GROWTH RATE OF THE TIDAL p-MODE g-MODE INSTABILITY IN COALESCING BINARY NEUTRON STARS
We recently described an instability due to the nonlinear coupling of p-modes to g-modes and, as an application, we studied the stability of the tide in coalescing binary neutron stars. Although we found that the tide is p–g unstable early in the inspiral and rapidly drives modes to large energies,...
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| Format: | Article |
| Language: | en_US |
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IOP Publishing
2017
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| Online Access: | http://hdl.handle.net/1721.1/108320 https://orcid.org/0000-0001-9194-2084 |