Maximum latent heat of neutron star matter independent of general relativity

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Lope Oter, Eva and Llanes Estrada, Felipe José (2022) Maximum latent heat of neutron star matter independent of general relativity. Physical review C, 105 (5). ISSN 2469-9985

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Official URL: http://dx.doi.org/10.1103/PhysRevC.105.L052801




Abstract

We establish bounds on the maximum possible specific latent heat of cold neutron-star matter derived from hadron physics alone. Existing chiral perturbation theory computations for the equation of state, together with perturbative quantum chromodynamics (QCD), relevant at highest densities (even if they would turn out not to be physically realizable) bind the maximum latent heat which is possible in actual neutron stars. Because these are already near gravitational collapse in general relativity, no denser form of cold matter can exist: thus, the bounds are a generic physical limit. Even in scenarios that modify the theory of gravity, the existence of a family of latent-heat maxima is relevant to diagnose progress in the knowledge of the equation of state of neutron matter, by quantifying the maximum possible (presumed) phase transition that its error bands would allow. Thus, latent heat is a natural benchmark for the equation of state in cold QCD.


Item Type:Article
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©2022 American Physical Society
Supported by Grants No. MICINN: PID2019-108655GB-I00 and No. PID2019-106080GB-C21 (Spain); the COST action CA16214 (Multimessenger Physics and Astrophysics of Neutron Stars); Universidad Complutense de Madrid under research Group No. 910309 and the IPARCOS institute.

Uncontrolled Keywords:Superconductivity
Subjects:Sciences > Physics
ID Code:73085
Deposited On:11 Jul 2022 17:03
Last Modified:02 Aug 2022 08:29

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