Critical phenomena in the gravitational collapse of electromagnetic waves
Critical phenomena in the gravitational collapse of electromagnetic waves
We numerically investigate the threshold of black-hole formation in the gravitational collapse of electromagnetic waves in axisymmetry. We find approximate power-law scaling
ρ
max
∼
(
η
∗
−
η
)
−
2
γ
of the maximum density in the time evolution of near-subcritical data with
γ
≃
0.145
, where
η
is the amplitude of the initial data. We directly observe approximate discrete self-similarity in near-critical time evolutions with a log-scale echoing period of
Δ
≃
0.55
. The critical solution is approximately the same for two families of initial data, providing some evidence of universality. Neither the discrete self-similarity nor the universality, however, are exact. We speculate that the absence of an exactly discrete self-similarity might be caused by the interplay of electromagnetic and gravitational wave degrees of freedom, or by the presence of higher-order angular multipoles, or both, and discuss implications of our findings for the critical collapse of vacuum gravitational waves.
Baumgarte, Thomas W.
fa9007a1-bb4a-4527-b199-5fc26e0ff89c
Gundlach, Carsten
586f1eb5-3185-4b2b-8656-c29c436040fc
Hilditch, David
108ec927-5127-4228-86d5-493291f22021
Baumgarte, Thomas W.
fa9007a1-bb4a-4527-b199-5fc26e0ff89c
Gundlach, Carsten
586f1eb5-3185-4b2b-8656-c29c436040fc
Hilditch, David
108ec927-5127-4228-86d5-493291f22021
Baumgarte, Thomas W., Gundlach, Carsten and Hilditch, David
(2019)
Critical phenomena in the gravitational collapse of electromagnetic waves.
Physical Review Letters, 123 (17), [171103].
(doi:10.1103/PhysRevLett.123.171103).
Abstract
We numerically investigate the threshold of black-hole formation in the gravitational collapse of electromagnetic waves in axisymmetry. We find approximate power-law scaling
ρ
max
∼
(
η
∗
−
η
)
−
2
γ
of the maximum density in the time evolution of near-subcritical data with
γ
≃
0.145
, where
η
is the amplitude of the initial data. We directly observe approximate discrete self-similarity in near-critical time evolutions with a log-scale echoing period of
Δ
≃
0.55
. The critical solution is approximately the same for two families of initial data, providing some evidence of universality. Neither the discrete self-similarity nor the universality, however, are exact. We speculate that the absence of an exactly discrete self-similarity might be caused by the interplay of electromagnetic and gravitational wave degrees of freedom, or by the presence of higher-order angular multipoles, or both, and discuss implications of our findings for the critical collapse of vacuum gravitational waves.
Text
Critical Phenomena in the gravitational collapse of electromagnetic wavespdf
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Accepted/In Press date: 22 September 2019
e-pub ahead of print date: 25 October 2019
Identifiers
Local EPrints ID: 436044
URI: http://eprints.soton.ac.uk/id/eprint/436044
ISSN: 0031-9007
PURE UUID: a7d1f6be-5da8-441c-97d8-9a815f81218e
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Date deposited: 27 Nov 2019 17:30
Last modified: 17 Mar 2024 02:51
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Author:
Thomas W. Baumgarte
Author:
David Hilditch
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