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Excitation of neutron star normal modes during binary inspiral

Reisenegger, Andreas and Goldreich, Peter (1994) Excitation of neutron star normal modes during binary inspiral. Astrophysical Journal, 426 (2). pp. 688-691. ISSN 0004-637X. https://resolver.caltech.edu/CaltechAUTHORS:20130417-134602700

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Abstract

As a compact binary inspirals due to the emission of gravitational waves, its orbital period decreases continuously down to approximately 1 ms, its value at coalescence. During the last part of the inspiral, the two stars are close together, and their tidal interactions become strong. Neutron stars have many normal modes (core g-modes, crustal discontinuity modes, shear modes, etc.) whose periods lie in the range (approximately several ms) swept by the orbital period. Some of these modes are resonantly excited by the tidal force. The amount of energy a mode absorbs is proportional to the square of the overlap integral between its displacement field and the tidal force field. For all modes of interest, this overlap is poor, resulting in relatively weak excitation. For the best case, the absorbed energy is only a small fraction (approximately 10^(-6)) of the orbital energy, so the orbital phase shift is too weak to be detected by observations of the gravitational wave signal emitted by the inspiraling binary. However, with displacement amplitudes of excited quadrupole modes ranging up to 0.5% of the stellar radius, the possibility of a detectable electromagnetic signature cannot be dismissed. Both the periods of the modes and the energy they absorb depend quite strongly on the internal structure of the star. Their observation could shed light on the correct high-density equation of state.


Item Type:Article
Related URLs:
URLURL TypeDescription
http://dx.doi.org/10.1086/174105DOIUNSPECIFIED
http://adsabs.harvard.edu/doi/10.1086/174105PublisherUNSPECIFIED
Additional Information:© 1994 American Astronomical Society. Received 1993 August 26; accepted 1993 November 12. We are grateful to Lars Bildsten, Eanna Flanagan, Dong Lai, Patrick McDermott, Tod Strohmayer, Hugh Van Horn, and Yanqin Wu for informative conversations. This work was supported by NSF grant AST 89-13664 and NASA grant NAGW2372.
Funders:
Funding AgencyGrant Number
NSFAST 89-13664
NASANAGW 2372
Subject Keywords:binaries: close; gravitation; stars: neutron; stars: oscillations
Issue or Number:2
Record Number:CaltechAUTHORS:20130417-134602700
Persistent URL:https://resolver.caltech.edu/CaltechAUTHORS:20130417-134602700
Official Citation:Excitation of neutron star normal modes during binary inspiral Reisenegger, Andreas; Goldreich, Peter Astrophysical Journal, vol. 426, no.2, p.688-691, 1994
Usage Policy:No commercial reproduction, distribution, display or performance rights in this work are provided.
ID Code:37995
Collection:CaltechAUTHORS
Deposited By: Ruth Sustaita
Deposited On:19 Apr 2013 18:07
Last Modified:03 Oct 2019 04:53

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