Emergence of the fuzzy horizon through gravitational collapse
Anand Murugan, Vatche Sahakian

TL;DR
This paper explores how gravitational collapse in light-cone M theory leads to a phase transition forming large membranes, supporting the fuzzball and Matrix black hole models through non-commutative dynamics.
Contribution
It demonstrates the emergence of a fuzzy horizon via a thermodynamic phase transition involving D-brane binding during black hole formation in M theory.
Findings
Formation of large membranes at the horizon
Support for fuzzball and Matrix black hole models
Universal phase transition in gravitational collapse
Abstract
For a large enough Schwarzschild black hole, the horizon is a region of space where gravitational forces are weak; yet it is also a region leading to numerous puzzles connected to stringy physics. In this work, we analyze the process of gravitational collapse and black hole formation in the context of light-cone M theory. We find that, as a shell of matter contracts and is about to reveal a black hole horizon, it undergoes a thermodynamic phase transition. This involves the binding of D0 branes into D2's, and the new phase leads to large membranes of the size of the horizon. These in turn can sustain their large size through back-reaction and the dielectric Myers effect - realizing the fuzzball proposal of Mathur and the Matrix black hole of M(atrix) theory. The physics responsible for this phenomenon lies in strongly coupled 2+1 dimensional non-commutative dynamics. The phenomenon has…
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.
