-
[1]
O. Adriani, G. C. Barbarino, G. A. Bazilevskaya et al., Nature, 458: 607 (2009)
-
[2]
A. A. Abdo, M. Ackermann, M. Ajello et al., Physical Review Letters, 102: 181101 (2009)
-
[3]
M. Aguilar, L. Ali Cavasonza, G. Ambrosi et al., Physical Review Letters, 122: 041102 (2019)
-
[4]
M. Aguilar, D. Aisa, A. Alvino et al., Physical Review Letters, 113: 121102 (2014)
-
[5]
X. Li, Z.-Q. Shen, B.-Q. Lu et al., Physics Letters B, 749: 267 (2015)
-
[6]
DAMPE Collaboration, G. Ambrosi, Q. An et al., Nature, 552: 63 (2017)
-
[7]
M. Aguilar, L. Ali Cavasonza, B. Alpat et al., Physical Review Letters, 122: 101101 (2019)
-
[8]
F. Aharonian, A. G. Akhperjanian, G. Anton et al., A&A, 508: 561 (2009)
-
[9]
D. Kerszberg, for the HESS collaboration. 2017
-
[10]
D. Borla Tridon, International Cosmic Ray Conference, 6: 47 (2011)
-
[11]
A. Archer, W. Benbow, R. Bird et al., Phys. Rev. D, 98: 062004 (2018)
-
[12]
S. Profumo, Central European Journal of Physics, 10: 1 (2012)
-
[13]
H. Yüksel, M. D. Kistler, and T. Stanev, Physical Review Letters, 103: 051101 (2009)
-
[14]
Y. Fujita, K. Kohri, R. Yamazaki et al., Phys. Rev. D, 80: 063003 (2009)
-
[15]
W. Liu, X.-J. Bi, S.-J. Lin et al., Phys. Rev. D, 96: 023006 (2017)
-
[16]
L. Bergström, J. Edsjö, and g. Zaharijas, Physical Review Letters, 103: 031103 (2009)
-
[17]
P.-F. Yin, Q. Yuan, J. Liu et al., Phys. Rev. D, 79: 023512 (2009)
-
[18]
M. A.Malkov, P. H. Diamond and R. Z. Sagdeev, Phys. Rev. D, 94: 063006 (2016)
-
[19]
X.-J. Bi, P.-F. Yin, and Q. Yuan, Frontiers of Physics, 8: 794 (2013)
-
[20]
Y.-Z. Fan, B. Zhang, and J. Chang, International Journal of Modern Physics D, 19: 2011 (2010)
-
[21]
G. Vannoni, S. Gabici, and F. A. Aharonian, A&A, 497: 17 (2009)
-
[22]
C. Jin, W. Liu, and H.-B. Hu et al., Phys. Rev. D, 97: 123005 (2018)
-
[23]
B. Wang, Q. Yuan, C. Fan et al., Science China Physics, Mechanics, and Astronomy, 53: 842 (2010)
-
[24]
N. Tomassetti, ApJ, 752: L13 (2012)
-
[25]
C. Evoli, D. Gaggero, and D. Grasso, J. Cosmology Astropart. Phys., 2015: 039 (2015)
-
[26]
O. Adriani, G. C. Barbarino, G. A. Bazilevskaya et al., Science, 332: 69 (2011)
-
[27]
J. Feng, N. Tomassetti, and A. Oliva, Phys. Rev. D, 94: 123007 (2016)
-
[28]
Y.-Q. Guo, Z. Tian, and C. Jin, ApJ, 819: 54 (2016)
-
[29]
W. Liu, Y.-h. Yao, and Y.-Q. Guo, ApJ, 869: 176 (2018)
-
[30]
A. A. Abdo, B. T. Allen, T. Aune et al., ApJ, 700: L127 (2009)
-
[31]
A. U. Abeysekara, A. Albert, R. Alfaro et al., Science, 358: 911 (2017)
-
[32]
M. DI MAURO, S. MANCONI, F. DONATO, 2019, in AAS/High Energy Astrophysics Division, AAS/High Energy Astrophysics Division, 112.35
-
[33]
N. Tomassetti, Phys. Rev. D, 92: 081301 (2015)
-
[34]
D. Benyamin, E. Nakar, T. Piran et al., ApJ, 826: 47 (2016)
-
[35]
D. Gaggero, L. Maccione, G. Di Bernardo et al., Physical Review Letters, 111: 021102 (2013)
-
[36]
T. A. Porter, G. Jóhannesson, and I. V. Moskalenko, ApJ, 846: 67 (2017)
-
[37]
D. Maurin, F. Donato, R. Taillet et al., ApJ, 555: 585 (2001)
-
[38]
A. W. Strong, I. V. Moskalenko, and V. S. Ptuskin, Annual Review of Nuclear and Particle Science, 57: 285 (2007)
-
[39]
A. D. Erlykin and A. W. Wolfendale, Astroparticle Physics, 42: 70 (2013)
-
[40]
P. Blasi, E. Amato, and P. D. Serpico, Physical Review Letters, 109: 061101 (2012)
-
[41]
W. I. Axford, E. Leer, G. Skadron, 1977, in International Cosmic Ray Conference, Vol. 11, International Cosmic Ray Conference, 132
-
[42]
R. D. Blandford and J. P. Ostriker, ApJ, 221: L29 (1978)
-
[43]
