Greybody factors for rotating black holes in four dimensions
Mirjam Cvetic, Finn Larsen

TL;DR
This paper derives the wave equation for scalar fields around rotating four-dimensional black holes, calculates greybody factors for Hawking radiation, and interprets the emission spectrum via an effective string theory approach.
Contribution
It provides a detailed analysis of greybody factors for rotating 4D black holes, extending previous 5D results, and offers a string theory interpretation of Hawking radiation spectra.
Findings
Greybody factors calculated for non-extremal black holes.
Emission spectrum analyzed for large partial wave numbers.
Effective string theory description of Hawking radiation spectrum.
Abstract
We present the wave equation for a minimally coupled scalar field in the background of a rotating four-dimensional black hole that is parametrized by its mass, angular momentum, and four independent U(1) charges. The near horizon structure is identical to the five-dimensional case, and suggestive of an underlying description in string theory that is valid in the general non-extremal case. We calculate the greybody factors for the Hawking radiation. For sufficiently large partial wave number the emission spectrum can be calculated for general non-extremal black holes and any particle energy. We interpret this spectrum in terms of a multi-body process in an effective string 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.
