English

The MiniBooNE anomaly and heavy neutrino decay

High Energy Physics - Phenomenology 2010-01-11 v5 Cosmology and Nongalactic Astrophysics High Energy Physics - Experiment

Abstract

The anomaly in the low energy distribution of quasi-elastic neutrino events reported by the MiniBooNE collaboration is discussed. We show that the observed excess of electron-like events could originate from the production and decay of a heavy neutrino (νh\nu_h) in the MiniBooNE detector. The νh\nu_h is created by mixing in νμ\nu_\mu neutral-current interactions and decays radiatively into νγ \nu \gamma due to a transition magnetic moment between the νh\nu_h and a light neutrino ν\nu. The energy measured in the detector arises from the subsequent conversion of the decay photon into a \pair\pair pair within the detector volume. The analysis of the energy and angular distributions of the excess events suggests that the νh\nu_h has a mass around 500 MeV and the lifetime τνh109\tau_{\nu_h} \lesssim 10^{-9} s. Existing experimental data are found to be consistent with a mixing strength between the νh\nu_h and the νμ\nu_\mu of Uμh2(14)×103|U_{\mu h}|^2 \simeq (1-4)\times 10^{-3} and a νh\nu_h transition magnetic moment of μtr(16)×109μB \mu_{tr} \simeq (1- 6)\times 10^{-9} \mu_B. Finally, we discuss the reason why no significant excess of low energy events has been observed in the recent antineutrino data.

Keywords

Cite

@article{arxiv.0902.3802,
  title  = {The MiniBooNE anomaly and heavy neutrino decay},
  author = {S. N. Gninenko},
  journal= {arXiv preprint arXiv:0902.3802},
  year   = {2010}
}

Comments

version accepted for publication in Phys. Rev. Lett