HAGEDORN EQUATION OF STATE IN NEUTRON STARS

被引：14

作者：

RHOADES, CE

RUFFINI, R

机构：

来源：

关键词：

D O I：

10.1086/180672

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：L83 / &

共 16 条

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[2] CORRECTION
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[3] NEUTRON STAR MODELS BASED ON AN IMPROVED EQUATION OF STATE
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[J]. ASTROPHYSICS AND SPACE SCIENCE, 1970, 6 (02) : 228 - &
[4] HADRONIC MATTER NEAR BOILING POINT
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[J]. NUOVO CIMENTO A, 1968, 56 (04): : 1027 - +
[5] HAGEDORN R, 1968, NUOVO CIMENTO, V6, P311
[6] HAGEDORN R, 1965, NUOVO CIMENTO, V3, P147
[7] ON HADRONIC MASS SPECTRUM
HAGEDORN, R
[J]. NUOVO CIMENTO A, 1967, 52 (04): : 1336 - +
[8] HAGEDORN R, 1969, TH1027 CERN REPT
[9] Harrison B. K., 1965, GRAVITATION THEORY G
[10] SLOWLY ROTATING RELATIVISTIC STARS .2. MODELS FOR NEUTRON STARS AND SUPERMASSIVE STARS
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[J]. ASTROPHYSICAL JOURNAL, 1968, 153 (3P1) : 807 - &