English

Explaining LSND by a decaying sterile neutrino

High Energy Physics - Phenomenology 2009-11-11 v2 Astrophysics High Energy Physics - Experiment

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 gm4g m_4\sim few eV, gg being the neutrino--scalar coupling and m4m_4 the heavy neutrino mass, e.g. m4m_4 in the range from 1 keV to 1 MeV and g106103g \sim 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.

Keywords

Cite

@article{arxiv.hep-ph/0505216,
  title  = {Explaining LSND by a decaying sterile neutrino},
  author = {Sergio Palomares-Ruiz and Silvia Pascoli and Thomas Schwetz},
  journal= {arXiv preprint arXiv:hep-ph/0505216},
  year   = {2009}
}

Comments

23 pages, 5 figures, minor improvements, matches published version

R2 v1 2026-07-22T14:02:03.424Z