Explaining LSND by a decaying sterile neutrino
| dc.contributor.area | Physics | en_US |
| dc.contributor.author | Palomares-Ruiz, Sergio | en_US |
| dc.contributor.author | Pascoli, Silvia | en_US |
| dc.contributor.author | Schwetz, Thomas | en_US |
| dc.contributor.department | Elementary Particle Theory | en_US |
| dc.date.accessioned | 2005 | en_US |
| dc.date.accessioned | 2011-09-07T20:28:42Z | |
| dc.date.available | 2005 | en_US |
| dc.date.available | 2011-09-07T20:28:42Z | |
| dc.date.issued | 2005 | en_US |
| dc.description.abstract | We propose an explanation of the LSND evidence for electron antineutrino appearance based on neutrino decay. We introduce a heavy neutrino, which is produced in pion and muon decays because of a small mixing with muon neutrinos, and then decays into a scalar particle and a light neutrino, predominantly of the electron type. We require values of gm4 ~ few eV, g being the neutrino-scalar coupling and m4 the heavy neutrino mass, e.g. m4 in the range from 1 keV to 1 MeV and g ~ 10-6-10-3. Performing a fit to the LSND data as well as all relevant null-result experiments, we show that all data can be explained within this decay scenario. In the minimal version of the decay model, we predict a signal in the upcoming MiniBooNE experiment corresponding to a transition probability of the same order as seen in LSND. In addition, we show that extending our model to two nearly degenerate heavy neutrinos it is possible to introduce CP violation in the decay, which can lead to a suppression of the signal in MiniBooNE running in the neutrino mode. We briefly discuss signals in future neutrino oscillation experiments, we show that our scenario is compatible with bounds from laboratory experiments, and we comment on implications in astrophysics and cosmology. | en_US |
| dc.format.extent | 343566 bytes | en_US |
| dc.format.mimetype | application/pdf | en_US |
| dc.identifier.citation | JHEP 0509 (2005) 048 | en_US |
| dc.identifier.uri | https://openscience.sissa.it/handle/1963/1744 | en_US |
| dc.language.iso | en_US | en_US |
| dc.relation.ispartofseries | SISSA;34/2005/EP | en_US |
| dc.relation.ispartofseries | arXiv.org;hep-ph/0505216 | en_US |
| dc.relation.uri | 10.1088/1126-6708/2005/09/048 | en_US |
| dc.title | Explaining LSND by a decaying sterile neutrino | en_US |
| dc.type | Preprint | en_US |