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  • Open Access

Heavy neutral lepton at same-sign muon collider

Ryuichiro Kitano1,*, Ian Low2,3,†, Ryutaro Matsudo1,‡, Shohei Okawa1,4,5,§, and Subhojit Roy3,∥

  • *Contact author: ryuichiro.kitano@yukawa.kyoto-u.ac.jp
  • †Contact author: ilow@northwestern.edu
  • ‡Contact author: matsudo@post.kek.jp
  • §Contact author: shohei.okawa@apctp.org
  • ∥Contact author: sroy@anl.gov

Phys. Rev. D 114, 055006 – Published 9 September, 2026

DOI: https://doi.org/10.1103/prx6-wnwr

Abstract

We explore the discovery potential of heavy neutral leptons (HNLs), motivated by models addressing the origin of neutrino masses, at the proposed high-energy same-sign muon collider known as μTRISTAN. The study focuses on two complementary HNL-mediated signatures: (i) the lepton-flavor-violating (LFV) channel μ+μ+→W+τ+ν¯μ and (ii) the lepton-number-violating (LNV) channel μ+μ+→W+W+. The LNV process is the muon analogue of inverse neutrinoless double beta decay and, if observed, would provide strong evidence for Majorana neutrinos, while the LFV process offers a novel probe of flavor-changing neutral currents in the lepton sector. At the μTRISTAN collider with s∼O(10)  TeV, the resulting sensitivity to the HNL mixing with muon and tau neutrinos, as a function of mass, can surpass current bounds from the measurements of electroweak precision observables over a broad mass range. In particular, for the mixing with muon neutrinos, the collider bound can improve by an order of magnitude for 5–10 TeV HNLs.

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References (98)

