Critical gravitational collapse with angular momentum
General Relativity and Quantum Cosmology
2016-10-12 v2
Abstract
We derive a theoretical model of mass and angular momentum scaling in type-II critical collapse with rotation. We focus on the case where the critical solution has precisely one, spherically symmetric, unstable mode. We demonstrate excellent agreement with numerical results for critical collapse of a rotating radiation fluid, which falls into this case.
Keywords
Cite
@article{arxiv.1608.00491,
title = {Critical gravitational collapse with angular momentum},
author = {Carsten Gundlach and Thomas W. Baumgarte},
journal= {arXiv preprint arXiv:1608.00491},
year = {2016}
}
Comments
Version accepted for publication in PRD