Effects of Neutron-Star Dynamic Tides on Gravitational Waveforms within the Effective-One-Body Approach.

@article{Hinderer2016EffectsON,
  title={Effects of Neutron-Star Dynamic Tides on Gravitational Waveforms within the Effective-One-Body Approach.},
  author={Tanja Hinderer and Andrea Taracchini and Francois Foucart and Alessandra Buonanno and Jan Steinhoff and Matthew D Duez and Lawrence E. Kidder and Harald P. Pfeiffer and Mark A. Scheel and B{\'e}la Szil{\'a}gyi and Kenta Hotokezaka and Koutarou Kyutoku and Masaru Shibata and Cory W Carpenter},
  journal={Physical review letters},
  year={2016},
  volume={116 18},
  pages={
          181101
        }
}
Extracting the unique information on ultradense nuclear matter from the gravitational waves emitted by merging neutron-star binaries requires robust theoretical models of the signal. We develop a novel effective-one-body waveform model that includes, for the first time, dynamic (instead of only adiabatic) tides of the neutron star as well as the merger signal for neutron-star-black-hole binaries. We demonstrate the importance of the dynamic tides by comparing our model against new numerical… 

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