Chameleon-neutrino conformal coupling and MSW-mediated solar neutrino deficit

A modified version of the MSW effect is studied within the framework of screening models through conformal couplings of a scalar field within matter. Such a coupling leads to a new, unknown interaction between the scalar field and the neutrino. We mainly look for the discrepancy in the total solar e...

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Main Authors: H. Yazdani Ahmadabadi, H. Mohseni Sadjadi
Format: Article
Language:English
Published: Elsevier 2024-03-01
Series:Physics Letters B
Online Access:http://www.sciencedirect.com/science/article/pii/S0370269324000510
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author H. Yazdani Ahmadabadi
H. Mohseni Sadjadi
author_facet H. Yazdani Ahmadabadi
H. Mohseni Sadjadi
author_sort H. Yazdani Ahmadabadi
collection DOAJ
description A modified version of the MSW effect is studied within the framework of screening models through conformal couplings of a scalar field within matter. Such a coupling leads to a new, unknown interaction between the scalar field and the neutrino. We mainly look for the discrepancy in the total solar electron-neutrinos flux through this interaction. Since the scalar field behavior depends on the local density of matter, we observe an indirect effect of matter on flavor changes, and subsequently, on neutrino flux through neutrino decay. The paper ends by describing various probabilities and comparing the results with observational data.
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spelling doaj.art-c872cdb1e5a248b79126e7aada1d5bf02024-03-14T06:13:12ZengElsevierPhysics Letters B0370-26932024-03-01850138493Chameleon-neutrino conformal coupling and MSW-mediated solar neutrino deficitH. Yazdani Ahmadabadi0H. Mohseni Sadjadi1Department of Physics, University of Tehran, P. O. B. 14395-547, Tehran 14399-55961, IranCorresponding author.; Department of Physics, University of Tehran, P. O. B. 14395-547, Tehran 14399-55961, IranA modified version of the MSW effect is studied within the framework of screening models through conformal couplings of a scalar field within matter. Such a coupling leads to a new, unknown interaction between the scalar field and the neutrino. We mainly look for the discrepancy in the total solar electron-neutrinos flux through this interaction. Since the scalar field behavior depends on the local density of matter, we observe an indirect effect of matter on flavor changes, and subsequently, on neutrino flux through neutrino decay. The paper ends by describing various probabilities and comparing the results with observational data.http://www.sciencedirect.com/science/article/pii/S0370269324000510
spellingShingle H. Yazdani Ahmadabadi
H. Mohseni Sadjadi
Chameleon-neutrino conformal coupling and MSW-mediated solar neutrino deficit
Physics Letters B
title Chameleon-neutrino conformal coupling and MSW-mediated solar neutrino deficit
title_full Chameleon-neutrino conformal coupling and MSW-mediated solar neutrino deficit
title_fullStr Chameleon-neutrino conformal coupling and MSW-mediated solar neutrino deficit
title_full_unstemmed Chameleon-neutrino conformal coupling and MSW-mediated solar neutrino deficit
title_short Chameleon-neutrino conformal coupling and MSW-mediated solar neutrino deficit
title_sort chameleon neutrino conformal coupling and msw mediated solar neutrino deficit
url http://www.sciencedirect.com/science/article/pii/S0370269324000510
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