Solution of Dirac equation in the near horizon geometry of an extreme Kerr black hole

Abstract

Dirac equation is solved in the near horizon limit geometry of an extreme Kerr black hole. We decouple equations first as usual, into an axial and angular part. The axial equation turns out to be independent of the mass and is solved exactly. The angular equation reduces, in the massless case, to a confluent Heun equation. In general for nonzero mass, the angular equation is expressible at best, as a set of coupled first order differential equations apt for numerical investigation. The axial potentials corresponding to the associated Schrodinger-type equations and their conserved currents are found. Finally, based on our solution, we verify in a similar way the absence of superradiance for Dirac particles in the near horizon, a result which is well-known within the context of general Kerr background.

arXiv comment20 pages, no figure, to be appeared in Phys.Rev.D

References in corpus (3)

• The Extreme Kerr Throat Geometry: A Vacuum Analog of AdS_2 x S^2
• Conformal mechanics on rotating Bertotti-Robinson spacetime
• Near Horizon Geometry of Extreme Black Holes and Colliding Waves

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