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• W2034683998 abstract "We show that the fundamental seismic shear mode, observed as a quasiperiodic oscillation in giant flares emitted by highly magnetized neutron stars, is particularly sensitive to the nuclear physics of the crust. The identification of an oscillation at $ensuremath{approx}30text{ }text{ }mathrm{Hz}$ as the fundamental crustal shear mode requires a nuclear symmetry energy that depends very weakly on density near saturation. If the nuclear symmetry energy varies more strongly with density, then lower frequency oscillations, previously identified as torsional Alfv'en modes of the fluid core, could instead be associated with the crust. If this is the case, then future observations of giant flares should detect oscillations at around 18 Hz. An accurate measurement of the neutron-skin thickness of lead will also constrain the frequencies predicted by the model." @default.
• W2034683998 created "2016-06-24" @default.
• W2034683998 creator A5037833302 @default.
• W2034683998 creator A5045387832 @default.
• W2034683998 date "2009-10-26" @default.
• W2034683998 modified "2023-10-17" @default.
• W2034683998 title "Constraints on Neutron Star Crusts from Oscillations in Giant Flares" @default.
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• W2034683998 doi "https://doi.org/10.1103/physrevlett.103.181101" @default.
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