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2012

Heavy neutrino decays at MiniBooNE

Masip, Manuel, Masjuan, Pere, Meloni, Davide

Understand

It has been proposed that a sterile neutrino \nu_h with m_h \approx 50 MeV and a dominant decay mode (\nu_h -> \nu\gamma) may be the origin of the experimental anomaly observed at LSND.

We define a particular model that could also explain the MiniBooNE excess consistently with the data at other neutrino experiments (radiative muon capture at TRIUMF, T2K, or single photon at NOMAD).
The key ingredients are (i) its long lifetime (\tau_h\approx 3-7x10^{-9} s), which introduces a 1/E dependence with the event energy, and (ii) its Dirac nature, which implies a photon preferably emitted opposite to the beam direction and further reduces the event energy at MiniBooNE.
We show that these neutrinos are mostly produced through electromagnetic interactions with nuclei, and that T2K observations force BR(\nu_h -> \nu_\tau\gamma) \le 0.01 \approx BR(\nu_h -> \nu_\mu\gamma).

Built on

L. F. Li and F. Wilczek, Phys. Rev. D 25
1982
Earlier work this paper cites.
R.N. Mohapatra and P.B. Pal, Massive Neutrinos in Physics and Astrophysics
1991
Earlier work this paper cites.
C. J. Horowitz, H. -c. Kim, D. P. Murdock and S. Pollock, Phys. Rev. C 48
1993
Earlier work this paper cites.
S. N. Gninenko and N. V. Krasnikov, Phys. Lett. B 450
1999
Earlier work this paper cites.
A. D. Dolgov, S. H. Hansen, G. Raffelt and D. V. Semikoz, Nucl. Phys. B 580
2000
Earlier work this paper cites.
C. Athanassopoulos et al
2001
Earlier work this paper cites.
V. Bernard, T. R. Hemmert and U. G. Meissner, Nucl. Phys. A 686
2001
Earlier work this paper cites.
B. Armbruster et al
2002
Earlier work this paper cites.
R. Bernabei et al
Original
2008
Earlier work this paper cites.