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Reviving portal dark matter with conversion mechanism
Phys. Rev. D 113, 115016 – Published 8 June, 2026
DOI: https://doi.org/10.1103/k7xm-mygl
Abstract
In many new physics models with extended gauge symmetry, the new gauge boson could mediate the interactions between the dark matter and standard model particles. For the conventional portal dark matter, the collider and the direct detection constraints typically pose a significant challenge. To address this pressing issue, we present in this paper a new benchmark model based on the gauged symmetry, which introduces a Dirac dark fermion and a heavier partner with zero and nonzero charge, respectively. Including the mass term results in the dark fermions and in the mass eigenstate, where the lighter one is regarded as the dark matter candidate. Various intriguing processes for the relic density arise with the compressed mass spectrum , such as the coscattering , the conversion , and the coannihilation processes. Suppressed by the small mixing angle between the dark fermions, the small effective gauge coupling of dark matter to the gauge boson is one distinct feature of this model, rendering phenomenology in many aspects more promising. In this paper, we investigate the production of dark matter through new mechanisms within the frameworks of resonance and secluded scenarios. The impacts of phenomenological constraints from colliders, dark matter, and cosmology are also taken into account. We report that the conversion mechanism is both favored by the resonance and secluded scenarios under current constraints.
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References (111)
- G. Bertone, D. Hooper, and J. Silk, Phys. Rep. 405, 279 (2005).
- M. Cirelli, A. Strumia, and J. Zupan, arXiv:2406.01705.
- A. De Simone and T. Jacques, Eur. Phys. J. C 76, 367 (2016).
- 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).
- Y. Bai and J. Berger, J. High Energy Phys. 11 (2013) 171.
- Y. Bai and J. Berger, J. High Energy Phys. 08 (2014) 153.
- M. Escudero, N. Rius, and V. Sanz, Eur. Phys. J. C 77, 397 (2017).
- M. Blennow, E. Fernandez-Martinez, A. Olivares-Del Campo, S. Pascoli, S. Rosauro-Alcaraz, and A. V. Titov, Eur. Phys. J. C 79, 555 (2019).
- L. Coito, C. Faubel, J. Herrero-García, A. Santamaria, and A. Titov, J. High Energy Phys. 08 (2022) 085.
- S. P. Li and X. J. Xu, J. Cosmol. Astropart. Phys. 06 (2023) 047.
- B. Patt and F. Wilczek, arXiv:hep-ph/0605188.
- J. March-Russell, S. M. West, D. Cumberbatch, and D. Hooper, J. High Energy Phys. 07 (2008) 058.
- N. Okada and O. Seto, Phys. Rev. D 82, 023507 (2010).
- A. Djouadi, O. Lebedev, Y. Mambrini, and J. Quevillon, Phys. Lett. B 709, 65 (2012).
- J. M. Cline, K. Kainulainen, P. Scott, and C. Weniger, Phys. Rev. D 88, 055025 (2013); 92, 039906(E) (2015).
- G. Arcadi, A. Djouadi, and M. Raidal, Phys. Rep. 842, 1 (2020).
- A. Alves, S. Profumo, and F. S. Queiroz, J. High Energy Phys. 04 (2014) 063.
- F. D’Eramo, B. J. Kavanagh, and P. Panci, J. High Energy Phys. 08 (2016) 111.
- S. Okada, Adv. High Energy Phys. 2018, 5340935 (2018).
- C. Blanco, M. Escudero, D. Hooper, and S. J. Witte, J. Cosmol. Astropart. Phys. 11 (2019) 024.
- P. J. Fitzpatrick, H. Liu, T. R. Slatyer, and Y. D. Tsai, Phys. Rev. D 106, 083517 (2022).
- R. N. Mohapatra and R. E. Marshak, Phys. Rev. Lett. 44, 1316 (1980); 44, 1643(E) (1980).
- P. Minkowski, Phys. Lett. 67B, 421 (1977).
- R. N. Mohapatra and G. Senjanovic, Phys. Rev. Lett. 44, 912 (1980).
- J. Schechter and J. W. F. Valle, Phys. Rev. D 22, 2227 (1980).
- J. Schechter and J. W. F. Valle, Phys. Rev. D 25, 774 (1982).
- M. Fukugita and T. Yanagida, Phys. Lett. B 174, 45 (1986).
- S. Davidson, E. Nardi, and Y. Nir, Phys. Rep. 466, 105 (2008).
- S. Iso, N. Okada, and Y. Orikasa, Phys. Rev. D 83, 093011 (2011).
- P. S. B. Dev, R. N. Mohapatra, and Y. Zhang, J. High Energy Phys. 03 (2018) 122.
- A. Das and Y. Orikasa, Phys. Lett. B 864, 139395 (2025).
- N. Okada and Y. Orikasa, Phys. Rev. D 85, 115006 (2012).
- T. Basak and T. Mondal, Phys. Rev. D 89, 063527 (2014).
- M. Escudero, N. Rius, and V. Sanz, J. High Energy Phys. 02 (2017) 045.
