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Aspects of Axions and ALPs Phenomenology

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arxiv 2205.06831 v1 pith:EBIWILA4 submitted 2022-05-13 hep-ph astro-ph.COastro-ph.HEastro-ph.SR

classification hep-phastro-ph.COastro-ph.HEastro-ph.SR
keywords axionsexperimentalalpsaspectsphenomenologyproposalssomeadvances
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The physics of axions and axion-like particles (ALPs) is enjoying an incredibly productive period, with many new experimental proposals, theoretical idea, and original astrophysical and cosmological arguments which help the search effort. The large number of experimental proposals is likely to lead to fundamental advances (perhaps, a discovery?) in the coming years. The aim of this article is to provide a very brief overview of some of the recent developments in axions and ALP phenomenology, and to discuss some relevant aspects in this important field. A particular attention is given to the definition of motivated regions in the axion parameters space, which should be the targets of experimental searches.

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Cited by 1 Pith paper

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  1. Solar Axions from Nuclear Transitions

    hep-ph 2026-05 unverdicted novelty 3.0 of 10

    Solar axion fluxes from 57Fe and 83Kr nuclear transitions differ by three orders of magnitude, yielding stronger constraints on |g_aN^eff × g_aγγ| and g_aγγ vs. m_a from Chandrayaan-2 XSM data for iron.

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