Axion-like Particles Implications for High-Energy Astrophysics

被引：33

作者：

Galanti, Giorgio ^{[1
]}

Roncadelli, Marco ^{[2
,3
]}

机构：

[1] INAF, Ist Astrofis Spaziale & Fis Cosm Milano, Via A Corti 12, I-20133 Milan, Italy

[2] INFN, Sez Pavia, Via A Bassi 6, I-27100 Pavia, Italy

[3] INAF, Osservatorio Astron Brera, Via E Bianchi 46, I-23807 Merate, Italy

来源：

UNIVERSE | 2022年 / 8卷 / 05期

关键词：

particle physics; astroparticle physics; axion-like particles; photon polarization; blazars; galaxy clusters; extragalactic space; EXTRAGALACTIC BACKGROUND LIGHT; STRONG-CP PROBLEM; GAMMA-RAY SPECTRA; MAGNETIC-FIELDS; COSMIC FILAMENTS; MONTE-CARLO; SN; 1987A; PHOTON; CONSTRAINTS; CLUSTER;

D O I：

10.3390/universe8050253

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We offer a pedagogical introduction to axion-like particles (ALPs) as far as their relevance for high-energy astrophysics is concerned, from a few MeV to 1000 TeV. This review is self-contained, in such a way to be understandable even to non-specialists. Among other things, we discuss two strong hints at a specific ALP that emerge from two very different astrophysical situations. More technical matters are contained in three Appendices.

引用

页数：72

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