- A. Das, S. Goswami, K. N. Vishnudath, and T. Nomura, Phys. Rev. D 101, 055026 (2020).
- A. Liu, F. L. Shao, Z. L. Han, Y. Jin, and H. Li, J. High Energy Phys. 10 (2024) 019.
- J. Abdallah, H. Araujo, A. Arbey, A. Ashkenazi, A. Belyaev, J. Berger, C. Boehm, A. Boveia, A. Brennan, and J. Brooke et al., Phys. Dark Universe 9–10, 8 (2015).
- M. Klasen, F. Lyonnet, and F. S. Queiroz, Eur. Phys. J. C 77, 348 (2017).
- P. Agnes et al. (DarkSide-50 Collaboration), Eur. Phys. J. C 83, 322 (2023).
- Z. Bo et al. (PandaX Collaboration), Phys. Rev. Lett. 134, 011805 (2025).
- J. Aalbers et al. (LZ Collaboration), Phys. Rev. Lett. 135, 011802 (2025).
- J. P. Lees et al. (BABAR Collaboration, Phys. Rev. Lett. 113, 201801 (2014).
- J. P. Lees et al. (BABAR Collaboration, Phys. Rev. Lett. 119, 131804 (2017).
- R. Aaij et al. (LHCb Collaboration), Phys. Rev. Lett. 120, 061801 (2018).
- R. Aaij et al. (LHCb Collaboration), Phys. Rev. Lett. 124, 041801 (2020).
- G. Aad et al. (ATLAS Collaboration), Phys. Lett. B 796, 68 (2019).
- N. Nath, N. Okada, S. Okada, D. Raut, and Q. Shafi, Eur. Phys. J. C 82, 864 (2022).
- R. N. Mohapatra and N. Okada, Phys. Rev. D 102, 035028 (2020).
- D. Tucker-Smith and N. Weiner, Phys. Rev. D 64, 043502 (2001).
- A. Filimonova, S. Junius, L. Lopez Honorez, and S. Westhoff, J. High Energy Phys. 06 (2022) 048.
- A. L. Foguel, P. Reimitz, and R. Z. Funchal, J. High Energy Phys. 05 (2025) 001.
- J. J. Zhang, Z. L. Han, A. Liu, and F. L. Shao, Nucl. Phys. B1014, 116864 (2025).
- K. Griest and D. Seckel, Phys. Rev. D 43, 3191 (1991).
- R. T. D’Agnolo, D. Pappadopulo, and J. T. Ruderman, Phys. Rev. Lett. 119, 061102 (2017).
- M. Garny, J. Heisig, B. Lülf, and S. Vogl, Phys. Rev. D 96, 103521 (2017).
- M. Garny, J. Heisig, M. Hufnagel, and B. Lülf, Phys. Rev. D 97, 075002 (2018).
- R. T. D’Agnolo, C. Mondino, J. T. Ruderman, and P. J. Wang, J. High Energy Phys. 08 (2018) 079.
- H. C. Cheng, L. Li, and R. Zheng, J. High Energy Phys. 09 (2018) 098.
- S. Junius, L. Lopez-Honorez, and A. Mariotti, J. High Energy Phys. 07 (2019) 136.
- R. T. D’Agnolo, D. Pappadopulo, J. T. Ruderman, and P. J. Wang, Phys. Rev. Lett. 124, 151801 (2020).
- T. N. Maity and T. S. Ray, Phys. Rev. D 101, 103013 (2020).
- F. Brümmer, J. High Energy Phys. 01 (2020) 113.
- J. Heeck, J. Heisig, and A. Thapa, Phys. Rev. D 107, 015028 (2023).
- J. Heisig, Phys. Rev. Lett. 133, 19 (2024).
- J. Heisig, A. Lessa, and L. M. D. Ramos, Phys. Rev. D 110, 015031 (2024).
- B. Díaz Sáez, J. Lahiri, and K. Möhling, J. Cosmol. Astropart. Phys. 10 (2024) 001.
- B. Díaz Sáez, Phys. Dark Universe 48, 101852 (2025).
- P. K. Paul, S. K. Sahoo, and N. Sahu, J. Cosmol. Astropart. Phys. 10 (2025) 053.
- S. Chatterjee and A. Hryczuk, J. High Energy Phys. 07 (2025) 279.
- A. Liu, Z. L. Han, F. Huang, F. L. Shao, and W. Wang, arXiv:2510.13231.
- P. K. Paul, S. K. Sahoo, and N. Sahu, arXiv:2511.14571.
- G. Alguero, G. Belanger, S. Kraml, and A. Pukhov, SciPost Phys. 13, 124 (2022).
- G. Alguero, G. Belanger, F. Boudjema, S. Chakraborti, A. Goudelis, S. Kraml, A. Mjallal, and A. Pukhov, Comput. Phys. Commun. 299, 109133 (2024).
- Y. D. Tsai, P. deNiverville, and M. X. Liu, Phys. Rev. Lett. 126, 181801 (2021).
