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：

INTERNATIONAL JOURNAL OF MODERN PHYSICS D | 2004年 / 13卷 / 07期

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

页码：1365 / 1373

页数：9

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