Impact of the tidal p−g instability on the gravitational wave signal from coalescing binary neutron stars
Recent studies suggest that coalescing neutron stars are subject to a fluid instability involving the nonlinear coupling of the tide to p modes and g modes. Its influence on the inspiral dynamics and thus the gravitational wave signal is, however, uncertain because we do not know precisely how the i...
| Main Authors: | , , |
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| Other Authors: | , , |
| Format: | Article |
| Language: | English |
| Published: |
American Physical Society,
2017-01-05T19:07:06Z.
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| Subjects: | |
| Online Access: | Get fulltext |