  1. G. Aad et al. (ATLAS Collaboration), Phys. Lett. B 716, 1 (2012).
  2. S. Chatrchyan et al. (CMS Collaboration), Phys. Lett. B 716, 30 (2012).
  3. M. Benedikt et al. (FCC Collaboration), Eur. Phys. J. C 85, 1468 (2025).
  4. T. Behnke et al., arXiv:1306.6327.
  5. C. Adolphsen et al., arXiv:1306.6353.
  6. C. Adolphsen et al., arXiv:1306.6328.
  7. P. Bambade et al., arXiv:1903.01629.
  8. A. F. Zarnecki (CLICdp, ILD Concept Group Collaborations), Proc. Sci. CORFU2019 (2020) 037 [arXiv:2004.14628].
  9. H. Abramowicz et al. (Linear Collider Collaboration), arXiv:2503.24049.
  10. M. Aicheler, P. N. Burrows, N. Catalan, R. Corsini, M. Draper, J. Osborne, D. Schulte, S. Stapnes, and M. J. Stuart, arXiv:1903.08655.
  11. C. Vernieri et al., J. Instrum. 18, P07053 (2023).
  12. M. Breidenbach, B. Bullard, E. A. Nanni, D. Ntounis, and C. Vernieri, PRX Energy 2, 047001 (2023); 4, 029901(E) (2025).
  13. C. A. Lindstrøm, R. D’Arcy, and B. Foster, J. Phys. Conf. Ser. 3124, 012001 (2025).
  14. B. Foster, R. D’Arcy, and C. A. Lindstrom, New J. Phys. 25, 093037 (2023).
  15. M. Dong et al. (CEPC Study Group Collaboration), arXiv:1811.10545.
  16. C. Anastopoulos et al., J. Phys. G 53, 040501 (2026).
  17. C. Accettura et al., Eur. Phys. J. C 83, 864 (2023); 84, 36(E) (2024).
  18. C. A. Heusch and F. Cuypers, AIP Conf. Proc. 352, 219 (1996).
  19. M. Antonelli, M. Boscolo, R. Di Nardo, and P. Raimondi, Nucl. Instrum. Methods Phys. Res., Sect. A 807, 101 (2016).
  20. K. Long, D. Lucchesi, M. Palmer, N. Pastrone, D. Schulte, and V. Shiltsev, Nat. Phys. 17, 289 (2021).
  21. J. P. Delahaye, M. Diemoz, K. Long, B. Mansoulié, N. Pastrone, L. Rivkin, D. Schulte, A. Skrinsky, and A. Wulzer, arXiv:1901.06150.
  22. D. Stratakis et al. (Muon Collider Collaboration), arXiv:2203.08033.
  23. M. Begel et al., arXiv:2503.23695.
  24. Y. Kondo et al., in 9th International Particle Accelerator Conference (2018), 10.18429/JACoW-IPAC2018-FRXGBF1.
  25. S. Aritome et al., Phys. Rev. Lett. 134, 245001 (2025).
  26. G. Belanger, F. Boudjema, D. London, and H. Nadeau, Phys. Rev. D 53, 6292 (1996).
  27. J. Gluza and M. Zralek, Phys. Lett. B 362, 148 (1995).
  28. K. Fridell, R. Kitano, and R. Takai, J. High Energy Phys. 06 (2023) 086.
  29. H. Fukuda, T. Moroi, A. Niki, and S.-F. Wei, J. High Energy Phys. 02 (2024) 214.
  30. A. Das and Y. Orikasa, Phys. Lett. B 851, 138577 (2024).
  31. J. Kriewald, E. Pinsard, and A. M. Teixeira, J. High Energy Phys. 02 (2025) 116.
  32. C. H. de Lima, D. McKeen, J. N. Ng, M. Shamma, and D. Tuckler, Phys. Rev. D 111, 075002 (2025).
  33. Y. Hamada, R. Kitano, R. Matsudo, H. Takaura, and M. Yoshida, Prog. Theor. Exp. Phys. 2022, 053B02 (2022).
  34. A. Das, J. Li, S. Mandal, T. Nomura, and R. Zhang, Phys. Rev. D 112, 035008 (2025).
  35. P. A. Zyla et al. (Particle Data Group Collaboration), Prog. Theor. Exp. Phys. 2020, 083C01 (2020).
  36. P. Minkowski, Phys. Lett. 67B, 421 (1977).
  37. T. Yanagida, Conf. Proc. C 7902131, 95 (1979).
  38. S. L. Glashow, NATO Sci. Ser. B 61, 687 (1980).
  39. M. Gell-Mann, P. Ramond, and R. Slansky, Conf. Proc. C 790927, 315 (1979).
  40. R. N. Mohapatra and G. Senjanovic, Phys. Rev. Lett. 44, 912 (1980).
  41. E. K. Akhmedov, M. Lindner, E. Schnapka, and J. W. F. Valle, Phys. Rev. D 53, 2752 (1996).
  42. S. M. Barr, Phys. Rev. Lett. 92, 101601 (2004).
  43. M. Malinsky, J. C. Romao, and J. W. F. Valle, Phys. Rev. Lett. 95, 161801 (2005).
  44. J. Schechter and J. W. F. Valle, Phys. Rev. D 22, 2227 (1980).
  45. M. Gronau, C. N. Leung, and J. L. Rosner, Phys. Rev. D 29, 2539 (1984).
  46. R. N. Mohapatra and J. W. F. Valle, Phys. Rev. D 34, 1642 (1986).
  47. F. F. Deppisch, P. S. Bhupal Dev, and A. Pilaftsis, New J. Phys. 17, 075019 (2015).
  48. P. D. Bolton, F. F. Deppisch, and P. S. Bhupal Dev, J. High Energy Phys. 03 (2020) 170.
  49. A. M. Sirunyan et al. (CMS Collaboration), Phys. Rev. Lett. 120, 221801 (2018).
  50. A. Tumasyan et al. (CMS Collaboration), Phys. Rev. Lett. 131, 011803 (2023).
