Imprints of vector field non-standard couplings on solar neutrino flux

Fuente: arXiv
Enregistré dans:
Détails bibliographiques
Auteurs principaux: Ahmadabadi, H. Yazdani, Sadjadi, H. Mohseni
Format: Preprint
Publié: 2022
Sujets:
Accès en ligne:
Tags: Ajouter un tag
Pas de tags, Soyez le premier à ajouter un tag!
_version_ 1866915022401175552
author Ahmadabadi, H. Yazdani
Sadjadi, H. Mohseni
author_facet Ahmadabadi, H. Yazdani
Sadjadi, H. Mohseni
contents Regarding the proximity of dark energy scale and neutrino mass, one can get new insight into the probe signatures of vector field dark energy component on neutrino flavor conversion. A vector field is assumed to be conformally coupled to various matter components through a screening paradigm. We show how the oscillation probabilities evolve differently with a finite-size matter density like the Sun for different values of relevant model parameters. Considering existing neutrino flavor conversion data, we point out how this non-standard coupling affects neutrino fluxes and also we compute the discrepancy in the total flux of solar electron-neutrinos.
format Preprint
id arxiv_https___arxiv_org_abs_2209_13367
institution arXiv
publishDate 2022
record_format arxiv
spellingShingle Imprints of vector field non-standard couplings on solar neutrino flux
Ahmadabadi, H. Yazdani
Sadjadi, H. Mohseni
High Energy Physics - Phenomenology
General Relativity and Quantum Cosmology
High Energy Physics - Theory
Regarding the proximity of dark energy scale and neutrino mass, one can get new insight into the probe signatures of vector field dark energy component on neutrino flavor conversion. A vector field is assumed to be conformally coupled to various matter components through a screening paradigm. We show how the oscillation probabilities evolve differently with a finite-size matter density like the Sun for different values of relevant model parameters. Considering existing neutrino flavor conversion data, we point out how this non-standard coupling affects neutrino fluxes and also we compute the discrepancy in the total flux of solar electron-neutrinos.
title Imprints of vector field non-standard couplings on solar neutrino flux
topic High Energy Physics - Phenomenology
General Relativity and Quantum Cosmology
High Energy Physics - Theory
url https://arxiv.org/abs/2209.13367