Axion Astrophysics

Fuente: arXiv
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Autori principali: Carenza, Pierluca, Giannotti, Maurizio, Isern, Jordi, Mirizzi, Alessandro, Straniero, Oscar
Natura: Preprint
Pubblicazione: 2024
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author Carenza, Pierluca
Giannotti, Maurizio
Isern, Jordi
Mirizzi, Alessandro
Straniero, Oscar
author_facet Carenza, Pierluca
Giannotti, Maurizio
Isern, Jordi
Mirizzi, Alessandro
Straniero, Oscar
contents Stars have been recognized as optimal laboratories to probe axion properties. In the last decades there have been significant advances in this field due to a better modelling of stellar systems and accurate observational data. In this work we review the current status of constraints on axions from stellar physics. We focus in particular on the Sun, globular cluster stars, white dwarfs and (proto)-neutron stars.
format Preprint
id arxiv_https___arxiv_org_abs_2411_02492
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Axion Astrophysics
Carenza, Pierluca
Giannotti, Maurizio
Isern, Jordi
Mirizzi, Alessandro
Straniero, Oscar
High Energy Physics - Phenomenology
Solar and Stellar Astrophysics
High Energy Physics - Experiment
High Energy Physics - Theory
Stars have been recognized as optimal laboratories to probe axion properties. In the last decades there have been significant advances in this field due to a better modelling of stellar systems and accurate observational data. In this work we review the current status of constraints on axions from stellar physics. We focus in particular on the Sun, globular cluster stars, white dwarfs and (proto)-neutron stars.
title Axion Astrophysics
topic High Energy Physics - Phenomenology
Solar and Stellar Astrophysics
High Energy Physics - Experiment
High Energy Physics - Theory
url https://arxiv.org/abs/2411.02492