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Neutrino mass ordering: Circumventing the challenges using synergy between T2HK and JUNO

Sandhya Choubey, Monojit Ghosh, and Deepak Raikwal
Phys. Rev. D 106, 115013 – Published 13 December 2022

Abstract

One of the major open problems of neutrino physics is mass ordering (MO). We discuss the prospects of measuring MO with two under-construction experiments T2HK and JUNO. JUNO alone is expected to measure MO with greater than 3σ significance as long as certain experimental challenges are met. In particular, JUNO needs better than 3% energy resolution for MO measurement. On the other hand, T2HK has rather poor prospects at measuring the MO, especially for certain ranges of the CP violating parameter δCP, posing a major drawback for T2HK. In this article we show that the synergy between JUNO and T2HK will bring twofold advantage. First, the synergy between the two experiments helps us determine the MO at a very high significance. With the baseline setup of the two experiments, we have a greater than 9σ determination of the MO for all values of δCP. Second, the synergy also allows us to relax the constraints on the two experiments. We show that JUNO could perform extremely well even for an energy resolution of 5%, while for T2HK the MO problem with “bad” values of δCP goes away. The MO sensitivity for the combined analysis is expected to be greater than 6σ for all values of δCP and with just 5% energy resolution for JUNO.

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  • Received 18 July 2022
  • Accepted 17 November 2022

DOI:https://doi.org/10.1103/PhysRevD.106.115013

Published by the American Physical Society under the terms of the Creative Commons Attribution 4.0 International license. Further distribution of this work must maintain attribution to the author(s) and the published article’s title, journal citation, and DOI. Funded by SCOAP3.

Published by the American Physical Society

Physics Subject Headings (PhySH)

  1. Physical Systems
Particles & Fields

Authors & Affiliations

Sandhya Choubey*

  • Department of Physics, School of Engineering Sciences, KTH Royal Institute of Technology, AlbaNova University Center, Roslagstullsbacken 21, SE–106 91 Stockholm, Sweden and The Oskar Klein Centre for Cosmoparticle Physics, AlbaNova University Center, Roslagstullsbacken 21, SE–106 91 Stockholm, Sweden

Monojit Ghosh

  • School of Physics, University of Hyderabad, Hyderabad—500046, India and Center of Excellence for Advanced Materials and Sensing Devices, Ruder Bošković Institute, 10000 Zagreb, Croatia

Deepak Raikwal

  • Harish-Chandra Research Institute, A CI of Homi Bhabha National Institute, Chhatnag Road, Jhunsi, Prayagraj 211019, India and Homi Bhabha National Institute, Anushakti Nagar, Mumbai 400094, India

  • *choubey@kth.se
  • monojit_rfp@uohyd.ac.in
  • deepakraikwal@hri.res.in

Article Text

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Issue

Vol. 106, Iss. 11 — 1 December 2022

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Images

  • Figure 1
    Figure 1

    ΔPμμ and ΔPμe as a function of Δm312 (IO) for L=295km and two values of energy.

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  • Figure 2
    Figure 2

    Mass ordering sensitivity χ2 as a function of Δm312 (IO) for T2HK.

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  • Figure 3
    Figure 3

    Mass ordering χ2 in JUNO for 10 energy bins out of the total 200 energy bins. Systematic uncertainties are neglected.

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  • Figure 4
    Figure 4

    Mass ordering sensitivity expected from a combined analysis of JUNO and T2HK, shown as a function of Δm312 (IO). Left: δCP=0°. Right: δCP=90°.

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  • Figure 5
    Figure 5

    Expected MO sensitivity χ2 as a function of energy resolution of JUNO.

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