Construction of astrophysical initial data for perturbations of relativistic stars
Construction of astrophysical initial data for perturbations of relativistic stars
We develop a framework for constructing initial data sets for perturbations about spherically symmetric matter distributions. This framework facilitates setting initial data representing sources of gravitational radiation involving relativistic stars. The procedure is based on the Lichnerowicz-York conformal approach to solve the constraints in Einstein’s equations. The correspondence of these initial data sets in terms of the standard gauge perturbation variables in the Regge-Wheeler perturbation variables is established, and examples of initial data sets of merging neutron stars under the close-limit approximation are presented.
4004-4015
Andersson, N.
2dd6d1ee-cefd-478a-b1ac-e6feedafe304
Kokkotas, K.D.
7bdb71db-179a-4f68-9f5d-bd45dfea7dfc
Laguna, P.
f8cbe99f-659e-41a8-b005-3ecfbedb09ea
Papadopoulos, P.
80a975f2-0aa9-4ef3-a266-550ca44c3cc7
Sipior, M.S.
4c334237-9060-4f83-b860-82957806ba1b
1999
Andersson, N.
2dd6d1ee-cefd-478a-b1ac-e6feedafe304
Kokkotas, K.D.
7bdb71db-179a-4f68-9f5d-bd45dfea7dfc
Laguna, P.
f8cbe99f-659e-41a8-b005-3ecfbedb09ea
Papadopoulos, P.
80a975f2-0aa9-4ef3-a266-550ca44c3cc7
Sipior, M.S.
4c334237-9060-4f83-b860-82957806ba1b
Andersson, N., Kokkotas, K.D., Laguna, P., Papadopoulos, P. and Sipior, M.S.
(1999)
Construction of astrophysical initial data for perturbations of relativistic stars.
Physical Review D, 60 (12), .
(doi:10.1103/PhysRevD.60.124004).
Abstract
We develop a framework for constructing initial data sets for perturbations about spherically symmetric matter distributions. This framework facilitates setting initial data representing sources of gravitational radiation involving relativistic stars. The procedure is based on the Lichnerowicz-York conformal approach to solve the constraints in Einstein’s equations. The correspondence of these initial data sets in terms of the standard gauge perturbation variables in the Regge-Wheeler perturbation variables is established, and examples of initial data sets of merging neutron stars under the close-limit approximation are presented.
This record has no associated files available for download.
More information
Published date: 1999
Identifiers
Local EPrints ID: 29427
URI: http://eprints.soton.ac.uk/id/eprint/29427
ISSN: 1550-7998
PURE UUID: 3e54fd76-b2de-4500-9cdd-0b21342fda9b
Catalogue record
Date deposited: 05 Jan 2007
Last modified: 16 Mar 2024 03:01
Export record
Altmetrics
Contributors
Author:
K.D. Kokkotas
Author:
P. Laguna
Author:
P. Papadopoulos
Author:
M.S. Sipior
Download statistics
Downloads from ePrints over the past year. Other digital versions may also be available to download e.g. from the publisher's website.
View more statistics