NEUTRON-STAR PROPERTIES AND THE RELATIVISTIC EQUATION OF STATE OF ASYMMETRIC NUCLEAR-MATTER

被引：29

作者：

HUBER, H

WEBER, F

WEIGEL, MK

机构：

[1] Sektion Physik, Universität München, D-85748 Garching

来源：

PHYSICAL REVIEW C | 1994年 / 50卷 / 03期

关键词：

D O I：

10.1103/PhysRevC.50.R1287

中图分类号：

O57 [原子核物理学、高能物理学];

学科分类号：

070202 ;

摘要：

We calculate the equation of state of asymmetric nuclear matter in generalized chemical equilibrium in the relativistic Brueckner-Hartree-Fock approximation, and study its impact on the properties of (rapidly) rotating neutron stars by solving the stellar structure equations in the framework of general relativity theory.

引用

页码：R1287 / R1291

页数：5

共 28 条

[1] [Anonymous], 1965, GRAVITATION THEORY G
[2] Baym G., 1978, Nuclear Physics with Heavy Ions and Mesons, P745
[3] FENG D, 1994, S HARMONY PHYSICS
[4] FENG D, IN PRESS PHYS REP
[5] FENG D, LBL34361 REP
[6] Glendenning N. K., 1991, Nuclear Physics B, Proceedings Supplements, V24B, P110, DOI 10.1016/0920-5632(91)90307-Z
[7] NEUTRON-STARS IN THE DERIVATIVE COUPLING MODEL
GLENDENNING, NK
WEBER, F
MOSZKOWSKI, SA
[J]. PHYSICAL REVIEW C, 1992, 45 (02): : 844 - 855
[8] THE HYPERON COMPOSITION OF NEUTRON STARS
GLENDENNING, NK
[J]. PHYSICS LETTERS B, 1982, 114 (06) : 392 - 396
[9] 1ST-ORDER PHASE-TRANSITIONS WITH MORE THAN ONE CONSERVED CHARGE - CONSEQUENCES FOR NEUTRON-STARS
GLENDENNING, NK
[J]. PHYSICAL REVIEW D, 1992, 46 (04): : 1274 - 1287
[10] NEUTRON STARS ARE GIANT HYPERNUCLEI
GLENDENNING, NK
[J]. ASTROPHYSICAL JOURNAL, 1985, 293 (02) : 470 - 493

← 1 2 3 →