\begin{document}$ e^\pm $\end{document} spectrum at \begin{document}$ \sim 1.4 $\end{document} TeV and find that the current AMS-02 antiproton results do not limit this contribution."> Impact of a nearby subhalo on the constraint of dark matter annihilation from cosmic ray antiprotons -
  • [1]

    J. F. Navarro, C. S. Frenk, and S. D. M. White, Astrophys. J.490, 493 (1997), arXiv:astro-ph/9611107

  • [2]

    A. A. Klypin, S. Gottlober, and A. V. Kravtsov, Astrophys. J.516, 530 (1999), arXiv:astro-ph/9708191

  • [3]

    S. Ghigna, B. Moore, F. Governatoet al., Mon. Not. Roy. Astron. Soc.300, 146 (1998), arXiv:astro-ph/9801192

  • [4]

    A. A. Klypin, A. V. Kravtsov, O. Valenzuelaet al., Astrophys. J.522, 82 (1999), arXiv:astroph/9901240

  • [5]

    B. Moore, S. Ghigna, F. Governatoet al., Astrophys. J. Lett.524, L19 (1999)), arXiv:astro-ph/9907411

  • [6]

    C. Boehm, P. Fayet, and R. Schaeffer, Phys. Lett. B518, 8 (2001), arXiv:astro-ph/0012504

  • [7]

    A. M. Green, S. Hofmann, and D. J. Schwarz, Mon. Not. Roy. Astron. Soc.353, L23 (2004), arXiv:astroph/0309621

  • [8]

    A. M. Green, S. Hofmann, and D. J. Schwarz, JCAP08, 003 (2005), arXiv:astro-ph/0503387

  • [9]

    A. M. Green, S. Hofmann, and D. J. Schwarz, AIP Conf. Proc.805, 431 (2005), arXiv:astro-ph/0508553

  • [10]

    E. Bertschinger, Phys. Rev. D74, 063509 (2006), arXiv:astro-ph/0607319

  • [11]

    V. Berezinsky, V. Dokuchaev, and Y. Eroshenko, Phys. Rev. D77, 083519 (2008), arXiv:0712.3499[astro-ph

  • [12]

    J. Diemand, M. Kuhlen, and P. Madau, Astrophys. J.667, 859 (2007), arXiv:astro-ph/0703337

  • [13]

    A. Loeb and M. Zaldarriaga, Phys. Rev. D71, 103520 (2005), arXiv:astro-ph/0504112

  • [14]

    J. Diemand, B. Moore, and J. Stadel, Nature433, 389 (2005), arXiv:astro-ph/0501589

  • [15]

    L. Gao, S. D. M. White, A. Jenkinset al., Mon. Not. Roy. Astron. Soc.363, 379 (2005), arXiv:astro-ph/0503003

  • [16]

    J. Diemand, M. Kuhlen, and P. Madau, Astrophys. J.649, 1 (2006), arXiv:astro-ph/0603250

  • [17]

    V. Springel, S. D. M. White, G. Tormenet al., Mon. Not. Roy. Astron. Soc.328, 726 (2001), arXiv:astro-ph/0012055

  • [18]

    A. R. Zentner and J. S. Bullock, Astrophys. J.598, 49 (2003), arXiv:astro-ph/0304292

  • [19]

    G. Tormen, A. Diaferio, and D. Syer, Mon. Not. Roy. Astron. Soc.299, 728 (1998), arXiv:astro-ph/9712222

  • [20]

    S. Ghigna, B. Moore, F. Governatoet al., Astrophys. J.544, 616 (2000), arXiv:astro-ph/9910166

  • [21]

    C. D. Wilsonet al., Mon. Not. Roy. Astron. Soc.424, 3050 (2012), arXiv:1206.1629[astro-ph.CO

  • [22]

    G. De Lucia, G. Kauffmann, V. Springelet al., Mon. Not. Roy. Astron. Soc.348, 333 (2004), arXiv:astroph/0306205

  • [23]

    A. V. Kravtsov, O. Y. Gnedin, and A. A. Klypin, Astrophys. J.609, 482 (2004), arXiv:astro-ph/0401088

  • [24]

    G. Kauffmann, S. D. M. White, and B. Guiderdoni, Mon. Not. Roy. Astron. Soc.264, 201 (1993)

  • [25]

    L. Gao, S. D. M. White, A. Jenkinset al., Mon. Not. Roy. Astron. Soc.355, 819 (2004), arXiv:astro-ph/0404589

  • [26]

    V. Springel, J. Wang, M. Vogelsbergeret al., Mon. Not. Roy. Astron. Soc.391, 1685 (2008), arXiv:0809.0898[astro-ph

  • [27]

    J. Diemand, M. Kuhlen, P. Madauet al., Nature454, 735 (2008), arXiv:0805.1244[astro-ph

  • [28]

