Oscillations of the Be7 solar neutrinos inside the Earth

A. N. Ioannisian, A. Yu. Smirnov, and D. Wyler
Phys. Rev. D 92, 013014 – Published 30 July 2015

Abstract

We explore in detail oscillations of solar Be7 neutrinos passing through the Earth. The depth of oscillations is at the (0.1–0.2)% level, and the length is approximately 30 km. The change of the oscillatory modulations with energy is comparable to the width of the Be7 line, which is determined by the temperature in the center of the Sun. This means that, depending on the length of the trajectory (nadir angle), one obtains different degrees of cancellations when averaging the oscillations over the Be7 neutrino energy. Thus, by exploring these oscillations in detail, it is possible to determine the width of the Be7 line and therefore the temperature of the Sun and to fix Δm212 precisely. Furthermore, it allows us to perform tomography of the Earth, in particular to measure the deviation from a spherical mass distribution and detect small inhomogeneities. Studies of the Be neutrinos open up a possibility to test quantum mechanics of neutrino oscillations and search for sterile neutrinos. We also estimate the accuracy of these measurements with future scintillator (or scintillator uploaded) detectors of 100kton mass.

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  • Received 29 April 2015

DOI:https://doi.org/10.1103/PhysRevD.92.013014

© 2015 American Physical Society

Authors & Affiliations

A. N. Ioannisian1,2, A. Yu. Smirnov3,4, and D. Wyler5

  • 1Yerevan Physics Institute, Alikhanian Br. 2, 375036 Yerevan, Armenia
  • 2Institute for Theoretical Physics and Modeling, 375036 Yerevan, Armenia
  • 3Max-Planck Institute for Nuclear Physics, Saupfercheckweg 1, D-69117 Heidelberg, Germany
  • 4ICTP, Strada Costiera 11, 34014 Trieste, Italy
  • 5Institut für Theoretische Physik, Universität Zürich, Winterthurerstrasse 190, CH-8057 Zürich, Switzerland

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Issue

Vol. 92, Iss. 1 — 1 July 2015

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