L/E-Flatness of the Electron-Like Event Ratio in Super-Kamiokande and a Degeneracy in Neutrino Masses

نویسندگان

  • I. Stancu
  • D. V. Ahluwalia
چکیده

We show that the L/E-flatness of the electron-like event ratio in the Super-Kamiokande atmospheric neutrino data implies the equality of the expectation values for the muon and tau neutrino masses. We establish this result by obtaining a set of three constraints on the neutrino-oscillation mixing matrix as contained in the indicated flatness. The resulting 3× 3 neutrino-oscillation matrix depends only on one angle. A remarkable result that follows directly from this matrix is the consistency between the mixing angles observed by LSND and Super-Kamiokande. Preprint submitted to Elsevier Preprint 18 April 2008

برای دانلود 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

Cp Violation in Neutrino Oscillations and L/e Flatness of the E-like Event Ratio at Super-kamiokande

We show that if the presently observed L/E-flatness of the electron-like event ratio in the Super-Kamiokande atmospheric neutrino data is confirmed then the indicated ratio must be unity. Further, it is found that once CP is violated the exact L/E flatness implies: (a) The CP-violating phase, in the standard parameterization, is narrowed down to two possibilities ±π/2, and (b) The mixing betwee...

متن کامل

Robust flavor equalization of cosmic neutrino flux by quasi bi - maximal mixing ⋆

The observed L/E flatness of the electron-like event ratio in the Super-Kamiokande atmospheric neutrino data strongly favors a quasi bi-maximal mixing matrix. This situation is here exploited to understand the numerical results of Yasuda on the high energy cosmic neutrino flux. In agreement with the Yasuda result, we analytically show how the quasi bi-maximal neutrino mixing makes the high ener...

متن کامل

Atmospheric neutrino data : Active-Active × Active-Sterile oscillations

Atmospheric showers are initiated when primary cosmic rays hit the Earth’s atmosphere. Secondary mesons produced in this collision, mostly pions and kaons, decay and give rise to electron and muon neutrino and anti-neutrinos fluxes [1]. In the past Fréjus and NUSEX [2] reported a R-value (R = (μ/e)data/(μ/e)MC) consistent with one, therefore other detectors like Kamiokande, IMB and Soudan-2 [3]...

متن کامل

Solutions to the Atmospheric Neutrino Problem

Neutrinos produced as decay products in hadronic showers from cosmic ray collisions with nuclei in the upper atmosphere have been observed by several detectors [1–7]. Although the absolute fluxes of atmospheric neutrinos are largely uncertain, the expected ratio (μ/e) of the muon neutrino flux (νμ + ν̄μ) over the electron neutrino flux (νe + ν̄e) is robust, since it largely cancels out the uncert...

متن کامل

Results from Super-kamiokande

The results from Super-Kamiokande on atmospheric neutrinos and solar neutrinos are presented. The contained event analysis of atmospheric neutrinos shows a small value of p/e ratio and a large asymmetry in the zenith angle distribution. A distortion of zenith angle distribution is observed in the upward-through-going muons resulting from atmospheric neutrino interactions in the rock surrounding...

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

برای دانلود 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

عنوان ژورنال:

دوره   شماره 

صفحات  -

تاریخ انتشار 1999