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arXiv · 2203.09145

Effects of dense matter on the tidal deformations of binary neutron star inspirals and gravitational waves

Loïc Perot·Nicolas Chamel
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Abstract

The role of the dense matter properties on the tidal deformability and gravitational waveforms of binary neutron stars is studied using a set of unified equations of state. Based on the nuclear energy-density functional theory, these equations of state provide a thermodynamically consistent treatment of all regions of the stars and were calculated using functionals that were precision fitted to experimental and theoretical nuclear data.

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Loïc Perot, Nicolas Chamel. 2022-03-17. Effects of dense matter on the tidal deformations of binary neutron star inspirals and gravitational waves. https://arxiv.org/abs/2203.09145

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