\begin{document}$ \mu^\pm \mu^\pm \rightarrow e^\pm e^\pm $\end{document} and \begin{document}$ \mu^\pm \mu^\pm \rightarrow \tau^\pm \tau^\pm $\end{document} and leptonic di-number violation (LNV) processes \begin{document}$ \mu^\pm \mu^\pm \rightarrow W^\pm _iW^\pm _j $\end{document} (\begin{document}$ i,\;j=1,\;2 $\end{document}) at same-sign high energy \begin{document}$ \mu^\pm \mu^\pm $\end{document} colliders are studied. The new physics (NP) factors that may play roles in these processes are highlighted by cataloging them into three types. Taking into account the experimental constraints, the processes at \begin{document}$ \mu^\pm\mu^\pm $\end{document} colliders are computed, and the results are presented properly. The results lead to the conclusion that observing the NP factors through the LFV and LNV processes at TeV-energy \begin{document}$ \mu^\pm\mu^\pm $\end{document} colliders has significant advantages that cannot be achieved elsewhere. Therefore, once the techniques for muon acceleration and collision are developed successfully, the option of building same-sign high energy muon colliders should be seriously considered."> Leptonic di-flavor and di-number violation processes at high energy <inline-formula><tex-math id="M1">\begin{document}${{ {\boldsymbol\mu}^{\bf\pm}}{\boldsymbol\mu}^{\bf\pm}} $\end{document}</tex-math><alternatives><graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="//www.macurncorp.com/hepnp/article/app/id/15f9781c-3e5c-4b58-9741-e71043c5f223/CPC-2023-0177_M1.jpg"/><graphic xmlns:xlink="http://www.w3.org/1999/xlink" xlink:href="//www.macurncorp.com/hepnp/article/app/id/15f9781c-3e5c-4b58-9741-e71043c5f223/CPC-2023-0177_M1.png"/></alternatives></inline-formula> colliders -
  • [1]

    M. Tanabashiet al. (Particle Data Group), Phys. Rev. D98, 030001 (2018)

  • [2]

    J. Schechter and J. W. F. Valle, Phys. Rev. D25, 2951 (1982)

  • [3]

    J. Adamet al. (MEG Collaboration), Phys. Rev. Lett.110, 201801 (2013)

  • [4]

    U. Bellgardtet al. (SINDRUM Collaboration), Nucl. Phys. B299, 1 (1988)

  • [5]

    B. Aubertet al. (BABAR Collaboration), Phys. Rev. Lett.104, 021802 (2010)

  • [6]

    K. Hayasaka, K. Inami, Y. Miyazakiet al., Phys. Lett. B687, 139 (2010)

  • [7]

    J. P. Delahaye, M. Diemoz, K. Longet al., arXiv: 1901.06150

  • [8]

    M. Bogomilovet al. (MICE Collaboration), Nature578(7793), 53 (2020)

  • [9]

    R. K. Ellis, B. Heinemann, J. de Blaset al., arXiv: 1910.11775

  • [10]

    K. Long, D. Lucchesi, M. Palmeret al., Nature Phys.17(3), 289 (2021)

  • [11]

    M. M. Alsharoaet al. (Neutrino Factory and Muon Collider), Phys. Rev. ST Accel. Beams6, 081001 (2003)

  • [12]

    S. Geer, Ann. Rev. Nucl. Part. Sci.59, 347 (2009)

  • [13]

    C. A. Heusch and F. Cuypers, AIP Conf. Proc.352, 219 (1996)

  • [14]

    V. Shiltsev, Mod. Phys. Lett. A25, 567 (2010)

  • [15]

    J. Chen, T. Han, and B. Tweedie, JHEP11, 093 (2017)

  • [16]

    D. Buttazzo, D. Redigolo, F. Salaet al., JHEP11, 144 (2018)

  • [17]

    M. Chiesa, F. Maltoni, L. Mantaniet al., JHEP09, 098 (2020)

  • [18]

    T. Han, Y. Ma, and K. Xie, Phys. Rev. D103, L031301 (2021)

  • [19]

    T. Han, D. Liu, I. Low, and X. Wang, Phys. Rev. D103, 013002 (2021)

  • [20]

    T. Han, Z. Liu, L. T. Wang and X. Wang, Phys. Rev. D103, 075004 (2021)

  • [21]

    P. Asadi, R. Capdevilla, C. Cesarottiet al., JHEP10, 182 (2021)

  • [22]

    R. Ruiz, A. Costantini, F. Maltoniet al., JHEP06, 114 (2022)

  • [23]

    S. Bottaro, D. Buttazzo, M. Costaet al., Eur. Phys. J. C82, 31 (2022)

  • [24]

    M. Cannoni, O. Panella, and S. Kolb, arXiv: hep-ph/0410214

  • [25]

    M. Raidal, Phys. Rev. D57, 2013 (1998)

  • [26]

    M. Cannoni, S. Kolb, and O. Panella, Eur. Phys. J. C28, 375 (2003)

  • [27]

    W. Rodejohann and H. Zhang, Phys. Rev. D83, 073005 (2011)

  • [28]

    T. G. Rizzo, Phys. Lett. B116, 23 (1982)

  • [29]

    D. A. Dicus, D. D. Karatas, and P. Roy, Phys. Rev. D44, 2033 (1991)

  • [30]

    G. Belanger, F. Boudjema, D. Londonet al., Phys. Rev. D53, 6292 (1996)

  • [31]

    B. Ananthanarayan and P. Minkowski, Phys. Lett. B373, 130 (1996)

  • [32]

