- Letter
- Open Access
- Access by Xinjiang University
Super-Kamiokande strongly constrains leptophilic dark matter capture in the Sun
Phys. Rev. D 113, L101305 – Published 13 May, 2026
DOI: https://doi.org/10.1103/txsw-2kdf
Abstract
The Sun can efficiently capture leptophilic dark matter that scatters with free electrons. If this dark matter subsequently annihilates into leptonic states, it can produce a detectable neutrino flux. Using 10 years of Super-Kamiokande observations, we set constraints on the dark matter–electron scattering cross section that exceed terrestrial direct detection searches by more than an order of magnitude for dark matter masses below 100 GeV and reach cross sections as low as .
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References (132)
- G. Bertone, D. Hooper, and J. Silk, Phys. Rep. 405, 279 (2005).
- G. Bertone and D. Hooper, Rev. Mod. Phys. 90, 045002 (2018).
- M. Cirelli, A. Strumia, and J. Zupan, arXiv:2406.01705.
- Y. Kahn and T. Lin, Rep. Prog. Phys. 85, 066901 (2022).
- S. Knapen, J. Kozaczuk, and T. Lin, Phys. Rev. D 104, 015031 (2021).
- T. Lin, Proc. Sci., 333 (2019) 009 [arXiv:1904.07915].
- C. Blanco, J. I. Collar, Y. Kahn, and B. Lillard, Phys. Rev. D 101, 056001 (2020).
- R. Essig et al., in Snowmass 2021 (2022); arXiv:2203.08297.
- E. Aprile et al. (XENON Collaboration), Eur. Phys. J. C 84, 784 (2024).
- J. Aalbers et al. (LZ Collaboration), Commun. Phys. 7, 292 (2024).
- S. Li et al. (PandaX Collaboration), Phys. Rev. Lett. 130, 261001 (2023).
- J. Bramante and T. Linden, Phys. Rev. Lett. 113, 191301 (2014).
- M. Baryakhtar, J. Bramante, S. W. Li, T. Linden, and N. Raj, Phys. Rev. Lett. 119, 131801 (2017).
- P. J. Fox and E. Poppitz, Phys. Rev. D 79, 083528 (2009).
- G. Bertone, M. Cirelli, A. Strumia, and M. Taoso, J. Cosmol. Astropart. Phys. 03 (2009) 009.
- I. John and T. Linden, Phys. Rev. D 108, 103022 (2023).
- I. John and T. Linden, J. Cosmol. Astropart. Phys. 12 (2021) 007.
- D. Borah, N. Das, S. Jahedi, and B. Thacker, J. High Energy Phys. 01 (2025) 074.
- B. Barman, S. Bhattacharya, S. Girmohanta, and S. Jahedi, J. High Energy Phys. 04 (2022) 146.
- E. Nardi, F. Sannino, and A. Strumia, J. Cosmol. Astropart. Phys. 01 (2009) 043.
- J. F. Acevedo, J. Bramante, A. Goodman, J. Kopp, and T. Opferkuch, J. Cosmol. Astropart. Phys. 04 (2021) 026.
- A. Berlin and D. Hooper, Phys. Rev. D 110, 075018 (2024).
- K.-W. Ng, K. A. Olive, and M. Srednicki, Phys. Lett. B 188, 138 (1987).
- B. Chauhan, M. H. Reno, C. Rott, and I. Sarcevic, J. Cosmol. Astropart. Phys. 01 (2024) 030.
- X. Chu, R. Garani, C. García-Cely, and T. Hambye, J. High Energy Phys. 05 (2024) 045.
- R. Garani and S. Palomares-Ruiz, J. Cosmol. Astropart. Phys. 05 (2017) 007.
- T. N. Maity, A. K. Saha, S. Mondal, and R. Laha, Phys. Rev. D 112, 023025 (2025).
- A. Albert et al. (HAWC Collaboration), Phys. Rev. Lett. 131, 051201 (2023).
- M. U. Nisa, J. F. Beacom, S. Y. BenZvi, R. K. Leane, T. Linden, K. C. Y. Ng, A. H. G. Peter, and B. Zhou, arXiv:1903.06349.
- A. Albert et al. (HAWC Collaboration), Phys. Rev. D 98, 123012 (2018).
- R. Abbasi et al. (IceCube Collaboration), Phys. Rev. D 105, 062004 (2022).
