English

Dirac Fermions in Non-trivial Topology Black Hole Backgrounds

High Energy Physics - Theory 2015-03-17 v2 General Relativity and Quantum Cosmology

Abstract

We discuss the behaviour of the Dirac fermions in a general spherically symmetric black hole background with a non-trivial topology of the event horizon. Both massive and massless cases are taken into account. The analytical studies of intermediate and late-time behaviour of massive Dirac hair in the background of a black hole with a global monopole and dilaton black hole pierced by a cosmic string will be conducted. It was revealed that in the case of a global monopole swallowed by a static black hole the intermediate late-time behaviour depends on the mass of the Dirac field, the multiple number of the wave mode and the global monopole parameter. The late-time behaviour is quite independent of these factors and has the decay rate proportional to t5/6t^{-5/6}. As far as the black hole pierced by a cosmic string is concerned the intermediate late-time behaviour depends only on the hair mass and the multipole number of the wave mode while the late-time behaviour dependence is the same as in the previous case. The main modification stems from the topology of the S2S^2 sphere pierced by a cosmic string. This factor modifies the eigenvalues of the Dirac operator acting on the transverse manifold.

Keywords

Cite

@article{arxiv.1004.4952,
  title  = {Dirac Fermions in Non-trivial Topology Black Hole Backgrounds},
  author = {Marek Gozdz and Lukasz Nakonieczny and Marek Rogatko},
  journal= {arXiv preprint arXiv:1004.4952},
  year   = {2015}
}

Comments

15 pages, RevTex, to be published in Phys.Rev.D15, some misprints were corrected