Continuous self-similar collapse solutions exist for a scale-invariant elastic matter model, and regularity imposes bounds on the elasticity parameters.
Crustal failure during binary inspiral
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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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Self-similar collapse with elasticity
Continuous self-similar collapse solutions exist for a scale-invariant elastic matter model, and regularity imposes bounds on the elasticity parameters.