Bi-maximal Neutrino Mixing With SO(3) Flavour Symmetry
| dc.creator | Ghosal, Ambar | |
| dc.date | 1999-05-25 | |
| dc.date | 1999-06-15 | |
| dc.date.accessioned | 2026-07-07T04:07:11Z | |
| dc.date.available | 2026-07-07T04:07:11Z | |
| dc.description | We demonstrate that an $SU(2)_L\times U(1)_Y$ model with extended Higgs sector gives rise to bi-maximal neutrino mixing through the incorporation of SO(3) flavour symmetry and discrete symmetry. The neutrino and the charged lepton masses are generated due to higher dimensional terms. The hierarchical structures of neutrinos and charged leptons are obtained due to inclusion of SO(3) flavour symmetry and discrete symmetry.The model can accommodate the vacuum oscillation solution of solar neutrino problem, through reasonable choice of model parameters along with the atmospheric neutrino experimental result. | |
| dc.description | 13pages, Latex, revised version | |
| dc.identifier | https://arxiv.org/abs/hep-ph/9905470 | |
| dc.identifier | http://arxiv.org/abs/hep-ph/9905470 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/49055 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | Bi-maximal Neutrino Mixing With SO(3) Flavour Symmetry | |
| dc.type | text |