Excision without excision
Excision without excision
We analyze and apply an alternative to black hole excision based on smoothing the interior of black holes with arbitrary -- possibly constraint violating -- initial data, and solving the vacuum Einstein evolution equations everywhere. By deriving the constraint propagation system for our hyperbolic formulation of the BSSN evolution system we rigorously prove that the constraints propagate causally and so any constraint violations introduced inside the black holes cannot affect the exterior spacetime. (This does not follow from the causal structure of the spacetime as is often assumed.) We present numerical evolutions of Cook-Pfeiffer binary black hole initial configurations showing that these techniques appear to work robustly for generic data. We also present numerical evidence from spherically symmetric evolutions that for the gauge conditions used the same stationary end-state is approached irrespective of the choice of initial data and smoothing procedure.
numerical relativity, black Holes, excision
081503(R)
Brown, David
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Sarbach, Olivier
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Schnetter, Erik
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Tiglio, Manuel
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Diener, Peter
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Hawke, Ian
fc964672-c794-4260-a972-eaf818e7c9f4
Pollney, Denis
a78b371e-934f-4fed-8754-91db5cdeb23e
2007
Brown, David
68e8f8ee-6aaf-45e4-9aee-7f76e39ddefe
Sarbach, Olivier
9b1b946c-5ff3-4eeb-b685-915c662edff8
Schnetter, Erik
fa61f1d3-135d-47af-80e2-4285f37a1e24
Tiglio, Manuel
70c1e9ee-b30c-4354-af43-1bd3b4b6af24
Diener, Peter
62485bb0-81d7-49df-b5ad-8f66610efc55
Hawke, Ian
fc964672-c794-4260-a972-eaf818e7c9f4
Pollney, Denis
a78b371e-934f-4fed-8754-91db5cdeb23e
Brown, David, Sarbach, Olivier, Schnetter, Erik, Tiglio, Manuel, Diener, Peter, Hawke, Ian and Pollney, Denis
(2007)
Excision without excision.
Physical Review D, 76, .
(doi:10.1103/PhysRevD.76.081503).
Abstract
We analyze and apply an alternative to black hole excision based on smoothing the interior of black holes with arbitrary -- possibly constraint violating -- initial data, and solving the vacuum Einstein evolution equations everywhere. By deriving the constraint propagation system for our hyperbolic formulation of the BSSN evolution system we rigorously prove that the constraints propagate causally and so any constraint violations introduced inside the black holes cannot affect the exterior spacetime. (This does not follow from the causal structure of the spacetime as is often assumed.) We present numerical evolutions of Cook-Pfeiffer binary black hole initial configurations showing that these techniques appear to work robustly for generic data. We also present numerical evidence from spherically symmetric evolutions that for the gauge conditions used the same stationary end-state is approached irrespective of the choice of initial data and smoothing procedure.
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Published date: 2007
Keywords:
numerical relativity, black Holes, excision
Identifiers
Local EPrints ID: 49013
URI: http://eprints.soton.ac.uk/id/eprint/49013
ISSN: 1550-7998
PURE UUID: a7a05158-4add-4c2c-9484-396661c46b36
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Date deposited: 19 Oct 2007
Last modified: 16 Mar 2024 03:45
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Contributors
Author:
David Brown
Author:
Olivier Sarbach
Author:
Erik Schnetter
Author:
Manuel Tiglio
Author:
Peter Diener
Author:
Denis Pollney
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