PION CONDENSATION IN NEUTRON STAR MATTER - EQUILIBRIUM CONDITIONS AND MODEL CALCULATIONS

被引：93

作者：

BAYM, G ^{[1
]}

FLOWERS, E ^{[1
]}

机构：

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

来源：

关键词：

D O I：

10.1016/0375-9474(74)90583-1

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：

引用

页码：29 / 64

页数：36

共 30 条

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[2] AU CK, TO BE PUBLISHED
[3] BAHCALL JN, 1965, PHYS REV, V140, P1445
[4] BAHCALL JN, 1965, PHYS REV, V140, P1452
[5] DEATH TO PION CONDENSATES IN NUCLEAR MATTER
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BROWN, GE
[J]. PHYSICS LETTERS B, 1973, B 47 (02) : 107 - 109
[6] POSSIBILITY OF A PHASE-TRANSITION TO A PION CONDENSATE IN NEUTRON STARS
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[J]. PHYSICS LETTERS B, 1973, B 43 (05) : 359 - 361
[7] BARSHAY S, 1973, 5 P INT C HIGH EN NU
[8] NEUTRON STAR MATTER
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[J]. NUCLEAR PHYSICS A, 1971, A175 (02) : 225 - &
[9] PION CONDENSATION IN NUCLEAR AND NEUTRON STAR MATTER
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[10] THEORY OF NUCLEAR MATTER
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