MSW Without Matter
| dc.creator | Goldman, T. | |
| dc.creator | McKellar, B. H. J. | |
| dc.creator | Stephenson Jr., G. J. | |
| dc.date | 1996-08-09 | |
| dc.date.accessioned | 2026-07-07T03:59:44Z | |
| dc.date.available | 2026-07-07T03:59:44Z | |
| dc.description | We examine the effects of a scalar field, coupled only to neutrinos, on oscillations among weak interaction current eigenstates. The existence of a real scalar field is manifested as effective masses for the neutrino mass eigenstates, the same for $\nbar$ as for $\n$. Under some conditions, this can lead to a vanishing of $δm^2$, giving rise to MSW-like effects. We present an idealized example and show that it may be possible to resolve the apparent discrepancy in spectra required by r-process nucleosynthesis in the mantles of supernovae and by Solar neutrino solutions. | |
| dc.description | 3pp. LaTeX including 2 psfigures; to appear in Proceedings, DPF96, Minneapolis, 11-15 August 1996 | |
| dc.identifier | https://arxiv.org/abs/hep-ph/9608287 | |
| dc.identifier | http://arxiv.org/abs/hep-ph/9608287 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/46348 | |
| dc.subject | High Energy Physics - Phenomenology | |
| dc.title | MSW Without Matter | |
| dc.type | text |