PreprintarXiv licencearXiv
XENONnT pp-Dominated Solar Neutrinos Constrain the ν1 Pseudo-Dirac Splitting
Abstract
XENONnT has measured a low-energy solar-neutrino signal dominated by pp neutrinos. At these energies, an ultra-small pseudo-Dirac mass-squared splitting induces detectable active-sterile oscillations over the Sun--Earth baseline. We study pseudo-Dirac oscillations of the first mass eigenstate, compute the resulting modification of the pp+7Be electron-recoil spectrum, and construct a likelihood from the published XENONnT energy spectra. We find that the XENONnT data exclude 5.9×10−13 eV2≲ δm12 ≤ 10−11 eV2 at the 2σ level, extending current solar-neutrino sensitivity to smaller mass splittings and approaching a regime previously discussed for future pp-sensitive detectors.
Related
- Testing the Pseudo-Dirac Nature of Atmospheric Neutrinos
- Search for Magnetic and Spin-Independent Inelastic Dark Matter with XENONnT
- Neutrino electromagnetic properties after the first pp solar neutrino observation at XENONnT
- Direct detection of solar chameleons with electron recoil data from XENONnT
- Probing Solar Chameleons with XENONnT Ionization-Only Data
BibTeX
@misc{leone2026xenonnt,
title = {{XENONnT $pp$-Dominated Solar Neutrinos Constrain the $ν_1$ Pseudo-Dirac Splitting}},
author = {Gio Leone},
howpublished = {arXiv},
year = {2026},
month = oct,
doi = {10.48550/arxiv.2609.38233},
eprint = {2609.38233},
archivePrefix = {arXiv},
url = {https://arxiv.org/abs/2609.38233},
}
RIS
TY - UNPB
TI - XENONnT pp-Dominated Solar Neutrinos Constrain the ν_1 Pseudo-Dirac Splitting
AU - Gio Leone
PY - 2026
DA - 2026/10/01
PB - arXiv
DO - 10.48550/arxiv.2609.38233
UR - https://arxiv.org/abs/2609.38233
AB - XENONnT has measured a low-energy solar-neutrino signal dominated by pp neutrinos. At these energies, an ultra-small pseudo-Dirac mass-squared splitting induces detectable active-sterile oscillations over the Sun--Earth baseline. We study pseudo-Dirac oscillations of the first mass eigenstate, compute the resulting modification of the pp+^7Be electron-recoil spectrum, and construct a likelihood from the published XENONnT energy spectra. We find that the XENONnT data exclude 5.9×10^−13 eV^2≲ δm_1^2 ≤ 10^−11 eV^2 at the 2σ level, extending current solar-neutrino sensitivity to smaller mass splittings and approaching a regime previously discussed for future pp-sensitive detectors.
ER -