENSATION; TEMPERATURE DEPENDENCE; TEMPERATURE DISTRIBUTION; ULTRAHIGH TEMPERATURE
Descriptors DEC
EQUATIONS; FLUID MECHANICS; MATTER; MECHANICS; STARS

Optional Information

Notes
For English translation see the journal Soviet Astronomy Letters (USA).