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Gravitational waves from neutron stars

Published online by Cambridge University Press:  21 October 2010

Nils Andersson*
Affiliation:
School of Mathematics, University of Southampton, Southampton SO17 1BJ, UK email: [email protected]
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Abstract

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In this presentation, I will outline some of the different ways that neutron stars can generate gravitational waves, discuss recent improvements in modeling the relevant scenarios in the context of improving detector sensitivity, and show how observations are beginning to put interesting “constraints” on our theoretical models.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2010

References

Abbott, B. P., et al. 2009, Rep. Prog. Phys. 72, 076901Google Scholar
Andersson, N. 2003, Class. Quantum Grav. 20, R105Google Scholar
Haskell, B. 2008, Class. Quantum Grav. 25, 114049Google Scholar
Sathyaprakash, B. S. & Schutz, B. F. 2009, Liv. Rev. Relativity, vol. 12, no. 2Google Scholar
Watts, A. L. & Krishnan, B. 2009 Adv. Sp. Res. 43, 1049Google Scholar