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Crustal failure during binary inspiral
Umeå University, Faculty of Science and Technology, Department of Physics.
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2012 (English)In: Astrophysical journal letters, ISSN 2041-8205, Vol. 749, no 2, L36- p.Article in journal (Refereed) Published
Abstract [en]

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.

Place, publisher, year, edition, pages
2012. Vol. 749, no 2, L36- p.
Keyword [en]
dense matter, gravitational waves, stars: neutron
National Category
Astronomy, Astrophysics and Cosmology
Identifiers
URN: urn:nbn:se:umu:diva-55019DOI: 10.1088/2041-8205/749/2/L36ISI: 000302638300020OAI: oai:DiVA.org:umu-55019DiVA: diva2:525789
Available from: 2012-05-09 Created: 2012-05-07 Last updated: 2012-05-09Bibliographically approved

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