- R. K. Leane, K. C. Y. Ng, and J. F. Beacom, Phys. Rev. D 95, 123016 (2017).
- N. F. Bell, M. J. Dolan, and S. Robles, J. Cosmol. Astropart. Phys. 11 (2021) 004.
- N. F. Bell and K. Petraki, J. Cosmol. Astropart. Phys. 04 (2011) 003.
- N. F. Bell, J. B. Dent, and I. W. Sanderson, Phys. Rev. D 104, 023024 (2021).
- N. F. Bell, A. J. Brennan, and T. D. Jacques, J. Cosmol. Astropart. Phys. 10 (2012) 045.
- C. Niblaeus, A. Beniwal, and J. Edsjo, J. Cosmol. Astropart. Phys. 11 (2019) 011.
- J. Edsjo, J. Elevant, R. Enberg, and C. Niblaeus, J. Cosmol. Astropart. Phys. 06 (2017) 033.
- D. Bose, T. N. Maity, and T. S. Ray, Phys. Rev. D 105, 123013 (2022).
- M. G. Aartsen et al. (IceCube Collaboration), J. Cosmol. Astropart. Phys. 04 (2016) 022.
- J. L. Feng, J. Smolinsky, and P. Tanedo, Phys. Rev. D 93, 115036 (2016); 96, 099903(E) (2017).
- C. Kouvaris, Phys. Rev. D 77, 023006 (2008).
- C. Kouvaris, Phys. Rev. D 92, 075001 (2015).
- C. Kouvaris, K. Langæble, and N. G. Nielsen, J. Cosmol. Astropart. Phys. 10 (2016) 012.
- A. Widmark, J. Cosmol. Astropart. Phys. 05 (2017) 046.
- R. Catena and A. Widmark, J. Cosmol. Astropart. Phys. 12 (2016) 016.
- T. T. Q. Nguyen and T. Linden, arXiv:2602.15113.
- A. Bottino, G. Fiorentini, N. Fornengo, B. Ricci, S. Scopel, and F. L. Villante, Phys. Rev. D 66, 053005 (2002).
- N. Bernal, J. Martín-Albo, and S. Palomares-Ruiz, J. Cosmol. Astropart. Phys. 08 (2013) 011.
- R. K. Leane, T. Linden, P. Mukhopadhyay, and N. Toro, Phys. Rev. D 103, 075030 (2021).
- R. K. Leane and J. Smirnov, J. Cosmol. Astropart. Phys. 12 (2023) 040.
- I. John, R. K. Leane, and T. Linden, Phys. Rev. D 112, 023028 (2025).
- I. John, R. K. Leane, and T. Linden, Phys. Rev. D 109, 123041 (2024).
- C. Ilie and C. Levy, Phys. Rev. D 104, 083033 (2021).
- C. Ilie, Astrophys. J. 970, 159 (2024).
- C. V. Cappiello, Phys. Rev. Lett. 130, 221001 (2023).
- D. Krishna, R. Sherpa, A. K. Saha, T. N. Maity, R. Laha, and N. Raj, arXiv:2503.07713.
- A. Gould, Astrophys. J. 321, 571 (1987).
- T. T. Q. Nguyen and T. M. P. Tait, Phys. Rev. D 107, 115016 (2023).
- R. K. Leane and J. Tong, J. Cosmol. Astropart. Phys. 12 (2024) 031.
- M. Cirelli, G. Corcella, A. Hektor, G. Hutsi, M. Kadastik, P. Panci, M. Raidal, F. Sala, and A. Strumia, J. Cosmol. Astropart. Phys. 03 (2011) 051; 10 (2012) E01.
- P. Baratella, M. Cirelli, A. Hektor, J. Pata, M. Piibeleht, and A. Strumia, J. Cosmol. Astropart. Phys. 03 (2014) 053.
- C. Rott, J. Siegal-Gaskins, and J. F. Beacom, Phys. Rev. D 88, 055005 (2013).
- C. Arina, M. Di Mauro, N. Fornengo, J. Heisig, A. Jueid, and R. R. de Austri, J. Cosmol. Astropart. Phys. 03 (2024) 035.
- C. W. Bauer, N. L. Rodd, and B. R. Webber, J. High Energy Phys. 06 (2021) 121.
