@Article{Miranda_etal2020,
author="Miranda, O. G.
and Papoulias, D. K.
and Tortola, M.
and Valle, J. W. F.",
title="XENON1T signal from transition neutrino magnetic moments",
journal="Physics Letters B",
year="2020",
publisher="Elsevier",
volume="808",
pages="135685--5pp",
abstract="The recent puzzling results of the XENONIT collaboration at few keV electronic recoils could be due to the scattering of solar neutrinos endowed with finite Majorana transition magnetic moments (TMMs). Within such general formalism, we find that the observed excess in the XENONIT data agrees well with this interpretation. The required TMM strengths lie within the limits set by current experiments, such as Borexino, specially when one takes into account a possible tritium contamination.",
optnote="WOS:000571769700059",
optnote="exported from refbase (https://references.ific.uv.es/refbase/show.php?record=4541), last updated on Thu, 08 Oct 2020 08:40:40 +0000",
issn="0370-2693",
doi="10.1016/j.physletb.2020.135685",
opturl="https://arxiv.org/abs/2007.01765",
opturl="https://doi.org/10.1016/j.physletb.2020.135685",
language="English"
}