Gravitational waves and pulsating stars: what can we hope to learn from future observations?
Gravitational waves and pulsating stars: what can we hope to learn from future observations?
We present new results for pulsating stars in general relativity. First we show that the so-called gravitational-wave modes of a neutron star can be excited when a gravitational wave impinges on the star. Numerical simulations suggest that the modes may be astrophysically relevant, and we discuss whether they will be observable with future gravitational-wave detectors. We also discuss how such observations could lead to estimates of both the radius and the mass of a neutron star, and thus put constraints on the nuclear equation of state.
4134-4137
Andersson, Nils
2dd6d1ee-cefd-478a-b1ac-e6feedafe304
Kokkotas, Kostas D.
0b8bb98a-a65f-434b-855b-ec5b488b4a96
1996
Andersson, Nils
2dd6d1ee-cefd-478a-b1ac-e6feedafe304
Kokkotas, Kostas D.
0b8bb98a-a65f-434b-855b-ec5b488b4a96
Andersson, Nils and Kokkotas, Kostas D.
(1996)
Gravitational waves and pulsating stars: what can we hope to learn from future observations?
Physical Review Letters, 77 (20), .
(doi:10.1103/PhysRevLett.77.4134).
Abstract
We present new results for pulsating stars in general relativity. First we show that the so-called gravitational-wave modes of a neutron star can be excited when a gravitational wave impinges on the star. Numerical simulations suggest that the modes may be astrophysically relevant, and we discuss whether they will be observable with future gravitational-wave detectors. We also discuss how such observations could lead to estimates of both the radius and the mass of a neutron star, and thus put constraints on the nuclear equation of state.
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Published date: 1996
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Local EPrints ID: 29414
URI: http://eprints.soton.ac.uk/id/eprint/29414
PURE UUID: 4aae53d4-f82d-497a-b00a-1003b1355d76
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Date deposited: 05 Jan 2007
Last modified: 16 Mar 2024 03:01
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Author:
Kostas D. Kokkotas
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