CRITERIA FOR PION CONDENSATION THRESHOLDS IN NEUTRON STAR MATTER

被引：13

作者：

AU, CK

BAYM, G

FLOWERS, E

机构：

[1] UNIV ILLINOIS,DEPT PHYSICS,URBANA,IL 61801

[2] NYU,DEPT PHYS,NEW YORK,NY 10003

来源：

PHYSICS LETTERS B | 1974年 / B 51卷 / 01期

关键词：

D O I：

10.1016/0370-2693(74)90135-X

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

收藏

页码：1 / 4

页数：4

相关论文

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[1] PION CONDENSATION IN NEUTRON STAR MATTER - EQUILIBRIUM CONDITIONS AND MODEL CALCULATIONS
BAYM, G
FLOWERS, E
[J]. NUCLEAR PHYSICS A, 1974, A222 (01) : 29 - 64
[2] PION CONDENSATION IN NUCLEAR AND NEUTRON STAR MATTER
BAYM, G
[J]. PHYSICAL REVIEW LETTERS, 1973, 30 (26) : 1340 - 1342
[3] BERTSCH G, IN PRESS
[4] PHASE-TRANSITIONS (PI-CONDENSATION) IN NUCLEI AND NEUTRON STARS
MIGDAL, AB
[J]. PHYSICS LETTERS B, 1973, B 45 (05) : 448 - 450
[5] PHASE-TRANSITION IN NUCLEAR MATTER AND MULTIPARTICLE NUCLEAR FORCES
MIGDAL, AB
[J]. NUCLEAR PHYSICS A, 1973, A210 (02) : 421 - 428
[6] MIGDAL AB, 1973, PHYS REV LETT, V31, P247
[7] COMMENT ON PI CONDENSATION IN NUCLEAR MATTER
SAWYER, RF
[J]. PHYSICAL REVIEW LETTERS, 1973, 31 (26) : 1556 - 1559