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Alleviating the present tension between T2K and NOνA with nonstandard neutrino interactions

Adriano Cherchiglia1,2, Pedro Pasquini3,1, O. L. G. Peres1, F. F. Rodrigues1,4, R. R. Rossi1,5, and E. S. Souza1

Phys. Rev. D 112, 093004 – Published 13 November, 2025

DOI: https://doi.org/10.1103/55qm-zbhv

Abstract

Since neutrino oscillation was observed, several experiments have been built to measure its parameters. NuMI Off-axis νe Appearance (NOνA) and Tokai-to-Kamioka (T2K) are two long-baseline experiments dedicated to measuring mainly the mixing angle θ23, the charge-parity (CP) conjugation phase δCP, and the mass ordering. However, there is a tension in current data. The T2K allowed region is in conflict with the region allowed by NOνA. We propose a nonstandard charged current interaction (CC-NSI) in neutrino production to relieve this tension. The CC-NSI is computed through quantum field theory formalism, where we derive perturbative analytical formulae considering CC-NSI in the pion decay. Within this new approach, we can alleviate NOνA and T2K tension for CC-NSI complex parameters of order 10−3. We show the new phase has a degeneracy to the Dirac CP phase of the form δCP±ϕ=1.5π, being a possible source of violation of charge-parity symmetry.

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References (71)