    J. Gluza and M. Zralek, Phys. Lett. B362, 148 (1995)

  • [33]

    J. Gluza and M. Zralek, Phys. Lett. B372, 259 (1996)

  • [34]

    C. Greub and P. Minkowski, eConfC960625, NEW149 (1996)

  • [35]

    W. Rodejohann, Phys. Rev. D81, 114001 (2010)

  • [36]

    S. Banerjee, P. S. B. Dev, A. Ibarraet al., Phys. Rev. D92, 075002 (2015)

  • [37]

    T. Asaka and T. Tsuyuki, Phys. Rev. D92(9), 094012 (2015)

  • [38]

    K. Wang, T. Xu, and L. Zhang, Phys. Rev. D95(7), 075021 (2017)

  • [39]

    P. Bandyopadhyay and A. Karan, arXiv: 2011.04191

  • [40]

    D. London, G. Belanger, and J. N. Ng, Phys. Lett. B188, 155 (1987)

  • [41]

    J. Gluza and M. Zralek, Phys. Rev. D52, 6238 (1995)

  • [42]

    P. Helde, K. Huitu, J. Maalampiet al., Nucl. Phys. B437, 305 (1995)

  • [43]

    J. Barry, L. Dorame, and W. Rodejohann, Eur. Phys. J. C72, 2023 (2012)

  • [44]

    J. L. Yang, C. H. Chang, and T. F. Feng, Commun. Theor. Phys.74, 085202 (2022)

  • [45]

    S. Khalil and H. Okada, Phys. Rev. D79, 083510 (2009)

  • [46]

    A. Elsayed, S. Khalil, and S. Moretti, Phys. Lett. B715, 208 (2012)

  • [47]

    S. Khalil and S. Moretti, Rept. Prog. Phys.80, 036201 (2017)

  • [48]

    J. L. Yang, H. B. Zhang, C. X. Liuet al., JHEP08, 086 (2021)

  • [49]

    P. Duka, J. Gluza, and M. Zralek, Annals Phys.280, 336 (2000)

  • [50]

    P. S. B. Dev, R. N. Mohapatra, and Y. Zhang, JHEP05, 174 (2016)

  • [51]

    S. Patra, F. S. Queiroz, and W. Rodejohann, Phys. Lett. B752, 186 (2016)

  • [52]

    M. Mitra, R. Ruiz, D. J. Scottet al., Phys. Rev. D94, 095016 (2016)

  • [53]

    A. Maiezza, G. Senjanovic, and J. C. Vasquez, Phys. Rev. D95, 095004 (2017)

  • [54]

    R. Mohapatra and A. Smirnov, Ann. Rev. Nucl. Part. Sci.56, 569 (2006)

  • [55]

    R. Mohapatraet al., Rept. Prog. Phys.70, 1757 (2007)

  • [56]

    R. N. Mohapatra and G. Senjanovic, Phys. Rev. Lett.44, 912 (1980)

  • [57]

    J. Schechter and J. W. F. Valle, Phys. Rev. D22, 2227 (1980)

  • [58]

    T. P. Cheng and L. F. Li, Phys. Rev. D22, 2860 (1980)

  • [59]

    G. Lazarides, Q. Shafi, and C. Wetterich, Nucl. Phys. B181, 287 (1981)

  • [60]

    P. S. Bhupal Dev, S. Goswami, and M. Mitra, Phys. Rev. D91, 113004 (2015)

  • [61]

    A. Denner, arXiv: 0709.1075

  • [62]

    T. Hahn and M. Perez-Victoria, Comput. Phys. Commun.118, 153 (1999)

  • [63]

    I. Esteban, M. Gonzalez-Garcia, A. Hernandez-Cabezudoet al., JHEP01, 106 (2019)

  • [64]

    A. M. Sirunyanet al. (CMS Collaboration), Phys. Rev. Lett.120, (2018)

  • [65]

    G. Aadet al. (ATLAS Collaboration), JHEP10, 265 (2019)

  • [66]

    A. M. Sirunyanet al. (CMS Collaboration), JHEP2019, 122 (2019)

  • [67]

    B. Fuks, J. Neundorf, K. Peterset al., Phys. Rev. D103(5), 055005 (2021)

  • [68]

    A. M. Sirunyanet al. (CMS Collaboration), JHEP2017, 121 (2017)

  • [69]

    A. M. Sirunyanet al. (CMS Collaboration), JHEP2018, 148 (2018)

  • [70]

    M. Aaboudet al. (ATLAS Collaboration), JHEP01, 016 (2019)

  • [71]

    M. Aaboudet al. (ATLAS Collaboration), Phys. Lett. B798, 134942 (2019)

  • [72]

    ATLAS Collaboration, ATLAS-CONF-2017-053.

  • [73]

    CMS Collaboration, CMS-PAS-HIG-16-036.

  • [74]

    W. Y. Keung and W. J. Marciano, Phys. Rev. D30, 248 (1984)

  • [75]

    R. N. Cahn, Rept. Prog. Phys.52, 389 (1989)

  • [76]

    A. Djouadi, J. Kalinowski, and P. M. Zerwas, Z. Phys. C70, 435 (1996)

  • [77]

    M. Aoki, S. Kanemura, and K. Yagyu, Phys. Rev. D85, 055007 (2012)

  • [78]

    L. Willmann, P. V. Schmidt, H. P. Wirtzet al., Phys. Rev. Lett.82, 49 (1999)

  • [79]

    J. Alwall, R. Frederix, S. Frixioneet al., JHEP07, 079 (2014)

  • [80]

    P. Li, Z. Liu, and K. F. Lyu, JHEP03, 231 (2023)

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