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Neutron star seismology
Published online by Cambridge University Press: 20 March 2013
Abstract
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I will provide an overview of recent improvements in our models for vibrating neutron stars, discussing the role of composition, heat, crust elasticity and superfluidity. I will explain how the results may impact on observations, in particular related to magnetar QPOs and future gravitational-wave searches.
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- Copyright © International Astronomical Union 2013
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