PION CONDENSATION IN NUCLEAR AND NEUTRON STAR MATTER

被引：105

作者：

BAYM, G ^{[1
]}

机构：

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

来源：

关键词：

D O I：

10.1103/PhysRevLett.30.1340

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

引用

页码：1340 / 1342

页数：3

共 9 条

[1] BAHCALL JN, 1965, PHYS REV, V140, P1445
[2] BAHCALL JN, 1965, PHYS REV, V140, P1452
[3] POSSIBILITY OF A PHASE-TRANSITION TO A PION CONDENSATE IN NEUTRON STARS
BARSHAY, S
VAGRADOV, G
BROWN, GE
[J]. PHYSICS LETTERS B, 1973, B 43 (05) : 359 - 361
[4] BAYM G, TO BE PUBLISHED
[5] PI-CONDENSATION AND NEUTRON STAR COOLING
KOGUT, J
MANASSAH, JT
[J]. PHYSICS LETTERS A, 1972, A 41 (02) : 129 - &
[6] MIGDAL AB, 1972, SOV PHYS JETP-USSR, V34, P1184
[7] MIGDAL AB, 1971, ZH EKSP TEOR FIZ, V61, P2210
[8] PION CONDENSATION IN SUPERDENSE NUCLEAR MATTER
SAWYER, RF
SCALAPINO, DJ
[J]. PHYSICAL REVIEW D, 1973, 7 (04) : 953 - 964
[9] STANDING PION WAVES IN SUPERDENSE MATTER
SAWYER, RF
YAO, AC
[J]. PHYSICAL REVIEW D, 1973, 7 (06): : 1579 - 1586