Mass Splitting of Three Seesaw Neutrinos
| dc.creator | Ma, Ernest | |
| dc.date | 1999-02-25 | |
| dc.date.accessioned | 2026-07-07T04:06:31Z | |
| dc.date.available | 2026-07-07T04:06:31Z | |
| dc.description | If a family symmetry exists so that all three neutrinos have equal Majorana masses (via the seesaw mechanism), then the breaking of this symmetry from charged-lepton masses (via two-loop double $W$ exchange) implies $Δm$ less than about $10^{-9}m_0$. With the common mass $m_0 \sim$ eV for hot dark matter, $Δm^2 \sim 10^{-10}$ eV$^2$ is natural for vacuum solar neutrino oscillations. | |
| dc.description | 8 pages including 1 figure, talk at WIN99 | |
| dc.identifier | https://arxiv.org/abs/hep-ph/9902465 | |
| dc.identifier | http://arxiv.org/abs/hep-ph/9902465 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/48802 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | Mass Splitting of Three Seesaw Neutrinos | |
| dc.type | text |