Solar Neutrinos and the Strongest Oscillation Constraints on Scalar NSI

Fuente: arXiv
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Main Authors: Denton, Peter B., Giarnetti, Alessio, Meloni, Davide
Format: Preprint
Published: 2024
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author Denton, Peter B.
Giarnetti, Alessio
Meloni, Davide
author_facet Denton, Peter B.
Giarnetti, Alessio
Meloni, Davide
contents Scalar non-standard neutrino interactions (sNSI) is a scenario where neutrinos can develop a medium dependent contribution to their mass due to a new scalar mediator. This scenario differs from the commonly discussed vector mediator case in that the oscillation effect scales with density rather than density and neutrino energy. Thus the strongest oscillation constraint comes from solar neutrinos which experience the largest density in a neutrino oscillation experiment. We derive constraints on all the sNSI parameters as well as the absolute neutrino mass scale by combining solar and reactor data and find solar neutrinos to be $>1$ order of magnitude more sensitive to sNSI than terrestrial probes such as long-baseline experiments.
format Preprint
id arxiv_https___arxiv_org_abs_2409_15411
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Solar Neutrinos and the Strongest Oscillation Constraints on Scalar NSI
Denton, Peter B.
Giarnetti, Alessio
Meloni, Davide
High Energy Physics - Phenomenology
High Energy Physics - Experiment
Scalar non-standard neutrino interactions (sNSI) is a scenario where neutrinos can develop a medium dependent contribution to their mass due to a new scalar mediator. This scenario differs from the commonly discussed vector mediator case in that the oscillation effect scales with density rather than density and neutrino energy. Thus the strongest oscillation constraint comes from solar neutrinos which experience the largest density in a neutrino oscillation experiment. We derive constraints on all the sNSI parameters as well as the absolute neutrino mass scale by combining solar and reactor data and find solar neutrinos to be $>1$ order of magnitude more sensitive to sNSI than terrestrial probes such as long-baseline experiments.
title Solar Neutrinos and the Strongest Oscillation Constraints on Scalar NSI
topic High Energy Physics - Phenomenology
High Energy Physics - Experiment
url https://arxiv.org/abs/2409.15411