Analytical treatment of SUSY Quasi-normal modes in a non-rotating Schwarzschild black hole

Details Analytical treatment of SUSY Quasi-normal modes in a non-rotating Schwarzschild black hole Analytical treatment of SUSY Quasi-normal modes in a non-rotating Schwarzschild black hole

2010-06-19

arxiv.org/abs/1006.3860v4

Eur.Phys.J.C71:1526,2011

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

Version to be published in European Physical Journal C

Scientific paper

10.1140/epjc/s10052-010-1526-9

We use the Fock-Ivanenko formalism to obtain the Dirac equation which describes the interaction of a massless 1/2-spin neutral fermion with a gravitational field around a Schwarzschild black hole (BH). We obtain approximated analytical solutions for the eigenvalues of the energy (quasi-normal frequencies) and their corresponding eigenstates (quasi-normal states). The interesting result is that all the excited states [and their supersymmetric (SUSY) partners] have a purely imaginary frequency, which can be expressed in terms of the Hawking temperature. Furthermore, as one expects for SUSY Hamiltonians, the isolated bottom state has a real null energy eigenvalue.

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