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. Governato et al., Mon. Not. Roy. Astron. Soc. 300, 146 (1998), arXiv:astro-ph/9801192
[4]
A. A. Klypin, A. V. Kravtsov, O. Valenzuela et al., Astrophys. J. 522, 82 (1999), arXiv:astroph/9901240
[5]
B. Moore, S. Ghigna, F. Governato et al., Astrophys. J. Lett. 524, L19 (1999)), arXiv:astro-ph/9907411
[6]
C. Boehm, P. Fayet, and R. Schaeffer, Phys. Lett. B 518, 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, JCAP 08, 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. D 74, 063509 (2006), arXiv:astro-ph/0607319
[11]
V. Berezinsky, V. Dokuchaev, and Y. Eroshenko, Phys. Rev. D 77, 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. D 71, 103520 (2005), arXiv:astro-ph/0504112
[14]
J. Diemand, B. Moore, and J. Stadel, Nature 433, 389 (2005), arXiv:astro-ph/0501589
[15]
L. Gao, S. D. M. White, A. Jenkins et 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. Tormen et 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. Governato et al., Astrophys. J. 544, 616 (2000), arXiv:astro-ph/9910166
[21]
C. D. Wilson et al., Mon. Not. Roy. Astron. Soc. 424, 3050 (2012), arXiv:1206.1629[astro-ph.CO
[22]
G. De Lucia, G. Kauffmann, V. Springel et 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. Jenkins et al., Mon. Not. Roy. Astron. Soc. 355, 819 (2004), arXiv:astro-ph/0404589
[26]
V. Springel, J. Wang, M. Vogelsberger et al., Mon. Not. Roy. Astron. Soc. 391, 1685 (2008), arXiv:0809.0898[astro-ph
[27]
J. Diemand, M. Kuhlen, P. Madau et al., Nature 454, 735 (2008), arXiv:0805.1244[astro-ph
[28]
S. Garrison-Kimmel, M. Boylan-Kolchin, J. Bullock et 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. Tsai et al., Phys. Rev. Lett. 118, 191101 (2017), arXiv:1610.03840[astroph.HE
[31]
M.-Y. Cui, X. Pan, Q. Yuan et al., JCAP 06, 024 (2018), arXiv:1803.02163[astro-ph.HE
[32]
A. Cuoco, J. Heisig, L. Klamt et al., Phys. Rev. D 99, 103014 (2019), arXiv:1903.01472[astro-ph.HE
[33]
I. Cholis, T. Linden, and D. Hooper, Phys. Rev. D 99, 103026 (2019), arXiv:1903.02549[astro-ph.HE
[34]
S.-J. Lin, X.-J. Bi, and P.-F. Yin, Phys. Rev. D 100, 103014 (2019), arXiv:1903.09545[astro-ph.HE
[35]
M. Boudaud, Y. Génolini, L. Derome et 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. Krämer et al., JCAP 12, 037 (2021), arXiv:2107.12395[astro-ph.HE
[38]
C.-R. Zhu, M.-Y. Cui, Z.-Q. Xia et al., Phys. Rev. Lett. 129, 231101 (2022), arXiv:2204.03767[astro-ph.HE
[39]
X.-J. Lv, X.-J. Bi, K. Fang et al., (2023), arXiv: 2304.00760[astro-ph.HE
[40]
M. Aguilar et al. (AMS), Phys. Rept. 894, 1 (2021)
[41]
J. Chang et 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. Fang et al., Phys. Rev. D 95, 083007 (2017), arXiv:1701.06149[astro-ph.HE
[46]
M. di Mauro, F. Donato, A. Goudelis et al., Phys. Rev. D 90 , 085017 (2014) [Erratum: Phys. Rev. D 98 , 049901 (2018)], arXiv: 1408.0288[hep-ph
[47]
M. Cirelli, G. Corcella, A. Hektor et al., JCAP 03 , 051 (2011) [Erratum: JCAP 10 , E01 (2012)], arXiv: 1012.4515[hep-ph
[48]
P. Ciafaloni, D. Comelli, A. Riotto et al., JCAP 03, 019 (2011), arXiv:1009.0224[hep-ph
[49]
Q. Yuan et al., (2017), arXiv: 1711.10989[astro-ph.HE
[50]
P. Brun, T. Delahaye, J. Diemand et al., Phys. Rev. D 80, 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. D 81, 043532 (2010), arXiv:1001.3144[astroph.GA
[53]
M. Kamionkowski and S. M. Koushiappas, Phys. Rev. D 77, 103509 (2008), arXiv:0801.3269[astro-ph
[54]
G. Ambrosi et al. (DAMPE), Nature 552, 63 (2017), arXiv:1711.10981[astro-ph.HE
[55]
P. Ciafaloni, M. Cirelli, D. Comelli et al., JCAP 06, 018 (2011), arXiv:1104.2996[hep-ph
[56]
A. De Simone, A. Riotto, and W. Xue, JCAP 05, 003 (2013), arXiv:1304.1336[hep-ph