Adaptive event horizon tracking and critical phenomena in binary black hole coalescence
Creators
- 1. Center for Relativity, University of Texas at Austin, Austin, Texas 78712-1081 (United States)
Description
This work establishes critical phenomena in the topological transition of black hole coalescence. We describe and validate a computational front tracking event horizon solver, developed for generic studies of the black hole coalescence problem. We then apply this to the Kastor-Traschen axisymmetric analytic solution of the extremal Maxwell-Einstein black hole merger with a cosmological constant. The surprising result of this computational analysis is a power law scaling of the minimal throat proportional to time. The minimal throat connecting the two holes obeys this power law during a short time immediately at the beginning of merger. We also confirm the behavior analytically. Thus, at least in one axisymmetric situation a critical phenomenon exists. We give arguments for a broader universality class than the restricted requirements of the Kastor-Traschen solution
Additional details
Identifiers
- DOI
- 10.1103/PhysRevD.68.104003;
- arXiv
- arXiv:gr-qc/0303109v2;
Publishing Information
- Journal Title
- Physical Review. D, Particles Fields
- Journal Volume
- 68
- Journal Issue
- 10
- Journal Page Range
- p. 104003-104003.13
- ISSN
- 0556-2821
- CODEN
- PRVDAQ
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 35080096
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; S71: CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS;
- Descriptors DEI
- ANALYTICAL SOLUTION; BINARY STARS; BLACK HOLES; COALESCENCE; COSMOLOGICAL CONSTANT; EINSTEIN-MAXWELL EQUATIONS; SCALING LAWS
- Descriptors DEC
- EQUATIONS; FIELD EQUATIONS; MATHEMATICAL SOLUTIONS; STARS
Optional Information
- Notes
- (c) 2003 The American Physical Society