Stability of the Next-to-Tribimaximal Mixings under Radiative Corrections with the Variation of the SUSY Breaking Scale in MSSM

We analyze the radiative stability of the next-to-tribimaximal mixings (NTBM) with the variation of the SUSY breaking scale (mS) in MSSM, for both normal ordering (NO) and inverted ordering (IO) at the fixed input value of the seesaw scale MR=1015 GeV and two different values of tanβ. All the neutri...

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Main Authors: Kh. Helensana Devi, K. Sashikanta Singh, N. Nimai Singh
Format: Article
Language:English
Published: Wiley 2023-01-01
Series:Advances in High Energy Physics
Online Access:http://dx.doi.org/10.1155/2023/2365316
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author Kh. Helensana Devi
K. Sashikanta Singh
N. Nimai Singh
author_facet Kh. Helensana Devi
K. Sashikanta Singh
N. Nimai Singh
author_sort Kh. Helensana Devi
collection DOAJ
description We analyze the radiative stability of the next-to-tribimaximal mixings (NTBM) with the variation of the SUSY breaking scale (mS) in MSSM, for both normal ordering (NO) and inverted ordering (IO) at the fixed input value of the seesaw scale MR=1015 GeV and two different values of tanβ. All the neutrino oscillation parameters receive varying radiative corrections irrespective of the mS values at the electroweak scale, which are all within the 3σ range of the latest global fit data at a low value of tanβ. NO is found to be more stable than IO for all four different NTBM mixing patterns.
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institution Kabale University
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spelling doaj-art-0da2d059ccb54163b3e98142d5a9574f2025-02-03T06:47:33ZengWileyAdvances in High Energy Physics1687-73652023-01-01202310.1155/2023/2365316Stability of the Next-to-Tribimaximal Mixings under Radiative Corrections with the Variation of the SUSY Breaking Scale in MSSMKh. Helensana Devi0K. Sashikanta Singh1N. Nimai Singh2Department of PhysicsDepartment of PhysicsDepartment of PhysicsWe analyze the radiative stability of the next-to-tribimaximal mixings (NTBM) with the variation of the SUSY breaking scale (mS) in MSSM, for both normal ordering (NO) and inverted ordering (IO) at the fixed input value of the seesaw scale MR=1015 GeV and two different values of tanβ. All the neutrino oscillation parameters receive varying radiative corrections irrespective of the mS values at the electroweak scale, which are all within the 3σ range of the latest global fit data at a low value of tanβ. NO is found to be more stable than IO for all four different NTBM mixing patterns.http://dx.doi.org/10.1155/2023/2365316
spellingShingle Kh. Helensana Devi
K. Sashikanta Singh
N. Nimai Singh
Stability of the Next-to-Tribimaximal Mixings under Radiative Corrections with the Variation of the SUSY Breaking Scale in MSSM
Advances in High Energy Physics
title Stability of the Next-to-Tribimaximal Mixings under Radiative Corrections with the Variation of the SUSY Breaking Scale in MSSM
title_full Stability of the Next-to-Tribimaximal Mixings under Radiative Corrections with the Variation of the SUSY Breaking Scale in MSSM
title_fullStr Stability of the Next-to-Tribimaximal Mixings under Radiative Corrections with the Variation of the SUSY Breaking Scale in MSSM
title_full_unstemmed Stability of the Next-to-Tribimaximal Mixings under Radiative Corrections with the Variation of the SUSY Breaking Scale in MSSM
title_short Stability of the Next-to-Tribimaximal Mixings under Radiative Corrections with the Variation of the SUSY Breaking Scale in MSSM
title_sort stability of the next to tribimaximal mixings under radiative corrections with the variation of the susy breaking scale in mssm
url http://dx.doi.org/10.1155/2023/2365316
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AT nnimaisingh stabilityofthenexttotribimaximalmixingsunderradiativecorrectionswiththevariationofthesusybreakingscaleinmssm