  51. A. Tumasyan et al. (CMS Collaboration), J. High Energy Phys. 07 (2022) 081.
  52. T. G. Rizzo, Phys. Lett. B 116, 23 (1982).
  53. W. Tornow (KamLAND-Zen Collaboration), in 34th International Symposium on Physics in Collision (2014), arXiv:1412.0734.
  54. G. Anton et al. (EXO-200 Collaboration), Phys. Rev. Lett. 123, 161802 (2019).
  55. M. Agostini et al. (GERDA Collaboration), Phys. Rev. Lett. 125, 252502 (2020).
  56. D. Q. Adams et al. (CUORE Collaboration), Nature (London) 604, 53 (2022).
  57. S. Abe et al. (KamLAND-Zen Collaboration), Phys. Rev. Lett. 130, 051801 (2023).
  58. W. Rodejohann, Phys. Rev. D 81, 114001 (2010).
  59. R. Jiang, T. Yang, S. Qian, Y. Ban, J. Li, Z. You, and Q. Li, Phys. Rev. D 109, 035020 (2024).
  60. J.-L. Yang, C.-H. Chang, and T.-F. Feng, Chin. Phys. C 48, 043101 (2024).
  61. P. Dehghani, M. Frank, and B. Fuks, Phys. Rev. D 112, 035020 (2025).
  62. P. S. B. Dev, J. Heeck, and A. Thapa, Eur. Phys. J. C 84, 148 (2024).
  63. T. Han, A. Ibarra, S. Roy, and M. Sabová, arXiv:2608.10062.
  64. S. Weinberg, Phys. Rev. Lett. 43, 1566 (1979).
  65. R. Foot, H. Lew, X. G. He, and G. C. Joshi, Z. Phys. C 44, 441 (1989).
  66. E. Ma, Phys. Rev. Lett. 81, 1171 (1998).
  67. T. Asaka and M. Shaposhnikov, Phys. Lett. B 620, 17 (2005).
  68. K. Bondarenko, A. Boyarsky, D. Gorbunov, and O. Ruchayskiy, J. High Energy Phys. 11 (2018) 032.
  69. A. M. Abdullahi et al., J. Phys. G 50, 020501 (2023).
  70. M. Fukugita and T. Yanagida, Phys. Lett. B 174, 45 (1986).
  71. M. Fukugita and T. Yanagida, Phys. Rev. Lett. 89, 131602 (2002).
  72. A. Boyarsky, O. Ruchayskiy, and M. Shaposhnikov, Annu. Rev. Nucl. Part. Sci. 59, 191 (2009).
  73. S. Davidson, E. Nardi, and Y. Nir, Phys. Rep. 466, 105 (2008).
  74. A. Granelli, D. Meloni, M. Parriciatu, J. T. Penedo, and S. T. Petcov, J. High Energy Phys. 12 (2025) 035.
  75. F. del Aguila, J. de Blas, and M. Perez-Victoria, Phys. Rev. D 78, 013010 (2008).
  76. E. Akhmedov, A. Kartavtsev, M. Lindner, L. Michaels, and J. Smirnov, J. High Energy Phys. 05 (2013) 081.
  77. J. de Blas, EPJ Web Conf. 60, 19008 (2013).
  78. L. Basso, O. Fischer, and J. J. van der Bij, Europhys. Lett. 105, 11001 (2014).
  79. S. Antusch and O. Fischer, J. High Energy Phys. 10 (2014) 094.
  80. S. Antusch and O. Fischer, J. High Energy Phys. 05 (2015) 053.
  81. M. Chrzaszcz, M. Drewes, T. E. Gonzalo, J. Harz, S. Krishnamurthy, and C. Weniger, Eur. Phys. J. C 80, 569 (2020).
  82. D. Bryman, V. Cirigliano, A. Crivellin, and G. Inguglia, Annu. Rev. Nucl. Part. Sci. 72, 69 (2022).
  83. M. Blennow, E. Fernández-Martínez, J. Hernández-García, J. López-Pavón, X. Marcano, and D. Naredo-Tuero, J. High Energy Phys. 08 (2023) 030.
  84. J. C. Gallardo et al., eConf C 960625, R4 (1996).
  85. C. M. Ankenbrandt et al., Phys. Rev. ST Accel. Beams 2, 081001 (1999).
  86. D. London, G. Belanger, and J. N. Ng, Phys. Lett. B 188, 155 (1987).
  87. C. A. Heusch and P. Minkowski, Nucl. Phys. B416, 3 (1994).
  88. T. Asaka and T. Tsuyuki, Phys. Rev. D 92, 094012 (2015).
  89. K. Wang, T. Xu, and L. Zhang, Phys. Rev. D 95, 075021 (2017).
  90. J. Alwall, R. Frederix, S. Frixione, V. Hirschi, F. Maltoni, O. Mattelaer, H. S. Shao, T. Stelzer, P. Torrielli, and M. Zaro, J. High Energy Phys. 07 (2014) 079.
  91. A. Alloul, N. D. Christensen, C. Degrande, C. Duhr, and B. Fuks, Comput. Phys. Commun. 185, 2250 (2014).
  92. T. Sjostrand, S. Mrenna, and P. Z. Skands, J. High Energy Phys. 05 (2006) 026.
  93. T. Sjostrand, S. Mrenna, and P. Z. Skands, Comput. Phys. Commun. 178, 852 (2008).
  94. J. de Favereau, C. Delaere, P. Demin, A. Giammanco, V. Lemaître, A. Mertens, and M. Selvaggi (delphes 33 Collaboration), J. High Energy Phys. 02 (2014) 057.
  95. Y. Hamada, R. Kitano, R. Matsudo, S. Okawa, R. Takai, H. Takaura, and L. Treuer, Phys. Rev. D 110, 113011 (2024).
  96. K. Harigaya, R. Kitano, and R. Takai, J. High Energy Phys. 04 (2026) 085.
  97. C. F. von Weizsacker, Z. Phys. 88, 612 (1934).
  98. E. J. Williams, Phys. Rev. 45, 729 (1934).

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