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- W4283705631 abstract "Tidal effects in gravitational-wave (GW) observations from binary neutron star mergers have the potential to probe ultradense matter and shed light on the unknown nuclear equation of state of neutron stars. Tidal effects in inspiralling neutron star binaries become relevant at GW frequencies of a few hundred Hz and require detectors with exquisite high-frequency sensitivity. Third generation GW detectors such as the Einstein Telescope or Cosmic Explorer will be particularly sensitive in this high-frequency regime, allowing us to probe neutron star tides beyond the adiabatic approximation. Here we assess whether dynamical tides can be measured from a neutron star inspiral. We find that the measurability of dynamical tides depends strongly on the neutron star mass and equation of state. For a semirealistic population of 10,000 inspiralling binary neutron stars, we conservatively estimate that on average $mathcal{O}(50)$ binaries will have measurable dynamical tides. As dynamical tides are characterized not only by the star's tidal deformability but also by its fundamental ($f$-) mode frequency, they present a possibility of probing higher-order tidal effects and test consistency with quasiuniversal relations. For a GW170817-like signal in a third generation detector network, we find that the stars' $f$-mode frequencies can be measured to within a few hundred Hz." @default.
- W4283705631 created "2022-06-30" @default.
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- W4283705631 date "2022-06-28" @default.
- W4283705631 modified "2023-10-15" @default.
- W4283705631 title "Prospects for distinguishing dynamical tides in inspiralling binary neutron stars with third generation gravitational-wave detectors" @default.
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- W4283705631 doi "https://doi.org/10.1103/physrevd.105.123032" @default.
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