Dirac fermions in nontrivial topology black hole backgrounds

被引:6
|
作者
Gozdz, Marek [1 ]
Nakonieczny, Lukasz [2 ]
Rogatko, Marek [2 ]
机构
[1] Marie Curie Sklodowska Univ, Inst Informat, PL-20031 Lublin, Poland
[2] Marie Curie Sklodowska Univ, Inst Phys, PL-20031 Lublin, Poland
关键词
ABELIAN GAUGE-FIELDS; QUASI-NORMAL MODES; EQUATION; NONEXISTENCE; EXCITATION; PARTICLES; COLLAPSE; GRAVITY;
D O I
10.1103/PhysRevD.81.104027
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We discuss the behavior of the Dirac fermions in a general spherically symmetric black hole background with a nontrivial topology of the event horizon. Both massive and massless cases are taken into account. We will conduct an analytical study of intermediate and late-time behavior of massive Dirac hair in the background of a black hole with a global monopole and dilaton black hole pierced by a cosmic string. In the case of a global monopole swallowed by a static black hole, the intermediate late-time behavior depends on the mass of the Dirac field, the multiple number of the wave mode, and the global monopole parameter. The late-time behavior is quite independent of these factors and has a decay rate proportional to t(-5/6). As far as the black hole pierced by a cosmic string is concerned, the intermediate late-time behavior depends only on the hair mass and the multipole number of the wave mode, while the late-time behavior dependence is the same as in the previous case. The main modification stems from the topology of the S-2 sphere pierced by a cosmic string. This factor modifies the eigenvalues of the Dirac operator acting on the transverse manifold.
引用
收藏
页数:12
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