TY  - JOUR
AU  - Miranda, O. G.
AU  - Papoulias, D. K.
AU  - Tortola, M.
AU  - Valle, J. W. F.
PY  - 2020
DA  - 2020//
TI  - XENON1T signal from transition neutrino magnetic moments
T2  - Phys. Lett. B
JO  - Physics Letters B
SP  - 135685
EP  - 5pp
VL  - 808
PB  - Elsevier
AB  - 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.
SN  - 0370-2693
UR  - https://arxiv.org/abs/2007.01765
UR  - https://doi.org/10.1016/j.physletb.2020.135685
DO  - 10.1016/j.physletb.2020.135685
LA  - English
N1  - WOS:000571769700059
ID  - Miranda_etal2020
ER  -