Axion astrophysics

IF 29.5 1区物理与天体物理 Q1 PHYSICS, MULTIDISCIPLINARY Physics Reports Pub Date : 2025-02-26 DOI:10.1016/j.physrep.2025.02.002

Pierluca Carenza , Maurizio Giannotti , Jordi Isern , Alessandro Mirizzi , Oscar Straniero

引用次数: 0

Abstract

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 modeling 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.

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Axion天体物理学

恒星被认为是探测轴子性质的最佳实验室。在过去的几十年里，由于更好的恒星系统建模和准确的观测数据，这一领域取得了重大进展。在这项工作中，我们回顾了从恒星物理学中对轴子的约束的现状。我们特别关注太阳、球状星团恒星、白矮星和（原）中子星。

本文章由计算机程序翻译，如有差异，请以英文原文为准。

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来源期刊

Physics Reports 物理-物理：综合

CiteScore

56.10

自引率

0.70%

发文量

102

审稿时长

9.1 weeks

期刊介绍： Physics Reports keeps the active physicist up-to-date on developments in a wide range of topics by publishing timely reviews which are more extensive than just literature surveys but normally less than a full monograph. Each report deals with one specific subject and is generally published in a separate volume. These reviews are specialist in nature but contain enough introductory material to make the main points intelligible to a non-specialist. The reader will not only be able to distinguish important developments and trends in physics but will also find a sufficient number of references to the original literature.

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