Dynamics and gravitational wave signature of collapsar formation
Dynamics and gravitational wave signature of collapsar formation
We perform 3+1 general relativistic simulations of rotating core collapse in the context of the collapsar model for long gamma-ray bursts. We employ a realistic progenitor, rotation based on results of stellar evolution calculations, and a simplified equation of state. Our simulations track self-consistently collapse, bounce, the postbounce phase, black hole formation, and the subsequent early hyperaccretion phase. We extract gravitational waves from the spacetime curvature and identify a unique gravitational wave signature associated with the early phase of collapsar formation
161103-[4 pages]
Ott, C.D.
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Reisswig, C.
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Schnetter, E.
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O'Connor, E.
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Sperhake, U.
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Loeffler, F.
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Diener, P.
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Abdikamalov, E.
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Hawke, I.
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Burrows, A.
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8 December 2010
Ott, C.D.
09af5461-86ca-4840-be3a-90f258b1f6be
Reisswig, C.
7c08299f-467e-4589-91f8-cb8c52c93298
Schnetter, E.
544c2aff-bf71-45af-8d32-230f486eb837
O'Connor, E.
9fa323ff-e890-4196-931e-e800ee2ac492
Sperhake, U.
cf4a7e32-ded0-4733-92a7-89318207c158
Loeffler, F.
badfdf01-cb15-4bff-8f5e-e6f0aa273868
Diener, P.
aae1812e-86aa-4957-a9f7-861a847a5630
Abdikamalov, E.
9565a108-10a8-4026-8e29-89dea33b1659
Hawke, I.
fc964672-c794-4260-a972-eaf818e7c9f4
Burrows, A.
cd63946a-6733-439d-a071-225505c8c34c
Ott, C.D., Reisswig, C., Schnetter, E., O'Connor, E., Sperhake, U., Loeffler, F., Diener, P., Abdikamalov, E., Hawke, I. and Burrows, A.
(2010)
Dynamics and gravitational wave signature of collapsar formation.
Physical Review Letters, 106 (16), .
(doi:10.1103/PhysRevLett.106.161103).
Abstract
We perform 3+1 general relativistic simulations of rotating core collapse in the context of the collapsar model for long gamma-ray bursts. We employ a realistic progenitor, rotation based on results of stellar evolution calculations, and a simplified equation of state. Our simulations track self-consistently collapse, bounce, the postbounce phase, black hole formation, and the subsequent early hyperaccretion phase. We extract gravitational waves from the spacetime curvature and identify a unique gravitational wave signature associated with the early phase of collapsar formation
Other
1012.1853v1
- Author's Original
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Published date: 8 December 2010
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Imported from arXiv
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Mathematics
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Local EPrints ID: 180747
URI: http://eprints.soton.ac.uk/id/eprint/180747
PURE UUID: 6bac0df3-fbcb-4f42-830a-f355a86ec7f5
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Date deposited: 13 Apr 2011 10:41
Last modified: 15 Mar 2024 03:22
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Author:
C.D. Ott
Author:
C. Reisswig
Author:
E. Schnetter
Author:
E. O'Connor
Author:
U. Sperhake
Author:
F. Loeffler
Author:
P. Diener
Author:
E. Abdikamalov
Author:
A. Burrows
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