- N. Aghanim et al. (Planck Collaboration), Astron. Astrophys. 641, A6 (2020); 652, C4(E) (2021).
- S. K. A., A. Das, G. Lambiase, T. Nomura, and Y. Orikasa, Eur. Phys. J. C 84, 1224 (2024).
- S. Schael et al. (ALEPH, DELPHI, L3, OPAL, and LEP Electroweak Collaborations), Phys. Rep. 532, 119 (2013).
- A. M. Sirunyan et al. (CMS Collaboration), J. High Energy Phys. 07 (2021) 208.
- T. Ferber, C. Garcia-Cely, and K. Schmidt-Hoberg, Phys. Lett. B 833, 137373 (2022).
- M. J. Dolan, T. Ferber, C. Hearty, F. Kahlhoefer, and K. Schmidt-Hoberg, J. High Energy Phys. 12 (2017) 094; 03 (2021) 190(E).
- M. Karliner, M. Low, J. L. Rosner, and L. T. Wang, Phys. Rev. D 92, 035010 (2015).
- P. Agnes et al. (Global Argon Dark Matter Collaboration), Phys. Rev. D 107, 112006 (2023).
- R. Agnese et al. (SuperCDMS Collaboration), Phys. Rev. D 95, 082002 (2017).
- D. S. Akerib et al. (LZ Collaboration), arXiv:1509.02910.
- Y. F. Liang et al. (CDEX Collaboration), Phys. Rev. D 112, 112025 (2025).
- M. Cirelli, N. Fornengo, J. Koechler, E. Pinetti, and B. M. Roach, J. Cosmol. Astropart. Phys. 07 (2023) 026; 08 (2025) E02.
- L. Lopez-Honorez, O. Mena, S. Palomares-Ruiz, and A. C. Vincent, J. Cosmol. Astropart. Phys. 07 (2013) 046.
- T. R. Slatyer, Phys. Rev. D 93, 023527 (2016).
- R. K. Leane, T. R. Slatyer, J. F. Beacom, and K. C. Y. Ng, Phys. Rev. D 98, 023016 (2018).
- K. Dutta, A. Ghosh, A. Kar, and B. Mukhopadhyaya, J. Cosmol. Astropart. Phys. 08 (2023) 071.
- M. Aguilar et al. (AMS Collaboration), Phys. Rev. Lett. 113, 121102 (2014).
- M. Aguilar et al. (AMS Collaboration), Phys. Rev. Lett. 122, 041102 (2019).
- A. Albert et al. (Fermi-LAT and DES Collaborations), Astrophys. J. 834, 110 (2017).
- H. Abdallah et al. (H.E.S.S. Collaboration), Phys. Rev. Lett. 117, 111301 (2016).
- H. Abdalla et al. (H.E.S.S. Collaboration), Phys. Rev. Lett. 129, 111101 (2022).
- R. Caputo et al. (AMEGO Collaboration), arXiv:1907.07558.
- C. A. Kierans (AMEGO Team), Proc. SPIE Int. Soc. Opt. Eng. 11444, 1144431 (2020).
- R. Caputo, M. Ajello, C. A. Kierans, J. S. Perkins, J. L. Racusin, L. Baldini, M. G. Baring, E. Bissaldi, E. Burns, N. Cannady et al., J. Astron. Telesc. Instrum. Syst. 8, 044003 (2022).
- A. De Angelis et al. (e-ASTROGAM Collaboration), Exp. Astron. 44, 25 (2017).
- A. De Angelis et al. (e-ASTROGAM Collaboration), J. High Energy Astrophys. 19, 1 (2018).
- T. Dzhatdoev and E. Podlesnyi, Astropart. Phys. 112, 1 (2019).
- M. Cirelli and A. Kar, SciPost Phys. 19, 080 (2025).
- A. Berlin and F. Kling, Phys. Rev. D 99, 015021 (2019).
- A. Hayrapetyan et al. (CMS Collaboration), Phys. Rev. Lett. 132, 041802 (2024).
- W. Liu and J. Sun, Phys. Rev. D 111, 115022 (2025).
- M. Kawasaki, K. Kohri, T. Moroi, and Y. Takaesu, Phys. Rev. D 97, 023502 (2018).
- M. Lucca, N. Schöneberg, D. C. Hooper, J. Lesgourgues, and J. Chluba, J. Cosmol. Astropart. Phys. 02 (2020) 026.
- T. Hambye, M. Hufnagel, and M. Lucca, J. Cosmol. Astropart. Phys. 05 (2022) 033.
- A. Liu, F. L. Shao, Z. L. Han, Y. Jin, and H. Li, Phys. Rev. D 108, 115028 (2023).
- M. Pospelov, A. Ritz, and M. B. Voloshin, Phys. Lett. B 662, 53 (2008).
- S. Profumo, F. S. Queiroz, J. Silk, and C. Siqueira, J. Cosmol. Astropart. Phys. 03 (2018) 010.