Status of Oscillation plus Decay of Atmospheric and Long-Baseline Neutrinos

نویسندگان

  • M. C. Gonzalez-Garcia
  • Michele Maltoni
چکیده

We study the interplay of neutrino oscillation and invisible decay in atmospheric and long-baseline neutrinos experiments. We perform a global analysis of the full atmospheric data from Super-Kamiokande together with long-baseline K2K and MINOS in these scenarios. We find that the admixture of νμ → ντ oscillations with parameters ∆m232 = 2.6×10 −3 eV and θ23 ∼ 34 ◦ plus decay of the heavy neutrino, ν3, with lifetime of the order τ3/m3 ∼ 2.6× 10 −12 s/eV provides a reasonable fit to atmospheric neutrinos, although this solution becomes more disfavored (dropping to the 99% CL) once long-baseline data are included. Other than this local minimum, the analysis shows no evidence in favor of a non-vanishing neutrino decay width and an lower bound on the decay lifetime τ3/m3 ≥ 9.3 × 10 −11 s/eV is set at 99% CL. In the framework of Majoron models, this constraint can be translated into a bound on the Majoron coupling to ν3 and an unmixed very light sterile state, |gs3| ≤ 8.6 × 10 −3 (2.2 eV/m3).

برای دانلود رایگان متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

Constraints on Neutrinoless Double Beta Decay from Neutrino Oscillation Experiments

We show that, in the framework of a general model with mixing of three Majorana neutrinos and a neutrino mass hierarchy, the results of the Bugey and Krasnoyarsk reactor neutrino oscillation experiments imply strong limitations for the effective Majorana mass | 〈m〉 | that characterizes the amplitude of neutrinoless double beta decay. We obtain further limitations on | 〈m〉 | from the data of the...

متن کامل

Reconciling Cold Dark Matter with Cobe/iras plus Solar and Atmospheric Neutrino Data

We present a model where an unstable MeV Majorana tau neutrino can naturally reconcile the cold dark matter model (CDM) with cosmological observations of large and small scale density fluctuations and, simultaneously, with data on solar and atmospheric neutrinos. The solar neutrino deficit is explained through long wavelength, socalled just-so oscillations involving conversions of νe into both ...

متن کامل

Atmospheric Neutrino Oscillations among Three Neutrino Flavors and Long-baseline Experiments

Anticipating future long-baseline neutrino experiments to search for neutrino oscillations in various oscillation channels, we have analyzed the atmospheric neutrino data in the framework of a model with mixing of three massive neutrino fields that can accommodate the data of solar neutrino experiments. The oscillations of atmospheric and terrestrial neutrinos are described in this model by thr...

متن کامل

Earth matter density uncertainty in atmospheric neutrino oscillations

Abstract That muon neutrinos νμ oscillating into the mixture of tau neutrinos ντ and sterile neutrinos νs has been studied to explain the atmospheric νμ disappearance. In this scenario, the effect of Earth matter is a key to determine the fraction of νs. Considering that the Earth matter density has uncertainty and this uncertainty has significant effects in some neutrino oscillation cases, suc...

متن کامل

Atmospheric and Long Baseline Neutrino

This paper presents the recent results from Super-Kamiokande atmospheric neutri-nos and from K2K accelerator neutrinos. Both results show the signal of neutrino oscillation, and provide new and precise information of oscillation parameters. The oscillation parameters are constraint to be between 1.5×10 −3 eV 2 and 3.9×10 −3 eV 2 for ∆m 2 and to be greater than 0.92 for sin 2 2θ.

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

عنوان ژورنال:

دوره   شماره 

صفحات  -

تاریخ انتشار 2008