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Crustal failure during binary inspiral

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arxiv 1109.5041 v1 pith:BVYLMV53 submitted 2011-09-23 astro-ph.SR gr-qcnucl-th

A.J. Penner , N. Andersson , D.I. Jones , L Samuelsson , I. Hawke This is my paper · ORCID
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keywords inspiralbinarycrustcrustalstrainastronomybeforecalculations
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We present the first fully relativistic calculations of the crustal strain induced in a neutron star by a binary companion at the late stages of inspiral, employing realistic equations of state for the fluid core and the solid crust. We show that while the deep crust is likely to fail only shortly before coalescence, there is a large variation in elastic strain, with the outermost layers failing relatively early on in the inspiral. We discuss the significance of the results for both electromagnetic and gravitational-wave astronomy.

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