Evaporation of Schwarzschild Black Hole in the Large N Matrix Theory
Yi-hong Gao, Wei Zhang

TL;DR
This paper models the evaporation of Schwarzschild black holes within the large N Matrix theory using D0-brane clusters, deriving the Hawking radiation rate and providing evidence for Lorentz invariance in this framework.
Contribution
It presents a derivation of the Hawking evaporation rate for Schwarzschild black holes in the large N Matrix model using D0-brane clusters, supporting Lorentz invariance.
Findings
Correct formula for Hawking evaporation rate derived
Evidence supporting Lorentz invariance in Matrix model physics
Modeling black hole evaporation within large N Matrix theory
Abstract
By using the D0-brane cluster picture, we consider the Hawking radiation of Schwarszchild black hole (SBH) in large N Matrix model. We get the correct formula for the the Hawing evaporation rate. Our results give some evidence on the Lorentz invariance of the physics of Matrix model.
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.
Taxonomy
TopicsBlack Holes and Theoretical Physics · Cosmology and Gravitation Theories · Relativity and Gravitational Theory
