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: | English |
| Published: |
IOP Publishing,
2017-04-20T20:20:02Z.
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| Online Access: | Get fulltext |