- Q. Liu, J. Lazar, C. A. Argüelles, and A. Kheirandish, J. Cosmol. Astropart. Phys. 10 (2020) 043.
- M. Shiozawa (Super-Kamiokande Collaboration), Nucl. Instrum. Methods Phys. Res., Sect. A 433, 240 (1999).
- E. Drakopoulou, G. A. Cowan, M. D. Needham, S. Playfer, and M. Taani, J. Instrum. 13, P04009 (2018).
- G.-L. Lin, T. T. L. Nguyen, M. Spinrath, T. D. H. Van, and T.-C. Wang, J. Cosmol. Astropart. Phys. 08 (2022) 027.
- M. Pospelov and A. Ray, J. Cosmol. Astropart. Phys. 01 (2024) 029.
- Y. Ema, M. Pospelov, and A. Ray, J. High Energy Phys. 07 (2024) 094.
- M. Jiang et al. (Super-Kamiokande Collaboration), Prog. Theor. Exp. Phys. 2019, 053F01 (2019).
- E. Richard et al. (Super-Kamiokande Collaboration), Phys. Rev. D 94, 052001 (2016).
- E. Konishi, Y. Minorikawa, V. I. Galkin, M. Ishiwata, I. Nakamura, N. Takahashi, M. Kato, and A. Misaki, arXiv:1007.3812.
- E. Konishi, Y. Minorikawa, V. I. Galkin, M. Ishiwata, I. Nakamura, N. Takahashi, M. Kato, and A. Misaki, arXiv:1108.1064.
- V. I. Galkin, A. M. Anokhina, E. Konishi, and A. Misaki, arXiv:0808.0824.
- S. Robles and S. A. Meighen-Berger, Phys. Rev. D 112, L041301 (2025).
- B. Zhou and J. F. Beacom, Phys. Rev. D 109, 103003 (2024).
- K. C. Y. Ng, J. F. Beacom, A. H. G. Peter, and C. Rott, Phys. Rev. D 96, 103006 (2017).
- R. Garani and S. Palomares-Ruiz, J. Cosmol. Astropart. Phys. 05 (2022) 042.
- J. F. Acevedo, R. K. Leane, and J. Smirnov, J. Cosmol. Astropart. Phys. 04 (2024) 038.
- E. Aprile et al. (XENON Collaboration), Phys. Rev. Lett. 123, 251801 (2019).
- J. Kopp, V. Niro, T. Schwetz, and J. Zupan, Phys. Rev. D 80, 083502 (2009).
- C. O’Hare, Direct detection plots, https://github.com/cajohare/DirectDetectionPlots (2024).
- R. Essig, M. Fernandez-Serra, J. Mardon, A. Soto, T. Volansky, and T.-T. Yu, J. High Energy Phys. 05 (2016) 046.
- C. Boehm and P. Fayet, Nucl. Phys. B683, 219 (2004).
- C. Boehm, P. Fayet, and J. Silk, Phys. Rev. D 69, 101302 (2004).
- P. Fayet, Phys. Rev. D 70, 023514 (2004).
- S.-M. Choi, Y. Hochberg, E. Kuflik, H. M. Lee, Y. Mambrini, H. Murayama, and M. Pierre, J. High Energy Phys. 10 (2017) 162.
- T. Lin, H.-B. Yu, and K. M. Zurek, Phys. Rev. D 85, 063503 (2012).
- Y. Hochberg, E. Kuflik, H. Murayama, T. Volansky, and J. G. Wacker, Phys. Rev. Lett. 115, 021301 (2015).
- Y. Hochberg, E. Kuflik, T. Volansky, and J. G. Wacker, Phys. Rev. Lett. 113, 171301 (2014).
- E. Kuflik, M. Perelstein, N. R.-L. Lorier, and Y.-D. Tsai, Phys. Rev. Lett. 116, 221302 (2016).
- E. Kuflik, M. Perelstein, N. R.-L. Lorier, and Y.-D. Tsai, J. High Energy Phys. 08 (2017) 078.
- R. T. D’Agnolo, C. Mondino, J. T. Ruderman, and P.-J. Wang, J. High Energy Phys. 08 (2018) 079.
- X. Chu, T. Hambye, and M. H. G. Tytgat, J. Cosmol. Astropart. Phys. 05 (2012) 034.
