Thermal effects on tidal deformability of a coalescing binary neutron star system
A. Kanakis-Pegios, P.S. Koliogiannis, Ch.C. Moustakidis

TL;DR
This paper investigates how temperature influences the tidal deformability of neutron stars during inspiral, finding that even at low temperatures, the effects are minimal and indistinguishable, impacting gravitational wave analysis.
Contribution
The study applies hot equations of state from various nuclear models to assess temperature effects on tidal deformability, revealing negligible impact at low temperatures.
Findings
Temperature effects are minimal at T<1 MeV
Tidal deformability differences are indistinguishable with temperature
Implications for gravitational wave data analysis
Abstract
The study of neutron star mergers by the detection of the emitted gravitational waves is one of the most promised tools to study the properties of dense nuclear matter at high densities. It is worth claiming that, at the moment, strong evidence that the temperature of the stars is zero during the last orbits before coalescing does not exist. Contrariwise, there are some theoretical predictions suggesting that the star's temperature might even be a few MeV. According to the main theory, the tides transfer mechanical energy and angular momentum to the star at the expense of the orbit, where friction within the star converts the mechanical energy into heat. During the inspiral these effects are potentially detectable. Different treatments have been used to estimate the transfer of the mechanical energy and the size of the tidal friction, leading to different conclusions about the…
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Taxonomy
TopicsPulsars and Gravitational Waves Research · Gamma-ray bursts and supernovae · Astro and Planetary Science
