Radiative four neutrino masses and mixings
| dc.creator | Roy, Probir | |
| dc.date | 1998-10-22 | |
| dc.date.accessioned | 2026-07-07T04:05:31Z | |
| dc.date.available | 2026-07-07T04:05:31Z | |
| dc.description | The radiative model, proposed by Zee, is extended from the three neutrino $(ν_{e,μ,τ})$ sector to include a fourth sterile neutrino $ν_s$. The oscillations $ν_e \leftrightarrow ν_s$ (solar), $ν_μ\leftrightarrow ν_τ$ (atmospheric) and $ν_e \leftrightarrow ν_μ$ (LSND) are invoked to explain all oscillation data with the successful relation $(Δm^2)_{atm} \simeq 2[(Δm^2)_{solar} (Δm^2)_{LSND}]^{1/2}$ as an added bonus. | |
| dc.description | Talk given at the XXIX International Conference on High Energy Physics, Vancouver | |
| dc.identifier | https://arxiv.org/abs/hep-ph/9810448 | |
| dc.identifier | http://arxiv.org/abs/hep-ph/9810448 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/48436 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | Radiative four neutrino masses and mixings | |
| dc.type | text |