English

The Brown-York mass and the Thorne hoop conjecture

General Relativity and Quantum Cosmology 2010-11-11 v1

Abstract

The Thorne hoop conjecture is an attempt to make precise the notion that gravitational collapse occurs if enough energy is compressed into a small enough volume, with the `size' being defined by the circumference. We can make a precise statement of this form, in spherical symmetry, using the Brown-York mass as our measure of the energy. Consider a spherical 2-surface in a spherically symmetric spacetime. If the Brown-York mass, MBYM_{BY}, and the circumference, CC, satisfy C<2πMBYC < 2\pi M_{BY}, then the system must either have emerged from a white hole or will collapse into a black hole. We show that no equivalent result can hold true using either the Liu-Yau mass, MLYM_{LY} or the Wang-Yau mass, MWYM_{WY}. This forms a major obstacle to any attempt to establish a Thorne-type hoop theorem in the general case based on either the Liu-Yau or the Wang-Yau mass.

Keywords

Cite

@article{arxiv.0912.4001,
  title  = {The Brown-York mass and the Thorne hoop conjecture},
  author = {Niall O Murchadha and Roh-Suan Tung and Naqing Xie and Edward Malec},
  journal= {arXiv preprint arXiv:0912.4001},
  year   = {2010}
}

Comments

4 pages; accepted for publication in Physical Review Letters