G. Jóhannesson, R. Ruiz de Austri, A. C. Vincent et al., ApJ, 824: 16 (2016)
-
[44]
R. Trotta, G. Jóhannesson, I. V. Moskalenko et al., ApJ, 729: 106 (2011)
-
[45]
M. Ackermann, M. Ajello, A. Allafort et al., Science, 339: 807 (2013)
-
[46]
A. Neronov, D. V. Semikoz, and A. M. Taylor, Phys. Rev. Lett., 108: 051105 (2012)
-
[47]
A. W. Strong, E. Orlando, and T. R. Jaffe, A&A, 534: A54 (2011)
-
[48]
Y. Zhang, S. Liu, and Q. Yuan, ApJ, 844: L3 (2017)
-
[49]
F. A. Aharonian, Space Sci. Rev., 99: 187 (2001)
-
[50]
I. V. Moskalenko, A. W. Strong, J. F. Ormes et al., ApJ, 565: 280 (2002)
-
[51]
I. V. Moskalenko and A. W. Strong, ApJ, 493: 694 (1998)
-
[52]
T. Delahaye, J. Lavalle, R. Lineros et al., A&A, 524: A51 (2010)
-
[53]
C. Evoli, D. Gaggero, A. Vittino et al., J. Cosmology Astropart. Phys., 2: 015 (2017)
-
[54]
T. Delahaye, R. Lineros, F. Donato et al., A&A, 501: 821 (2009)
-
[55]
Q. Yuan and X.-J. Bi, J. Cosmology Astropart. Phys., 2015: 033 (2015)
-
[56]
S.-J. Lin, Q. Yuan, and X.-J. Bi, Phys. Rev. D, 91: 063508 (2015)
-
[57]
W. H. Press, S. A. Teukolsky, W. T. Vetterling et al, 2002, Numerical recipes in C++ : the art of scientific computing
-
[58]
J. S. Perko, A&A, 184: 119 (1987)
-
[59]
E. S. Levine, L. Blitz, and C. Heiles, Science, 312: 1773 (2006)
-
[60]
H. Weaver, 1970, in IAU Symposium, Vol. 38, The Spiral Structure of our Galaxy, ed. W. Becker & G. I. Kontopoulos, 126
-
[61]
D. A. Green, MNRAS, 454: 1517 (2015)
-
[62]
J. P. Vallée, ApJ, 566: 261 (2002)
-
[63]
J. P. Vallée, New A Rev., 79: 49 (2017)
-
[64]
C.-A. Faucher-Giguère and V. M. Kaspi, ApJ, 643: 332 (2006)
-
[65]
N. Kawanaka, K. Ioka, and M. M. Nojiri, ApJ, 710: 958 (2010)
-
[66]
G. Bernard, T. Delahaye, P. Salati et al., A&A, 544: A92 (2012)
-
[67]
P. Mertsch, J. Cosmology Astropart. Phys., 2: 31 (2011)
-
[68]
K. Fang, X.-J. Bi, and P.-F. Yin, ApJ, 854: 57 (2018)
-
[69]
T. Kobayashi, Y. Komori, K. Yoshida et al., ApJ, 601: 340 (2004)
-
[70]
D. Malyshev and D. W. Hogg, ApJ, 738: 181 (2011)
-
[71]
S. Kisaka and N. Kawanaka, MNRAS, 421: 3543 (2012)
-
[72]
M. Aguilar, D. Aisa, B. Alpat et al., Physical Review Letters, 114: 171103 (2015)
-
[73]
M. Aguilar, L. Ali Cavasonza, G. Ambrosi et al., Phys. Rev. Lett., 120: 021101 (2018)
-
[74]
M. Aguilar, L. Ali Cavasonza, B. Alpat et al., Physical Review Letters, 119: 251101 (2017)
-
[75]
Y. S. Yoon, T. Anderson, A. Barrau et al., ApJ, 839: 5 (2017)
-
[76]
Q. An, R. Asfandiyarov, P. Azzarello et al., Measurement of the cosmic ray proton spectrum from 40 GeV to 100 TeV with the DAMPE satellite. Science Advances, 5(9):eaax3793, September 2019
-
[77]
O. Adriani, Y. Akaike, K. Asano, et al., Direct Measurement of the Cosmic-Ray Proton Spectrum from 50 GeV to 10 TeV with the Calorimetric Electron Telescope on the International Space Station. Physical Review Letters, 122(18):181102, May 2019
-
[78]
S. Recchia, S. Gabici, F. A. Aharonian et al., Phys. Rev. D, 99: 103022 (2019)
-
[79]
O. Adriani, Y. Akaike, K. Asano et al., Phys. Rev. Lett., 120: 261102 (2018)
-
[80]
M. Ahlers, Physical Review Letters, 117: 151103 (2016)
-
[81]
W. Liu, Y.-Q. Guo, and Q. Yuan, J. Cosmology Astropart. Phys., 2019: 010 (2019)
-
[82]
S. Abdollahi, M. Ackermann, M. Ajello et al., Physical Review Letters, 118: 091103 (2017)
-
[83]
R. N. Manchester, G. B. Hobbs, A. Teoh et al., AJ, 129: 1993 (2005)
-
[84]
Z. Cao, Chinese Physics C, 34: 249 (2010)
-
[85]
S. N. Zhang, O. Adriani, S. Albergo et al., 2014, in Proc. SPIE, Vol. 9144, Space Telescopes and Instrumentation 2014: Ultraviolet to Gamma Ray, 91440X