arXiv · 2007.06579
Cosmic Imprints of XENON1T Axions
Abstract
The recent electron recoil excess observed by XENON1T has a possible interpretation in terms of solar axions coupled to electrons. If such axions are still relativistic at recombination they would also leave a cosmic imprint in the form of an additional radiation component, parameterized by an effective neutrino number $\Delta N_\text{eff}$. We explore minimal scenarios with a detectable signal in future CMB surveys: axions coupled democratically to all fermions, axion-electron coupling generated radiatively, the DFSZ framework for the QCD axion. The predicted $\Delta N_\text{eff}$ is larger than $0.03-0.04$ for all cases, close to the $2\sigma$ forecasted sensitivity of CMB-S4 experiments. This opens the possibility of testing with cosmological observations the solar axion interpretation of the XENON1T excess.
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Fernando Arias-Aragon, Francesco D'Eramo, Ricardo Z. Ferreira, Luca Merlo, Alessio Notari. 2020-07-13. Cosmic Imprints of XENON1T Axions. https://doi.org/10.1088/1475-7516/2020/11/025
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