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