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Potential of SKA to Detect CDM ALPs with Radio Astronomy

2020/07/24 by Ahmed Ayad, Ayad, Ahmed, Geoff Beck +1
Physics and Astronomy · #FOS: Physical sciences #High Energy Astrophysical Phenomena (astro-ph.HE) #High Energy Physics - Phenomenology (hep-ph) #astro-ph.HE #hep-ph

paper · pdf · doi:10.48550/arxiv.2007.14262

This work is a proceeding submitted to the International Conference on Neutrinos and Dark Matter (NDM)-2020

arxiv created 2020/07/24 · arxiv updated 2020/07/29

Abstract

Axion-like particles (ALPs) are light pseudo-scalar particles predicted in many theoretically well-motivated extensions to the standard model of particle physics (SM). The search for cold dark matter (CDM) ALPs has gained tremendous ground over the last few years. Essentially ALPs are characterized by their coupling with two photons which allows ALPs to decay into two photons. In this work, we explore the potential of the Square Kilometer Array (SKA) to detect CDM ALPs with radio astronomy in an attempt to detect an observational signature of ALPs conversion onto photons in astrophysical field.

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