English

Series expansions for three-flavor neutrino oscillation probabilities in matter

High Energy Physics - Phenomenology 2009-11-10 v2 High Energy Physics - Experiment

Abstract

We present a number of complete sets of series expansion formulas for neutrino oscillation probabilities in matter of constant density for three flavors. In particular, we study expansions in the mass hierarchy parameter αΔm212/Δm312\alpha \equiv \Delta m_{21}^2/\Delta m_{31}^2 and mixing parameter s13sinθ13s_{13} \equiv \sin \theta_{13} up to second order and expansions only in α\alpha and only in s13s_{13} up to first order. For each type of expansion we also present the corresponding formulas for neutrino oscillations in vacuum.We perform a detailed analysis of the accuracy of the different sets of series expansion formulas and investigate which type of expansion is most accurate in different regions of the parameter space spanned by the neutrino energy E, the baseline length L, and the expansion parameters α\alpha and s13s_{13}.We also present the formulas for series expansions in α\alpha and in s13s_{13} up to first order for the case of arbitrary matter density profiles. Furthermore, it is shown that in general all the 18 neutrino and antineutrino oscillation probabilities can be expressed through just two independent probabilites.

Keywords

Cite

@article{arxiv.hep-ph/0402175,
  title  = {Series expansions for three-flavor neutrino oscillation probabilities in matter},
  author = {E. K. Akhmedov and R. Johansson and M. Lindner and T. Ohlsson and T. Schwetz},
  journal= {arXiv preprint arXiv:hep-ph/0402175},
  year   = {2009}
}

Comments

36 pages, 7 figures, minor improvements, typos in Eqs. (58) and (59) corrected, version published in JHEP