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Neutron star seismology

Published online by Cambridge University Press:  20 March 2013

Nils Andersson
Nils Andersson*
Affiliation:
University of Southampton, United Kingdom email: [email protected]
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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.

Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S291: Neutron Stars and Pulsars: Challenges and Opportunities after 80 years , August 2012 , pp. 159
Copyright
Copyright © International Astronomical Union 2013