- Open Access
Searching for leptophilic composite asymmetric dark sector at colliders
Phys. Rev. D 112, 095027 – Published 19 November, 2025
DOI: https://doi.org/10.1103/xsmv-f97b
Abstract
Composite asymmetric dark matter (ADM) models provide a well-motivated paradigm that simultaneously explains dark matter (DM) relic density and matter-antimatter asymmetry. In these models, the mass of the DM candidate (the lightest dark baryon) is generated through the dark confinement scale dynamics. Although the leptophilic composite ADM model offers a viable framework, comprehensive studies of its collider phenomenology are absent. This work systematically explores novel signatures from the leptophilic composite asymmetric dark sector at both low-energy and high-energy colliders as well as other existing collider constraints. We demonstrate detectability of TeV-scale mediators along with sub-GeV to GeV-scale lightest dark mesons at Belle II and its proposed far detector, GAZELLE, as well as Circular Electron Positron Collider/Future Circular Collider-electron-positron experiments. Moreover, these experiments exhibit complementary coverage of the model parameter space.
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References (78)
- M. Battaglieri, A. Belloni, A. Chou, P. Cushman, B. Echenard, R. Essig, J. Estrada, J. L. Feng, B. Flaugher, P. J. Fox et al., arXiv:1707.04591.
- T. Lin, Proc. Sci., 333 (2019) 009 [arXiv:1904.07915].
- E. G. M. Ferreira, Astron. Astrophys. Rev. 29, 7 (2021).
- A. Belenchia, M. Carlesso, Ö. Bayraktar, D. Dequal, I. Derkach, G. Gasbarri, W. Herr, Y. L. Li, M. Rademacher, J. Sidhu et al., Phys. Rep. 951, 1 (2022).
- G. Arcadi, M. Dutra, P. Ghosh, M. Lindner, Y. Mambrini, M. Pierre, S. Profumo, and F. S. Queiroz, Eur. Phys. J. C 78, 203 (2018).
- G. Arcadi, D. Cabo-Almeida, M. Dutra, P. Ghosh, M. Lindner, Y. Mambrini, J. P. Neto, M. Pierre, S. Profumo, and F. S. Queiroz, Eur. Phys. J. C 85, 152 (2025).
- Y. Hochberg, E. Kuflik, T. Volansky, and J. G. Wacker, Phys. Rev. Lett. 113, 171301 (2014).
- J. L. Feng and J. Kumar, Phys. Rev. Lett. 101, 231301 (2008).
- K. Petraki and R. R. Volkas, Int. J. Mod. Phys. A 28, 1330028 (2013).
- K. M. Zurek, Phys. Rep. 537, 91 (2014).
- N. Bernal, M. Heikinheimo, T. Tenkanen, K. Tuominen, and V. Vaskonen, Int. J. Mod. Phys. A 32, 1730023 (2017).
- M. Baryakhtar, L. Rosenberg, and G. Rybka, arXiv:2504.10607.
- P. Villanueva-Domingo, O. Mena, and S. Palomares-Ruiz, Front. Astron. Space Sci. 8, 87 (2021).
- A. D. Sakharov, Pis’ma Zh. Eksp. Teor. Fiz. 5, 32 (1967).
- D. Bodeker and W. Buchmuller, Rev. Mod. Phys. 93, 3 (2021).
- S. Davidson, E. Nardi, and Y. Nir, Phys. Rep. 466, 105 (2008).
- I. Affleck and M. Dine, Nucl. Phys. B249, 361 (1985).
- S. I. Blinnikov and M. Y. Khlopov, Sov. J. Nucl. Phys. 36, 472 (1982).
- S. I. Blinnikov and M. Khlopov, Sov. Astron. 27, 371 (1983).
- M. Y. Khlopov, G. M. Beskin, N. E. Bochkarev, L. A. Pustylnik, and S. A. Pustylnik, Sov. Astron. 35, 21 (1991).
- D. S. M. Alves, S. R. Behbahani, P. Schuster, and J. G. Wacker, Phys. Lett. B 692, 323 (2010).
- D. Spier Moreira Alves, S. R. Behbahani, P. Schuster, and J. G. Wacker, J. High Energy Phys. 06 (2010) 113.
- Y. Bai and P. Schwaller, Phys. Rev. D 89, 063522 (2014).
- M. Ibe, A. Kamada, S. Kobayashi, and W. Nakano, J. High Energy Phys. 11 (2018) 203.
- M. Ibe, A. Kamada, S. Kobayashi, T. Kuwahara, and W. Nakano, J. High Energy Phys. 03 (2019) 173.
- M. Ibe, A. Kamada, S. Kobayashi, T. Kuwahara, and W. Nakano, Phys. Rev. D 100, 075022 (2019).
- E. Hall, T. Konstandin, R. McGehee, and H. Murayama, Phys. Rev. D 107, 055011 (2023).
- M. Zhang, Phys. Rev. D 104, 055008 (2021).
- S. Bottaro, M. Costa, and O. Popov, J. High Energy Phys. 11 (2021) 055.
- M. Ibe, S. Kobayashi, and K. Watanabe, J. High Energy Phys. 07 (2021) 220.
- A. C. Ritter and R. R. Volkas, Phys. Rev. D 107, 015029 (2023).
- P. Schwaller, D. Stolarski, and A. Weiler, J. High Energy Phys. 05 (2015) 059.
- T. Cohen, M. Lisanti, and H. K. Lou, Phys. Rev. Lett. 115, 171804 (2015).
