English

Solar and Atmospheric Four-Neutrino Oscillations

High Energy Physics - Phenomenology 2007-05-23 v2

Abstract

We present an analysis of the neutrino oscillation solutions of the solar and atmospheric neutrino problems in the framework of four-neutrino mixing where a sterile neutrino is added to the three standard ones and the mass spectra presents two separated doublets. Such scenarios allow for simultaneous transitions of solar νe\nu_e, as well as atmospheric νμ\nu_\mu, into active and sterile neutrinos controlled by the additional mixing angles ϑ23\vartheta_{23} and ϑ24\vartheta_{24}, and they contain as limiting cases the pure solar νe\nu_e-active and νe\nu_e-sterile neutrino oscillations, and the pure atmospheric νμνs\nu_\mu\to\nu_s and νμντ\nu_\mu\to\nu_\tau oscillations, respectively. We evaluate the allowed active-sterile admixture in both solar and atmospheric oscillations from the combined analysis. Our results show that, although the Super-Kamiokande data disfavour both the pure νμνs\nu_\mu\to\nu_s atmospheric channel and the pure νeνs\nu_e\to\nu_s solar channel, the result from the combined analysis still favours close-to-pure active and sterile oscillations and disfavours oscillations into a near-maximal active-sterile admixture.

Keywords

Cite

@article{arxiv.hep-ph/0105269,
  title  = {Solar and Atmospheric Four-Neutrino Oscillations},
  author = {M. C. Gonzalez-Garcia and M. Maltoni and C. Peña-Garay},
  journal= {arXiv preprint arXiv:hep-ph/0105269},
  year   = {2007}
}

Comments

ReVTeX, 22 pages, 7 Figures. Some typos corrected