Imprints of vector field non-standard couplings on solar neutrino flux
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 sho...
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| Format: | Article |
| Language: | English |
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Elsevier
2024-12-01
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| Series: | Physics Letters B |
| Online Access: | http://www.sciencedirect.com/science/article/pii/S0370269324006683 |
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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 | 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 | Article |
| id | doaj-art-93292b013b0640ee9affc020706445eb |
| institution | DOAJ |
| issn | 0370-2693 |
| language | English |
| publishDate | 2024-12-01 |
| publisher | Elsevier |
| record_format | Article |
| series | Physics Letters B |
| spelling | doaj-art-93292b013b0640ee9affc020706445eb2025-08-20T02:48:58ZengElsevierPhysics Letters B0370-26932024-12-0185913911010.1016/j.physletb.2024.139110Imprints of vector field non-standard couplings on solar neutrino fluxH. 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, IranRegarding 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.http://www.sciencedirect.com/science/article/pii/S0370269324006683 |
| spellingShingle | H. Yazdani Ahmadabadi H. Mohseni Sadjadi Imprints of vector field non-standard couplings on solar neutrino flux Physics Letters B |
| title | Imprints of vector field non-standard couplings on solar neutrino flux |
| title_full | Imprints of vector field non-standard couplings on solar neutrino flux |
| title_fullStr | Imprints of vector field non-standard couplings on solar neutrino flux |
| title_full_unstemmed | Imprints of vector field non-standard couplings on solar neutrino flux |
| title_short | Imprints of vector field non-standard couplings on solar neutrino flux |
| title_sort | imprints of vector field non standard couplings on solar neutrino flux |
| url | http://www.sciencedirect.com/science/article/pii/S0370269324006683 |
| work_keys_str_mv | AT hyazdaniahmadabadi imprintsofvectorfieldnonstandardcouplingsonsolarneutrinoflux AT hmohsenisadjadi imprintsofvectorfieldnonstandardcouplingsonsolarneutrinoflux |