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Permanent URL to this publication: http://dx.doi.org/10.5167/uzh-55338

Tsang, D; Read, J S; Hinderer, T; Piro, A L; Bondarescu, R (2011). Resonant shattering of neutron star crusts. Physical Review Letters, 108(1):011102.

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Abstract

The resonant excitation of neutron star (NS) modes by tides is investigated as a source of short gamma-ray burst (SGRB) precursors. We find that the driving of a crust-core interface mode can lead to shattering of the NS crust, liberating ˜1046-1047erg of energy seconds before the merger of a NS-NS or NS-black-hole binary. Such properties are consistent with Swift/BAT detections of SGRB precursors, and we use the timing of the observed precursors to place weak constraints on the crust equation of state. We describe how a larger sample of precursor detections could be used alongside coincident gravitational wave detections of the inspiral by Advanced LIGO class detectors to probe the NS structure. These two types of observations nicely complement one another, since the former constrains the equation of state and structure near the crust-core boundary, while the latter is more sensitive to the core equation of state.

Item Type:Journal Article, refereed, original work
Communities & Collections:07 Faculty of Science > Institute for Computational Science
DDC:530 Physics
Language:English
Date:January 2011
Deposited On:19 Feb 2012 13:22
Last Modified:14 Jul 2014 04:46
Publisher:American Physical Society
ISSN:0031-9007 (P) 1079-7114 (E)
Publisher DOI:10.1103/PhysRevLett.108.011102
Related URLs:http://arxiv.org/abs/1110.0467
Citations:Web of Science®. Times Cited: 23
Google Scholar™
Scopus®. Citation Count: 21

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