- T. Cohen, M. Lisanti, H. K. Lou, and S. Mishra-Sharma, J. High Energy Phys. 11 (2017) 196.
- M. Park and M. Zhang, Phys. Rev. D 100, 115009 (2019).
- S. Renner and P. Schwaller, J. High Energy Phys. 08 (2018) 052.
- H. Mies, C. Scherb, and P. Schwaller, J. High Energy Phys. 04 (2021) 049.
- D. Linthorne and D. Stolarski, Phys. Rev. D 104, 035019 (2021).
- P. Archer-Smith, D. Linthorne, and D. Stolarski, J. High Energy Phys. 02 (2022) 027.
- J. Carrasco and J. Zurita, J. High Energy Phys. 01 (2024) 034.
- A. Carmona, F. Elahi, C. Scherb, and P. Schwaller, J. High Energy Phys. 06 (2025) 198.
- W. Liu, J. Lockyer, and S. Kulkarni, Phys. Rev. D 112, 075029 (2025).
- G. Aad et al. (ATLAS Collaboration), Eur. Phys. J. C 80, 123 (2020).
- A. M. Sirunyan et al. (CMS Collaboration), J. High Energy Phys. 04 (2021) 123.
- A. Tumasyan et al. (CMS Collaboration), Phys. Rev. D 108, 012011 (2023).
- A. Hayrapetyan et al. (CMS Collaboration), Phys. Rev. D 109, 112001 (2024).
- G. Aad et al. (ATLAS Collaboration), J. High Energy Phys. 05 (2024) 150.
- P. J. Fox, R. Harnik, J. Kopp, and Y. Tsai, Phys. Rev. D 84, 014028 (2011).
- E. Bernreuther, K. Böse, T. Ferber, C. Hearty, F. Kahlhoefer, A. Morandini, and K. Schmidt-Hoberg, J. High Energy Phys. 12 (2022) 005.
- Z. Liu, Y. H. Xu, and Y. Zhang, J. High Energy Phys. 06 (2019) 009.
- A. Alloul, N. D. Christensen, C. Degrande, C. Duhr, and B. Fuks, Comput. Phys. Commun. 185, 2250 (2014).
- 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.
- J. Fiaschi and M. Klasen, J. High Energy Phys. 03 (2018) 094.
- B. Fuks, M. Klasen, D. R. Lamprea, and M. Rothering, J. High Energy Phys. 01 (2014) 168.
- G. Aad et al. (ATLAS Collaboration), J. High Energy Phys. 06 (2023) 153.
- D. Lindley, Astrophys. J. 294, 1 (1985).
- P. S. B. Dev, Q. f. Wu, and X. J. Xu, arXiv:2507.12270.
- T. Sjöstrand, S. Ask, J. R. Christiansen, R. Corke, N. Desai, P. Ilten, S. Mrenna, S. Prestel, C. O. Rasmussen, and P. Z. Skands, Comput. Phys. Commun. 191, 159 (2015).
- S. Knapen, J. Shelton, and D. Xu, Phys. Rev. D 103, 115013 (2021).
- A. Berlin, N. Blinov, S. Gori, P. Schuster, and N. Toro, Phys. Rev. D 97, 055033 (2018).
- S. M. Choi, H. M. Lee, P. Ko, and A. Natale, Phys. Rev. D 98, 015034 (2018).
- T. Kuwahara and S. R. Yuan, J. High Energy Phys. 06 (2023) 208.
- E. Bernreuther, N. Hemme, F. Kahlhoefer, and S. Kulkarni, Phys. Rev. D 110, 035009 (2024).
- J. P. Lees et al. (BABAR Collaboration), Phys. Rev. Lett. 114, 171801 (2015).
- D. Boutigny et al. (BABAR Collaboration), Report No. SLAC-R-0457.
- M. Duerr, T. Ferber, C. Garcia-Cely, C. Hearty, and K. Schmidt-Hoberg, J. High Energy Phys. 04 (2021) 146.
- I. Adachi, T.E. Browder, P. Križan, S. Tanaka, and Y. Ushiroda (Belle-II Collaboration), Nucl. Instrum. Methods Phys. Res., Sect. A 907, 46 (2018).
- D. W. Kang, P. Ko, and C. T. Lu, J. High Energy Phys. 04 (2021) 269.
- P. Ko, Y. Kwon, C. T. Lu, and X. Wei, J. High Energy Phys. 08 (2025) 150.
- F. Domingo, J. Günther, J. S. Kim, and Z. S. Wang, Eur. Phys. J. C 84, 642 (2024).
- M. Cacciari, G. P. Salam, and G. Soyez, J. High Energy Phys. 04 (2008) 063.
- M. Cacciari, G. P. Salam, and G. Soyez, Eur. Phys. J. C 72, 1896 (2012).
- J. B. Guimarães da Costa et al. (CEPC Study Group Collaboration), arXiv:1811.10545.
- R. Aaij et al. (LHCb Collaboration), J. High Energy Phys. 10 (2020) 156.
- A. Hayrapetyan et al. (CMS Collaboration), J. High Energy Phys. 12 (2023) 070.
- S. Born, R. Karur, S. Knapen, and J. Shelton, Phys. Rev. D 108, 035034 (2023).
- M. Abbrescia et al. (IDEA Study Group Collaboration), arXiv:2502.21223.
- S. Braibant and P. Giacomelli, Eur. Phys. J. Plus 136, 1143 (2021).