Constraining the p-Mode–g-Mode Tidal Instability with GW170817

Constraining the p-Mode–g-Mode Tidal Instability with GW170817

We analyze the impact of a proposed tidal instability coupling p modes and g modes within neutron stars on GW170817. This nonresonant instability transfers energy from the orbit of the binary to internal modes of the stars, accelerating the gravitational-wave driven inspiral. We model the impact of...

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Bibliographic Details
Other Authors:	Massachusetts Institute of Technology. Department of Physics
Format:	Article
Published:	American Physical Society 2020
Online Access:	https://hdl.handle.net/1721.1/124453

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