  1. I. Esteban, M. C. Gonzalez-Garcia, M. Maltoni, T. Schwetz, and A. Zhou, J. High Energy Phys. 09 (2020) 178.
  2. I. Esteban, M. C. Gonzalez-Garcia, M. Maltoni, I. Martinez-Soler, J. P. Pinheiro, and T. Schwetz, J. High Energy Phys. 12 (2024) 216.
  3. P. F. de Salas, D. V. Forero, S. Gariazzo, P. Martínez-Miravé, O. Mena, C. A. Ternes, M. Tórtola, and J. W. F. Valle, J. High Energy Phys. 02 (2021) 071.
  4. F. Capozzi, E. Di Valentino, E. Lisi, A. Marrone, A. Melchiorri, and A. Palazzo, Phys. Rev. D 104, 083031 (2021).
  5. M. Nizam, S. Bharti, S. Prakash, U. Rahaman, and S. Uma Sankar, Mod. Phys. Lett. A 35, 06 (2019).
  6. K. J. Kelly, P. A. N. Machado, S. J. Parke, Y. F. Perez-Gonzalez, and R. Z. Funchal, Phys. Rev. D 103, 013004 (2021).
  7. M. A. Acero et al. (NOvA Collaboration), Phys. Rev. D 106, 032004 (2022).
  8. K. Abe et al. (T2K Collaboration), Eur. Phys. J. C 83, 782 (2023).
  9. D. Dutta and P. Ghoshal, J. High Energy Phys. 09 (2016) 110.
  10. L. S. Miranda, P. Pasquini, U. Rahaman, and S. Razzaque, Eur. Phys. J. C 81, 444 (2021).
  11. X. Y. Yu, Z. Guan, U. Rahaman, and N. Ilic, arXiv:2501.00146.
  12. F. Capozzi, S. S. Chatterjee, and A. Palazzo, Phys. Rev. Lett. 124, 111801 (2020).
  13. S. S. Chatterjee and A. Palazzo, Phys. Rev. Lett. 126, 051802 (2021).
  14. S. S. Chatterjee and A. Palazzo, Phys. Rev. D 110, 113002 (2024).
  15. P. B. Denton, J. Gehrlein, and R. Pestes, Phys. Rev. Lett. 126, 051801 (2021).
  16. R. Majhi, D. K. Singha, K. N. Deepthi, and R. Mohanta, Eur. Phys. J. C 82, 919 (2022).
  17. S. S. Chatterjee and A. Palazzo, arXiv:2005.10338.
  18. A. de Gouvêa, G. Jusino Sánchez, and K. J. Kelly, Phys. Rev. D 106, 055025 (2022).
  19. U. Rahaman, Eur. Phys. J. C 81, 792 (2021).
  20. U. Rahaman, S. Razzaque, and S. U. Sankar, Universe 8, 109 (2022).
  21. H. X. Lin, J. Tang, and S. Vihonen, arXiv:2312.11704.
  22. G. Alonso-Álvarez, J. M. Cline, B. Laurent, and U. Rahaman, Eur. Phys. J. C 85, 635 (2025).
  23. L. Konwar, J. Vardani, and B. Yadav, Eur. Phys. J. C 84, 1103 (2024).
  24. A. Falkowski, M. González-Alonso, and Z. Tabrizi, J. High Energy Phys. 05 (2019) 173.
  25. A. Falkowski, M. González-Alonso, and Z. Tabrizi, J. High Energy Phys. 11 (2020) 048.
  26. Y. Du, H. L. Li, J. Tang, S. Vihonen, and J. H. Yu, J. High Energy Phys. 03 (2021) 019.
  27. A. Falkowski, M. González-Alonso, J. Kopp, Y. Soreq, and Z. Tabrizi, J. High Energy Phys. 10 (2021) 086.
  28. M. E. Chaves, P. C. de Holanda, and O. L. G. Peres, J. High Energy Phys. 03 (2023) 180.
  29. Y. Du, H. L. Li, J. Tang, S. Vihonen, and J. H. Yu, Phys. Rev. D 105, 075022 (2022).
  30. V. Bresó-Pla, A. Falkowski, M. González-Alonso, and K. Monsálvez-Pozo, J. High Energy Phys. 05 (2023) 074.
  31. J. Kopp, N. Rocco, and Z. Tabrizi, J. High Energy Phys. 08 (2024) 187.
  32. A. Cherchiglia and J. Santiago, J. High Energy Phys. 03 (2024) 018.
  33. P. Coloma, E. Fernández-Martínez, J. López-Pavón, X. Marcano, D. Naredo-Tuero, and S. Urrea, J. High Energy Phys. 02 (2025) 137.
  34. V. Bresó-Pla, S. Cruz-Alzaga, M. González-Alonso, and S. Prakash, arXiv:2505.01275.
  35. F. Kling, Y. Ma, K. Mekała, J. Reuter, and Z. Tabrizi, arXiv:2508.00761.
  36. S. Navas et al. (Particle Data Group), Phys. Rev. D 110, 030001 (2024).
  37. Z. Maki, M. Nakagawa, and S. Sakata, Prog. Theor. Phys. 28, 870 (1962).
  38. B. Pontecorvo, Sov. Phys. JETP 6, 429 (1958).
  39. N. Cabibbo, Phys. Rev. Lett. 10, 531 (1963).
  40. M. Kobayashi and T. Maskawa, Prog. Theor. Phys. 49, 652 (1973).
  41. See Supplemental Material at http://link.aps.org/supplemental/10.1103/55qm-zbhv for the full formula of the probability and some additional plots.
  42. W. Grimus and P. Stockinger, Phys. Rev. D 54, 3414 (1996).
  43. S. P. Mikheev and A. Y. Smirnov, Nuovo Cimento Soc. Ital. Fis. 9C, 17 (1986).
  44. L. Wolfenstein, Phys. Rev. D 17, 2369 (1978).
  45. M. M. Guzzo, L. J. F. Leite, S. W. P. Novelo, O. L. G. Peres, and V. Pleitez, Phys. Rev. D 107, 095037 (2023).
  46. K. Asano and H. Minakata, J. High Energy Phys. 06 (2011) 022.
  47. C. Jarlskog, Phys. Rev. Lett. 55, 1039 (1985).
  48. C. Jarlskog, Z. Phys. C 29, 491 (1985).
  49. P. Adamson et al. (NOvA Collaboration), Phys. Rev. Lett. 116, 151806 (2016).
  50. M. A. Acero et al. (NOvA Collaboration), Phys. Rev. Lett. 123, 151803 (2019).
  51. M. A. Acero et al. (NOvA Collaboration), Phys. Rev. D 110, 012005 (2024).
  52. K. Abe et al. (T2K Collaboration), Nucl. Instrum. Methods Phys. Res., Sect. A 659, 106 (2011).
  53. K. Abe et al. (T2K Collaboration), Phys. Rev. Lett. 107, 041801 (2011).
  54. K. Abe et al. (T2K Collaboration), Phys. Rev. D 103, 112008 (2021).
  55. C. Andreopoulos, C. Barry, S. Dytman, H. Gallagher, T. Golan, R. Hatcher, G. Perdue, and J. Yarba, arXiv:1510.05494.
  56. W. Li et al. (GENIE Collaboration), Phys. Rev. D 110, 072016 (2024).
  57. P. Huber, M. Lindner, and W. Winter, Comput. Phys. Commun. 167, 195 (2005).
  58. P. Huber, J. Kopp, M. Lindner, M. Rolinec, and W. Winter, Comput. Phys. Commun. 177, 432 (2007).
  59. F. P. An et al. (Daya Bay Collaboration), Phys. Rev. Lett. 130, 161802 (2023).
  60. Double Chooz Collaboration, Nat. Phys. 16, 558 (2020).
  61. G. Bak et al. (RENO Collaboration), Phys. Rev. Lett. 121, 201801 (2018).
  62. H. Minakata and H. Nunokawa, J. High Energy Phys. 10 (2001) 001.
  63. M. Ishitsuka, T. Kajita, H. Minakata, and H. Nunokawa, Phys. Rev. D 72, 033003 (2005).
  64. N. C. Ribeiro, H. Minakata, H. Nunokawa, S. Uchinami, and R. Zukanovich-Funchal, J. High Energy Phys. 12 (2007) 002.
  65. H. Nunokawa, S. J. Parke, and J. W. F. Valle, Prog. Part. Nucl. Phys. 60, 338 (2008).
  66. A. M. Gago, H. Minakata, H. Nunokawa, S. Uchinami, and R. Zukanovich Funchal, J. High Energy Phys. 01 (2010) 049.
  67. O. Mena, H. Nunokawa, and S. J. Parke, Phys. Rev. D 75, 033002 (2007).
  68. M. Maltoni and T. Schwetz, Phys. Rev. D 68, 033020 (2003).
  69. M. Maltoni, T. Schwetz, M. A. Tortola, and J. W. F. Valle, Nucl. Phys. B643, 321 (2002).
  70. P. A. N. Machado, 10.11606/T.43.2013.tde-03092014-091936 (2013).
  71. L. J. F. Leite, Code to compute the pion leptonic decay rate for NSI scenario (2023), https://github.com/LeoFerreira8/Pion-Decay-w-Scalar.

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