Fermion Emission from Five-Dimensional Black Holes
Kazuo Hosomichi
TL;DR
This paper calculates the semiclassical emission rate of spin 1/2 particles from five-dimensional charged black holes in supergravity, aligning with predictions from D-brane effective field theory.
Contribution
It provides the first semiclassical calculation of fermion emission rates from five-dimensional black holes in supergravity, confirming theoretical predictions.
Findings
Emission rate matches D-brane effective field theory predictions
Method extends previous bosonic emission calculations to fermions
Supports the consistency of supergravity and string theory models
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.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.