Slowly rotating boson-fermion star

被引:12
|
作者
De Sousa, CMG
Silveira, V
机构
[1] Univ Brasilia, Int Ctr Condensed Matter Phys, BR-70919970 Brasilia, DF, Brazil
[2] Univ Catolica brasilia, Diretoria Matemat, EPCT, BR-72022900 Brasilia, DF, Brazil
来源
关键词
D O I
10.1142/S0218271801001360
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Relativistic prescription is used to study the slow rotation of stars composed by self-gravitating bosons and fermions (fermions may be considered as neutrons). Previous results demand that purely boson stars are unable to display slow rotation, if one uses relativistic prescription with classical scalar fields. In contrast to this, the present work shows that a combined boson-fermion star in its ground-state can rotate. Its structure and stability are analysed under slow rotation approximations.
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收藏
页码:881 / 892
页数:12
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