The Sun as a target for axion dark matter detection

被引：0

作者：

Todarello, Elisa ^{[1
,2
]}

Regis, Marco ^{[1
,2
]}

Taoso, Marco ^{[2
]}

Giannotti, Maurizio ^{[3
]}

Ruz, Jaime ^{[3
]}

Vogel, Julia K. ^{[3
]}

机构：

[1] Univ Torino, Dipartimento Fis, Via P Giuria 1, I-10125 Turin, Italy

[2] Ist Nazl Fis Nucl, Sez Torino, Via P Giuria 1, I-10125 Turin, Italy

[3] Univ Zaragoza, Ctr Astroparticulas & Fis Altas Energias CAPA, Zaragoza 50009, Spain

来源：

PHYSICS LETTERS B | 2024年 / 854卷

关键词：

RADIO-EMISSION; CONSTRAINTS; CONVERSION; COSMOLOGY;

D O I：

10.1016/j.physletb.2024.138752

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The exploration of the parameter space of axion and axion-like particle dark matter is a major aim of the future program of astroparticle physics investigations. In this context, we present a possible strategy that focuses on detecting radio emissions arising from the conversion of dark matter axions in the Sun's magnetic field, including conversion in sunspots. We demonstrate that near-future low-frequency radio telescopes, such as the SKA Low, may access regions of unexplored parameter space for masses m a S 10 -6 eV.

引用

页数：5

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