    S. Garrison-Kimmel, M. Boylan-Kolchin, J. Bullocket al., Mon. Not. Roy. Astron. Soc.438, 2578 (2014), arXiv:1310.6746[astro-ph.CO

  • [29]

    A. Cuoco, M. Krämer, and M. Korsmeier, Phys. Rev. Lett.118, 191102 (2017), arXiv:1610.03071[astroph.HE

  • [30]

    M.-Y. Cui, Q. Yuan, Y.-L. S. Tsaiet al., Phys. Rev. Lett.118, 191101 (2017), arXiv:1610.03840[astroph.HE

  • [31]

    M.-Y. Cui, X. Pan, Q. Yuanet al., JCAP06, 024 (2018), arXiv:1803.02163[astro-ph.HE

  • [32]

    A. Cuoco, J. Heisig, L. Klamtet al., Phys. Rev. D99, 103014 (2019), arXiv:1903.01472[astro-ph.HE

  • [33]

    I. Cholis, T. Linden, and D. Hooper, Phys. Rev. D99, 103026 (2019), arXiv:1903.02549[astro-ph.HE

  • [34]

    S.-J. Lin, X.-J. Bi, and P.-F. Yin, Phys. Rev. D100, 103014 (2019), arXiv:1903.09545[astro-ph.HE

  • [35]

    M. Boudaud, Y. Génolini, L. Deromeet al., Phys. Rev. Res.2, 023022 (2020), arXiv:1906.07119[astro-ph.HE

  • [36]

    J. Heisig, M. Korsmeier, and M. W. Winkler, Phys. Rev. Res.2, 043017 (2020), arXiv:2005.04237[astro-ph.HE

  • [37]

    F. Kahlhoefer, M. Korsmeier, M. Krämeret al., JCAP12, 037 (2021), arXiv:2107.12395[astro-ph.HE

  • [38]

    C.-R. Zhu, M.-Y. Cui, Z.-Q. Xiaet al., Phys. Rev. Lett.129, 231101 (2022), arXiv:2204.03767[astro-ph.HE

  • [39]

    X.-J. Lv, X.-J. Bi, K. Fanget al., (2023), arXiv: 2304.00760[astro-ph.HE

  • [40]

    M. Aguilaret al. (AMS), Phys. Rept.894, 1 (2021)

  • [41]

    J. Changet al. (DAMPE), Astropart. Phys.95, 6 (2017), arXiv:1706.08453[astro-ph.IM

  • [42]

    I. V. Moskalenko and A. W. Strong, Astrophys. J.493, 694 (1998), arXiv:astro-ph/9710124

  • [43]

    A. W. Strong and I. V. Moskalenko, Astrophys. J.509, 212 (1998), arXiv:astro-ph/9807150

  • [44]

    T. K. Gaisser, R. Engel, and E. Resconi,Cosmic Rays and Particle Physics: 2nd Edition(Cambridge University Press, 2016).

  • [45]

    Q. Yuan, S.-J. Lin, K. Fanget al., Phys. Rev. D95, 083007 (2017), arXiv:1701.06149[astro-ph.HE

  • [46]

    M. di Mauro, F. Donato, A. Goudeliset al., Phys. Rev. D90, 085017 (2014) [Erratum: Phys. Rev. D98, 049901 (2018)], arXiv: 1408.0288[hep-ph

  • [47]

    M. Cirelli, G. Corcella, A. Hektoret al., JCAP03, 051 (2011) [Erratum: JCAP10, E01 (2012)], arXiv: 1012.4515[hep-ph

  • [48]

    P. Ciafaloni, D. Comelli, A. Riottoet al., JCAP03, 019 (2011), arXiv:1009.0224[hep-ph

  • [49]

    Q. Yuanet al., (2017), arXiv: 1711.10989[astro-ph.HE

  • [50]

    P. Brun, T. Delahaye, J. Diemandet al., Phys. Rev. D80, 035023 (2009), arXiv:0904.0812[astro-ph.HE

  • [51]

    A. V. Maccio’, A. A. Dutton, and F. C. v. d. Bosch, Mon. Not. Roy. Astron. Soc.391, 1940 (2008), arXiv:0805.1926[astro-ph

  • [52]

    M. Kamionkowski, S. M. Koushiappas, and M. Kuhlen, Phys. Rev. D81, 043532 (2010), arXiv:1001.3144[astroph.GA

  • [53]

    M. Kamionkowski and S. M. Koushiappas, Phys. Rev. D77, 103509 (2008), arXiv:0801.3269[astro-ph

  • [54]

    G. Ambrosiet al. (DAMPE), Nature552, 63 (2017), arXiv:1711.10981[astro-ph.HE

  • [55]

    P. Ciafaloni, M. Cirelli, D. Comelliet al., JCAP06, 018 (2011), arXiv:1104.2996[hep-ph

  • [56]

    A. De Simone, A. Riotto, and W. Xue, JCAP05, 003 (2013), arXiv:1304.1336[hep-ph

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