Solar neutrino oscillation from large extra dimensions

A plausible explanation for the existence of additional light sterile neutrinos is that they correspond to modulini, fermionic partners of moduli, which propagate in new large dimensions. We discuss the phenomenological implications of such states and show that solar neutrino oscillation is well des...

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Main Authors: Lukas, A, Ramond, P, Romanino, A, Ross, G
Format: Journal article
Language:English
Published: 2000
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author Lukas, A
Ramond, P
Romanino, A
Ross, G
author_facet Lukas, A
Ramond, P
Romanino, A
Ross, G
author_sort Lukas, A
collection OXFORD
description A plausible explanation for the existence of additional light sterile neutrinos is that they correspond to modulini, fermionic partners of moduli, which propagate in new large dimensions. We discuss the phenomenological implications of such states and show that solar neutrino oscillation is well described by small angle MSW oscillation to the tower of Kaluza Klein states associated with the modulini. In the optimal case the recoil electron energy spectrum agrees precisely with the measured one, in contrast to the single sterile neutrino case which is disfavoured. We also consider how all oscillation phenomena can be explained in a model including bulk neutrino states. In particular, we show that a naturally maximal mixing for atmospheric neutrinos can be easily obtained.
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spelling oxford-uuid:58fc2d8d-143b-4527-a252-9ec782dc8abb2022-03-26T17:07:08ZSolar neutrino oscillation from large extra dimensionsJournal articlehttp://purl.org/coar/resource_type/c_dcae04bcuuid:58fc2d8d-143b-4527-a252-9ec782dc8abbEnglishSymplectic Elements at Oxford2000Lukas, ARamond, PRomanino, ARoss, GA plausible explanation for the existence of additional light sterile neutrinos is that they correspond to modulini, fermionic partners of moduli, which propagate in new large dimensions. We discuss the phenomenological implications of such states and show that solar neutrino oscillation is well described by small angle MSW oscillation to the tower of Kaluza Klein states associated with the modulini. In the optimal case the recoil electron energy spectrum agrees precisely with the measured one, in contrast to the single sterile neutrino case which is disfavoured. We also consider how all oscillation phenomena can be explained in a model including bulk neutrino states. In particular, we show that a naturally maximal mixing for atmospheric neutrinos can be easily obtained.
spellingShingle Lukas, A
Ramond, P
Romanino, A
Ross, G
Solar neutrino oscillation from large extra dimensions
title Solar neutrino oscillation from large extra dimensions
title_full Solar neutrino oscillation from large extra dimensions
title_fullStr Solar neutrino oscillation from large extra dimensions
title_full_unstemmed Solar neutrino oscillation from large extra dimensions
title_short Solar neutrino oscillation from large extra dimensions
title_sort solar neutrino oscillation from large extra dimensions
work_keys_str_mv AT lukasa solarneutrinooscillationfromlargeextradimensions
AT ramondp solarneutrinooscillationfromlargeextradimensions
AT romaninoa solarneutrinooscillationfromlargeextradimensions
AT rossg solarneutrinooscillationfromlargeextradimensions