pith. sign in

arxiv: gr-qc/0312029 · v2 · submitted 2003-12-04 · 🌀 gr-qc

Quasinormal modes for Weyl neutrino field in R-N black holes

classification 🌀 gr-qc
keywords blackfieldholesneutrinoquasinormalweylfrequenciesmode
0
0 comments X
read the original abstract

We employ WKB approximation up to the third order to determine the low-lying quasinormal modes for Weyl neutrino field in R-N black holes, which are the most relevant to the evolution of the field around a black hole in the intermediate stage. It is showed that the quasinormal mode frequencies for Weyl neutrino field in R-N black holes are different from those in Schwartzchild black holes owning to the charge-induced additional gravitation, and the variations of the quasinormal mode frequencies for Weyl neutrino field are similar to those for integral spin fields in R-N black holes.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Fermionic Love number of Reissner-Nordstr\"om black holes

    gr-qc 2025-10 unverdicted novelty 6.0

    Static fermionic tidal Love numbers are non-vanishing for non-extremal Reissner-Nordström black holes.

  2. Quasinormal modes of black holes: from astrophysics to string theory

    gr-qc 2011-02 accept novelty 1.0

    This review surveys calculations and interpretations of quasinormal modes for black holes in astrophysics, higher dimensions, and holographic duals without presenting new results.