Searching non-standard interactions with atmospheric neutrinos at ESSnuSB

Atmospheric neutrinos provide a unique avenue to study neutrino interactions in matter. In this work, the prospects of constraining non-standard neutrino interactions with atmospheric neutrino oscillations are investigated for the proposed ESSnuSB far detector. By analyzing atmospheric neutrino samples equivalent to 5.4 Mt$\cdot$year exposure, it is found that ESSnuSB could be able to set the upper bounds $|ε_{eμ}^m| < 0.053, |ε_{eτ}^m| < 0.057, |ε_{μτ}^m| < 0.021, ε_{ee}^m - ε_{μμ}^m < 0.075$ and $|ε_{ττ}^m - ε_{μμ}^m| < 0.031$ at $90\%$ CL, when the results are minimized for $ϕ_{eμ}^m, ϕ_{eτ}^m$ and $ϕ_{μτ}^m$ and normal ordering is assumed for neutrino masses. It is also shown that the presence of non-standard interactions could affect the sensitivities to neutrino mass ordering and $θ_{23}^{}$ octant in comparison to the standard interaction scheme. The results of this work highlight the complementarity between atmospheric and accelerator neutrino programs in ESSnuSB.

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ArXiv.org
Published
2025-08-25
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Particle physics theoretical and experimental studies
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article
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article

Searching non-standard interactions with atmospheric neutrinos at ESSnuSB

Μάρκος Αναστασόπουλος, Sampsa Vihonen, E. Kasimi, H. Danared et al.
ArXiv.org
Particle physics theoretical and experimental studies
article

Searching non-standard interactions with atmospheric neutrinos at ESSnuSB

Μάρκος Αναστασόπουλος, Sampsa Vihonen, E. Kasimi, H. Danared, Alessio Giarnetti, G. Vankova-Kirilova, E. Bouquerel, P. Cupiał, D Sampsonidis, Nikolaos Gazis, P. Christiansen, F. Bramati, I Efthymiopoulos, Tommy Ohlsson, G. Brunetti, F. Sordo, T. W. Choi, Soraia Marangoni, M. Pari, R. Tarkeshian, B. Kildetoft, N. Vassilopoulos, A. Branca, A. Kayis Topaksu, L Halić, I. Bustinduy, Rickard Johansson, K. Niewczas, F Terranova, Martin Jenssen, Monojit Ghosh, B. Bolling, D d'Ago, Georgi V. Petkov, F. Pupilli, N. Jachowicz, R. Tsenov, Andrea Bignami, A. Tsirigotis, Matthew Collins, M Oglakci, T. Ekelöf, Davide Meloni, Branka Kovač, Natalia Milas, M. Bogomilov, Maja Olvegård, D. Saiang, C. Maiano, Mamad Eshraqi, M. Dracos, Anna Scanu, V. Zeter, Sandhya Choubey, Jacques Wurtz, M Blennow, E. Baussan, C. Marrelli, A. Leisos, E. Cristaldo Morales, A. Farricker, E. Fasoula, M. C. F. Hooft, J. A. Aguilar, E. Trachanas, Leszek Patrzałek, G Fanourakis, G Stavropoulos, Th. Geralis, Ch. Petridou, M Mezzetto, T. Fukuda, G. Gökbulut, Pascal Poussot, K. Kordas, A. Longhin, O. Zormpa, A. Psallidas, J. Cederkäll, C. Hagner, C. Schwab, T. Tolba, D. Barčot, M. Vanderpoorten, R Moolya
article en

Abstract

Atmospheric neutrinos provide a unique avenue to study neutrino interactions in matter. In this work, the prospects of constraining non-standard neutrino interactions with atmospheric neutrino oscillations are investigated for the proposed ESSnuSB far detector. By analyzing atmospheric neutrino samples equivalent to 5.4 Mt$\cdot$year exposure, it is found that ESSnuSB could be able to set the upper bounds $|ε_{eμ}^m| < 0.053, |ε_{eτ}^m| < 0.057, |ε_{μτ}^m| < 0.021, ε_{ee}^m - ε_{μμ}^m < 0.075$ and $|ε_{ττ}^m - ε_{μμ}^m| < 0.031$ at $90\%$ CL, when the results are minimized for $ϕ_{eμ}^m, ϕ_{eτ}^m$ and $ϕ_{μτ}^m$ and normal ordering is assumed for neutrino masses. It is also shown that the presence of non-standard interactions could affect the sensitivities to neutrino mass ordering and $θ_{23}^{}$ octant in comparison to the standard interaction scheme. The results of this work highlight the complementarity between atmospheric and accelerator neutrino programs in ESSnuSB.

ArXiv.org
Institut Pluridisciplinaire Hubert Curien (FR)
Openalex Percentile: Top 86%
Particle physics theoretical and experimental studies
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