Effective Field Theories for Neutron Stars Physics

Fuente: arXiv
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Main Authors: Alarcón, J. M., Lope-Oter, E., Cano, Y.
Format: Preprint
Published: 2025
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author Alarcón, J. M.
Lope-Oter, E.
Cano, Y.
author_facet Alarcón, J. M.
Lope-Oter, E.
Cano, Y.
contents There is an increasing interest in the community for the Neutron Stars and what we can learn from them. In this review we show how chiral effective field theory, combined with many-body methods, can provide important results that connect Neutron Star properties at zero temperature to nuclear physics and allows to use these compact objects as laboratories of new physics.
format Preprint
id arxiv_https___arxiv_org_abs_2511_04737
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Effective Field Theories for Neutron Stars Physics
Alarcón, J. M.
Lope-Oter, E.
Cano, Y.
High Energy Physics - Phenomenology
High Energy Astrophysical Phenomena
Nuclear Theory
There is an increasing interest in the community for the Neutron Stars and what we can learn from them. In this review we show how chiral effective field theory, combined with many-body methods, can provide important results that connect Neutron Star properties at zero temperature to nuclear physics and allows to use these compact objects as laboratories of new physics.
title Effective Field Theories for Neutron Stars Physics
topic High Energy Physics - Phenomenology
High Energy Astrophysical Phenomena
Nuclear Theory
url https://arxiv.org/abs/2511.04737