Resonant Shattering of Neutron Star Crusts

David Tsang, Jocelyn S. Read, Tanja Hinderer, Anthony L. Piro, Ruxandra Bondarescu

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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.
Original languageEnglish
Article number011102
JournalPhysical Review Letters
Volume108
Issue number1
DOIs
Publication statusPublished - Jan 2012

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Tsang, D., Read, J. S., Hinderer, T., Piro, A. L., & Bondarescu, R. (2012). Resonant Shattering of Neutron Star Crusts. Physical Review Letters, 108(1), [011102]. https://doi.org/10.1103/PhysRevLett.108.011102