Implications of the Dark-LMA solution for neutrino mass matrices
In this work we have re-investigated two different kinds of texture zero ansatz of the low energy neutrino mass matrix in view of the Dark-Large-Mixing-Angle (DLMA) solution of the solar neutrino problem which can arise in the presence of non-standard interactions. In particular we revisit the cases...
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doaj-8a0ea7ff585645bea6418d6a063e1efc2021-07-25T04:41:36ZengElsevierNuclear Physics B0550-32132021-08-01969115460Implications of the Dark-LMA solution for neutrino mass matricesMonojit Ghosh0Srubabati Goswami1Ananya Mukherjee2Department of Physics, School of Engineering Sciences, KTH Royal Institute of Technology, AlbaNova University Center, Roslagstullsbacken 21, SE–106 91 Stockholm, Sweden; The Oskar Klein Centre for Cosmoparticle Physics, AlbaNova University Center, Roslagstullsbacken 21, SE–106 91 Stockholm, Sweden; Center of Excellence for Advanced Materials and Sensing Devices, Ruder Bošković Institute, 10000 Zagreb, CroatiaPhysical Research Laboratory, Ahmedabad, 380009, IndiaPhysical Research Laboratory, Ahmedabad, 380009, India; Corresponding author.In this work we have re-investigated two different kinds of texture zero ansatz of the low energy neutrino mass matrix in view of the Dark-Large-Mixing-Angle (DLMA) solution of the solar neutrino problem which can arise in the presence of non-standard interactions. In particular we revisit the cases of (i) one zero mass matrices when the lowest neutrino mass is zero and (ii) one zero texture with a vanishing minor. In our study we find that for most of the cases, the texture zero conditions which are allowed for the LMA solution, are also allowed for the DLMA solution. However, we found two textures belonging to the case of one zero texture with a vanishing minor where LMA solution does not give a viable solution whereas DLMA solution does. We analyze all the possible texture zero cases belonging to these two kinds of texture zero structures in detail and present correlations between different parameters. We also present the predictions for the effective neutrino mass governing neutrino-less double beta decay for the allowed textures.http://www.sciencedirect.com/science/article/pii/S0550321321001577 |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
Monojit Ghosh Srubabati Goswami Ananya Mukherjee |
spellingShingle |
Monojit Ghosh Srubabati Goswami Ananya Mukherjee Implications of the Dark-LMA solution for neutrino mass matrices Nuclear Physics B |
author_facet |
Monojit Ghosh Srubabati Goswami Ananya Mukherjee |
author_sort |
Monojit Ghosh |
title |
Implications of the Dark-LMA solution for neutrino mass matrices |
title_short |
Implications of the Dark-LMA solution for neutrino mass matrices |
title_full |
Implications of the Dark-LMA solution for neutrino mass matrices |
title_fullStr |
Implications of the Dark-LMA solution for neutrino mass matrices |
title_full_unstemmed |
Implications of the Dark-LMA solution for neutrino mass matrices |
title_sort |
implications of the dark-lma solution for neutrino mass matrices |
publisher |
Elsevier |
series |
Nuclear Physics B |
issn |
0550-3213 |
publishDate |
2021-08-01 |
description |
In this work we have re-investigated two different kinds of texture zero ansatz of the low energy neutrino mass matrix in view of the Dark-Large-Mixing-Angle (DLMA) solution of the solar neutrino problem which can arise in the presence of non-standard interactions. In particular we revisit the cases of (i) one zero mass matrices when the lowest neutrino mass is zero and (ii) one zero texture with a vanishing minor. In our study we find that for most of the cases, the texture zero conditions which are allowed for the LMA solution, are also allowed for the DLMA solution. However, we found two textures belonging to the case of one zero texture with a vanishing minor where LMA solution does not give a viable solution whereas DLMA solution does. We analyze all the possible texture zero cases belonging to these two kinds of texture zero structures in detail and present correlations between different parameters. We also present the predictions for the effective neutrino mass governing neutrino-less double beta decay for the allowed textures. |
url |
http://www.sciencedirect.com/science/article/pii/S0550321321001577 |
work_keys_str_mv |
AT monojitghosh implicationsofthedarklmasolutionforneutrinomassmatrices AT srubabatigoswami implicationsofthedarklmasolutionforneutrinomassmatrices AT ananyamukherjee implicationsofthedarklmasolutionforneutrinomassmatrices |
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