Fermion Emission from Five-Dimensional Black Holes

Abstract

We calculate semiclassically the emission rate of spin 1/2 particles from charged, nonrotating black holes in D=5,N=8 supergravity. The relevant Dirac equation is solved by the same approximation as in the bosonic case. The resulting expression for the emission rate has a form which is predicted from D-brane effective field theory.

28 pages, Latex; 1 reference added

References in corpus (3)

• General Rotating Black Holes in String Theory: Greybody Factors and Event Horizons
• Universal Low-Energy Dynamics for Rotating Black Holes
• Black Hole Greybody Factors and Absorption of Scalars by Effective Strings

Cited by in corpus (6)

• Large N Field Theories, String Theory and Gravity
• Black Holes in Theories with Large Extra Dimensions: a Review
• The Bekenstein Formula and String Theory (N-brane Theory)
• Emission of Fermions from BTZ Black Holes
• Emission spectrum of soft massless states from heavy superstring
• Particle creation by a massless spin-$\frac{1}{2}$ field in a warped cosmological braneworld scenario