Fermion excitations of a tense brane black hole

Abstract

By finding the spinor eigenvalues for a single deficit angle (d-2)-sphere, we derive the radial potential for fermions on a d-dimensional black hole background that is embedded on a codimension two brane with conical singularity, where the deficit angle is related to the brane tension. From this we obtain the quasi-normal mode spectrum for bulk fermions on such a background. As a byproduct of our method, this also gives a rigorous proof for integer spin fields on the deficit 2-sphere.

7 pages, 1 figure

References in corpus (6)

• Split fermion quasi-normal modes
• Evaporation of a black hole off of a tense brane
• Wave dynamics of a six-dimensional black hole localized on a tensional three-brane
• High-energy black hole production
• Bulk dominated fermion emission on a Schwarzschild background
• Quasi-normal modes of a black hole localized on a codimension-two brane of finite tension

Cited by in corpus (9)

• Instability of higher dimensional charged black holes in the de-Sitter world
• Stability of higher dimensional Reissner-Nordstrom-anti-de Sitter black holes
• Decay of Dirac Massive Hair in the Background of Spherical Black Hole
• Greybody Factors for Rotating Black Holes on Codimension-2 Branes
• Quasinormal modes of black holes localized on the Randall-Sundrum 2-brane
• Gravitational parameter estimation in a waveguide
• Particle emission from a black hole on a tense codimension-2 brane
• Evolution of Massive Scalar Fields in the Spacetime of a Tense Brane Black Hole
• Fermion evaporation of a black hole off a tense brane