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 [J].

GLENDENNING, NK ;

WEBER, F ;

MOSZKOWSKI, SA .

PHYSICAL REVIEW C, 1992, 45 (02) :844-855

[8] THE HYPERON COMPOSITION OF NEUTRON STARS [J].

GLENDENNING, NK .

PHYSICS LETTERS B, 1982, 114 (06) :392-396

[9] 1ST-ORDER PHASE-TRANSITIONS WITH MORE THAN ONE CONSERVED CHARGE - CONSEQUENCES FOR NEUTRON-STARS [J].

GLENDENNING, NK .

PHYSICAL REVIEW D, 1992, 46 (04) :1274-1287

[10] NEUTRON STARS ARE GIANT HYPERNUCLEI [J].

GLENDENNING, NK .

ASTROPHYSICAL JOURNAL, 1985, 293 (02) :470-493

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