Resonant tidal excitation of superfluid neutron stars in coalescing binaries

Resonant tidal excitation of superfluid neutron stars in coalescing binaries

We study the resonant tidal excitation of g modes in coalescing superfluid neutron star (NS) binaries and investigate how such tidal driving impacts the gravitational-wave (GW) signal of the inspiral. Previous studies of this type treated the NS core as a normal fluid and thus did not account for it...

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Bibliographic Details
Main Authors: Weinberg, Nevin N. (Author), Yu, Hang,Ph. D.Massachusetts Institute of Technology (Author)
Other Authors: Massachusetts Institute of Technology. Department of Physics (Contributor), MIT Kavli Institute for Astrophysics and Space Research (Contributor), LIGO (Observatory : Massachusetts Institute of Technology) (Contributor)
Format: Article
Language:English
Published: Oxford University Press (OUP), 2019-06-21T19:45:55Z.
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