Effective mesonic and baryonic degrees of freedom in neutron stars

被引:2
|
作者
Dillig, M [1 ]
Schott, M
机构
[1] Univ Erlangen Nurnberg, Inst Theoret Phys 3, D-91058 Erlangen, Germany
[2] Univ Fed Rio Grande do Sul, Inst Fis, BR-91501970 Porto Alegre, RS, Brazil
来源
关键词
nuclear matter; mesonic systems; baryonic systems; neutron stars;
D O I
10.1142/S0218271804005559
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We present a sketchy survey on the role of effective mesonic and baxyonic degrees of freedom in dense hadronic matter and briefly mention still very crude attempts to include constituent quarks degrees of freedom for a transition to a quark gluon plasma.
引用
收藏
页码:1365 / 1373
页数:9
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