Non-linear viscous damping and gravitational wave detectability of the f-mode instability in neutron stars
Version of Record online: 18 APR 2012
© 2012 The Authors Monthly Notices of the Royal Astronomical Society © 2012 RAS
Monthly Notices of the Royal Astronomical Society
Volume 422, Issue 4, pages 3327–3338, June 2012
How to Cite
Passamonti, A. and Glampedakis, K. (2012), Non-linear viscous damping and gravitational wave detectability of the f-mode instability in neutron stars. Monthly Notices of the Royal Astronomical Society, 422: 3327–3338. doi: 10.1111/j.1365-2966.2012.20849.x
- Issue online: 21 MAY 2012
- Version of Record online: 18 APR 2012
- Accepted 2012 February 29. Received 2012 February 16; in original form 2011 December 16
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