- C. Dvorkin, T. Lin, and K. Schutz, Phys. Rev. D 99, 115009 (2019); 105, 119901(E) (2022).
- J. H. Chang, R. Essig, and A. Reinert, J. High Energy Phys. 03 (2021) 141.
- L. Barak et al. (SENSEI Collaboration), Phys. Rev. Lett. 125, 171802 (2020).
- I. M. Bloch et al. (SENSEI Collaboration), Phys. Rev. Lett. 134, 161002 (2025).
- I. Arnquist et al. (DAMIC-M Collaboration), Phys. Rev. Lett. 130, 171003 (2023).
- I. Arnquist et al. (DAMIC-M Collaboration), Phys. Rev. Lett. 132, 101006 (2024).
- R. Essig, T. Volansky, and T.-T. Yu, Phys. Rev. D 96, 043017 (2017).
- C. Cheng et al. (PandaX-II Collaboration), Phys. Rev. Lett. 126, 211803 (2021).
- T. T. Q. Nguyen, C. Blanco, R. Leane, and T. Linden, Jupiter is a Dark Matter Refrigerator: Electron Degeneracy Inhibits Evaporation (to be published).
- A. Abusleme et al. (JUNO Collaboration), Eur. Phys. J. C 81, 10 (2021).
- B. Abi et al. (DUNE Collaboration), arXiv:2002.03005.
- C. R. Harris et al., Nature (London) 585, 357–362 (2020).
- P. Virtanen et al., Nat. Methods 17, 261 (2020).
- J. D. Hunter, Comput. Sci. Eng. 9, 90 (2007).
- T. Kluyver, B. Ragan-Kelley, F. Pérez, B. Granger, M. Bussonnier, J. Frederic, K. Kelley, J. Hamrick, J. Grout, S. Corlay, P. Ivanov, D. Avila, S. Abdalla, and C. Willing (Jupyter Development Team), in (IOS Press, 2016), pp. 87–90, 10.3233/978-1-61499-649-1-87.
- A. Rohatgi, Webplotdigitizer: Version 4.6 (2022).
- T. Piffl et al., Astron. Astrophys. 562, A91 (2014).
- A. Gould, Astrophys. J. 321, 560 (1987).
- T. Linden, T. T. Q. Nguyen, and T. M. P. Tait, arXiv:2402.01839.
- C. Blanco and R. K. Leane, Phys. Rev. Lett. 132, 261002 (2024).
- C. Blanco, R. K. Leane, M. Moore, and J. Tong, arXiv:2408.15318.
- R. K. Leane and T. Linden, Phys. Rev. Lett. 131, 071001 (2023).
- L. Li and J. Fan, J. High Energy Phys. 10 (2022) 186.
- S. Yan, L. Li, and J. Fan, J. High Energy Phys. 06 (2024) 028.
- D. Croon and J. Smirnov, J. Cosmol. Astropart. Phys. 11 (2024) 046.
- E. Magg et al., Astron. Astrophys. 661, A140 (2022).
- M. French, A. Becker, W. Lorenzen, N. Nettelmann, M. Bethkenhagen, J. Wicht, and R. Redmer, Astrophys. J. Suppl. Ser. 202, 5 (2012).
- P. Bhattacharjee, F. Calore, and P. D. Serpico, Phys. Rev. D 107, 043012 (2023); 109, 129904(E) (2024).
- R. K. Leane and J. Smirnov, J. Cosmol. Astropart. Phys. 10 (2023) 057.
- D. Bose, R. Pramanick, and T. S. Ray, Phys. Lett. B 866, 139542 (2025).
- D. Bose, T. N. Maity, and T. S. Ray, J. Cosmol. Astropart. Phys. 05 (2022) 001.
- C. Andreopoulos et al., Nucl. Instrum. Methods Phys. Res., Sect. A 614, 87 (2010).
- M. Honda, T. Kajita, K. Kasahara, and S. Midorikawa, Phys. Rev. D 83, 123001 (2011).
- S. Desai et al. (Super-Kamiokande Collaboration), Astropart. Phys. 29, 42 (2008).
- B. Carew, A. R. Caddell, T. N. Maity, and C. A. J. O’Hare, Phys. Rev. D 109, 083016 (2024).
- P. Agnes et al. (DarkSide Collaboration), Phys. Rev. Lett. 130, 101002 (2023).