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Black Hole Creation in 2+1 Dimensions

Hans-Juergen Matschull

TL;DR

In 2+1 dimensional gravity with a negative cosmological constant, the paper shows that two point particles colliding in $AdS_3$ can form a BTZ black hole. It uses a cutting-gluing construction based on holonomies in $SL(2)$ to build the spacetime and analyzes the threshold energy that separates massive outcomes from black hole formation, with the horizon length fixed by the holonomy as $2\mu$ (the black hole mass). The approach yields an explicit solution describing the collapse into a non-rotating BTZ black hole and discusses extremal and rotating generalizations, including the global causal structure of black hole formation in AdS$_3$. The work provides a concrete, exact framework for black hole formation in a toy model of quantum gravity and clarifies the role of holonomies and geodesics in 3D AdS gravity.

Abstract

When two point particles, coupled to three dimensional gravity with a negative cosmological constant, approach each other with a sufficiently large center of mass energy, then a BTZ black hole is created. An explicit solution to the Einstein equations is presented, describing the collapse of two massless particles into a non-rotating black hole. Some general arguments imply that massive particles can be used as well, and the creation of a rotating black hole is also possible.

Black Hole Creation in 2+1 Dimensions

TL;DR

In 2+1 dimensional gravity with a negative cosmological constant, the paper shows that two point particles colliding in can form a BTZ black hole. It uses a cutting-gluing construction based on holonomies in to build the spacetime and analyzes the threshold energy that separates massive outcomes from black hole formation, with the horizon length fixed by the holonomy as (the black hole mass). The approach yields an explicit solution describing the collapse into a non-rotating BTZ black hole and discusses extremal and rotating generalizations, including the global causal structure of black hole formation in AdS. The work provides a concrete, exact framework for black hole formation in a toy model of quantum gravity and clarifies the role of holonomies and geodesics in 3D AdS gravity.

Abstract

When two point particles, coupled to three dimensional gravity with a negative cosmological constant, approach each other with a sufficiently large center of mass energy, then a BTZ black hole is created. An explicit solution to the Einstein equations is presented, describing the collapse of two massless particles into a non-rotating black hole. Some general arguments imply that massive particles can be used as well, and the creation of a rotating black hole is also possible.

Paper Structure

This paper contains 5 sections, 69 equations, 8 figures.

Figures (8)

  • Figure 1: Construction of a geodesic on the Poincaré disc
  • Figure 2: A particle cutting out a wedge from Minkowski space.
  • Figure 3: A massless particle passing through anti-de-Sitter space
  • Figure 4: Two particles colliding and joining.
  • Figure 5: Two massless particles joining and forming a massive particle.
  • ...and 3 more figures