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Resolving the atmospheric octant by an improved measurement of the reactor angle

Sabya Sachi Chatterjee, Pedro Pasquini, and J. W. F. Valle
Phys. Rev. D 96, 011303(R) – Published 20 July 2017

Abstract

Taking into account the current global information on neutrino oscillation parameters we forecast the capabilities of future long-baseline experiments such as DUNE and T2HK in settling the atmospheric octant puzzle. We find that a good measurement of the reactor angle θ13 plays a key role in fixing the octant of the atmospheric angle θ23 with such future accelerator neutrino studies.

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  • Received 14 March 2017

DOI:https://doi.org/10.1103/PhysRevD.96.011303

© 2017 American Physical Society

Physics Subject Headings (PhySH)

Particles & Fields

Authors & Affiliations

Sabya Sachi Chatterjee1,2,*, Pedro Pasquini3,†, and J. W. F. Valle4,‡

  • 1Institute of Physics, Sachivalaya Marg, Sainik School Post, Bhubaneswar 751005, India
  • 2Homi Bhabha National Institute, Training School Complex, Anushakti Nagar, Mumbai 400085, India
  • 3Instituto de Física Gleb Wataghin—UNICAMP, 13083-859 Campinas São Paulo, Brazil
  • 4AHEP Group, Institut de Física Corpuscular—C.S.I.C./Universitat de València, Parc Cientific de Paterna. Calle Catedratico José Beltrán, 2 E-46980 Paterna (València), SPAIN

  • *sabya@iopb.res.in
  • pasquini@ifi.unicamp.br
  • valle@ific.uv.es

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Issue

Vol. 96, Iss. 1 — 1 July 2017

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