Probing fundamental physics using compact astrophysical objects

Fuente: arXiv
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Hauptverfasser: Kolonia, E. -A., Martins, C. J. A. P., Gourgouliatos, Konstantinos N.
Format: Preprint
Veröffentlicht: 2025
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author Kolonia, E. -A.
Martins, C. J. A. P.
Gourgouliatos, Konstantinos N.
author_facet Kolonia, E. -A.
Martins, C. J. A. P.
Gourgouliatos, Konstantinos N.
contents It is well known that alternative theories to the Standard Model allow -- and sometimes require -- fundamental constants, such as the fine-structure constant, $α$, to vary in spacetime. We demonstrate that one way to investigate these variations is through the Mass-Radius relation of compact astrophysical objects, which is inherently affected by $α$ variations. We start by considering the model of a polytropic white dwarf, which we perturb by adding the $α$ variations for a generic class of Grand Unified Theories. We then extend our analysis to neutron stars, building upon the polytropic approach to consider more realistic equations of state, discussing the impact of such variations on mass-radius measurements in neutron stars. We present some constraints on these models based on current data and also outline how future observations might distinguish between extensions of the Standard Model.
format Preprint
id arxiv_https___arxiv_org_abs_2503_11447
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Probing fundamental physics using compact astrophysical objects
Kolonia, E. -A.
Martins, C. J. A. P.
Gourgouliatos, Konstantinos N.
High Energy Physics - Phenomenology
High Energy Astrophysical Phenomena
General Relativity and Quantum Cosmology
It is well known that alternative theories to the Standard Model allow -- and sometimes require -- fundamental constants, such as the fine-structure constant, $α$, to vary in spacetime. We demonstrate that one way to investigate these variations is through the Mass-Radius relation of compact astrophysical objects, which is inherently affected by $α$ variations. We start by considering the model of a polytropic white dwarf, which we perturb by adding the $α$ variations for a generic class of Grand Unified Theories. We then extend our analysis to neutron stars, building upon the polytropic approach to consider more realistic equations of state, discussing the impact of such variations on mass-radius measurements in neutron stars. We present some constraints on these models based on current data and also outline how future observations might distinguish between extensions of the Standard Model.
title Probing fundamental physics using compact astrophysical objects
topic High Energy Physics - Phenomenology
High Energy Astrophysical Phenomena
General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2503.11447