Cosmic ray electron spectrum due to the dispersion ofinjection spectrum

[1]
M. A. DuVernois, S. W. Barwick, J. J. Beatty et al, ApJ, 559: 296303 (2001)
[2]
J. J. Beatty, A. Bhattacharyya, C. Bower et al, Physical Review Letters, 93(24): 241102 (2004)
[3]
M. Aguilar, J. Alcaraz et al (AMS-01 Collaboration), Physics Letters B, 646: 145154 (2007)
[4]
J. Chang, J. H. Adams, H. S. Ahn et al, Nature, 456: 362365 (2008)
[5]
S. Torii, T. Yamagami, T. Tamura et al, High-energy electron observations by PPB-BETS flight in Antarctica. ArXiv e-prints, September 2008
[6]
O. Adriani, G. C. Barbarino, G. A. Bazilevskaya et al, Nature, 458: 607609 (2009)
[7]
A. A. Abdo, M. Ackermann, M. Ajello et al, Physical Review Letters, 102(18): 181101 (2009)
[8]
L. Accardo, M. Aguilar, D. Aisa et al, Physical Review Letters, 113(12): 121101 (2014)
[9]
M. Aguilar, D. Aisa, A. Alvino et al, Physical Review Letters, 113(12): 121102 (2014)
[10]
X.-J. Bi, P.-F. Yin, and Q. Yuan, Frontiers of Physics, 8: 794-827 (2013)
[11]
I. Cholis and D. Hooper, Phys. Rev. D, 88(2): 023013 (2013)
[12]
Q. Yuan and X.-J. Bi, Physics Letters B, 727: 17 (2013)
[13]
L. Feng, R.-Z. Yang, H.-N. He et al, Physics Letters B, 728: 250255 (2014)
[14]
X. Li, Z.-Q. Shen, B.-Q. Lu et al, Physics Letters B, 749: 267-271 (2015)
[15]
A. D. Panov, J. H. Adams, H. S. Ahn et al, Bulletin of the Russian Academy of Sciences, Physics, 73: 564567 (2009)
[16]
O. Adriani, G. C. Barbarino, G. A. Bazilevskaya et al, Science, 332: 69 (2011)
[17]
H. S. Ahn, P. Allison, M. G. Bagliesi et al, ApJl, 714: L89L93 (2010)
[18]
Y. S. Yoon, H. S. Ahn, P. S. Allison et al, ApJ, 728: 122 (2011)
[19]
M. Aguilar, D. Aisa, B. Alpat et al, Physical Review Letters, 114(17): 171103 (2015)
[20]
M. Aguilar, D. Aisa, B. Alpat et al, Physical Review Letters, 115(21): 211101 (2015)
[21]
M. Aguilar, L. Ali Cavasonza, G. Ambrosi et al, Phys. Rev. Lett., 120: 021101 (2018)
[22]
S. Abdollahi, M. Ackermann, M. Ajello et al, Phys. Rev. D, 95(8): 082007 (2017)
[23]
DAMPE Collaboration, G. Ambrosi, Q. An et al, Nature, 552: 6366 (2017)
[24]
W. Liu, X.-J. Bi, S.-J. Lin, B.-B. Wang, and P.-F. Yin, Phys. Rev. D, 96(2): 023006 (2017)
[25]
V. Ptuskin, V. Zirakashvili, and E.-S. Seo, ApJ, 763: 47 (2013)
[26]
F. Aharonian, A. G. Akhperjanian, U. Barres de Almeida et al, Physical Review Letters, 101(26): 261104 (2008)
[27]
F. Aharonian, A. G. Akhperjanian, G. Anton et al, AA, 508: 561564 (2009)
[28]
D. Borla Tridon, International Cosmic Ray Conference, 6: 47 (2011)
[29]
D. Staszak (VERITAS Collaboration), In 34th International Cosmic Ray Conference (ICRC2015), volume 34 of International Cosmic Ray Conference, page 411, July 2015
[30]
M. Amenomori, X. J. Bi, D. Chen et al, ApJ, 678: 11651179 (2008)
[31]
M. G. Aartsen, R. Abbasi, Y. Abdou et al, Phys. Rev. D, 88(4):042004 (2013)
[32]
G. Vannoni, S. Gabici, and F. A. Aharonian, AA, 497: 1726 (2009)
[33]
S. Thoudam and J. R. Hrandel, MNRAS, 414: 14321438 (2011)
[34]
Y. Ohira, R. Yamazaki, N. Kawanaka, and K. Ioka, MNRAS, 427: 91102 (2012)
[35]
K. Fang, X.-J. Bi, and P.-F. Yin, ApJ, 854: 57 (2018)
[36]
R. Schlickeiser and J. Ruppel, New Journal of Physics, 12(3):033044 (2010)
[37]
L . Stawarz, V. Petrosian, and R. D. Blandford, ApJ, 710: 236-247 (2010)
[38]
N. Kawanaka, K. Ioka, and M. M. Nojiri. Is Cosmic Ray Electron Excess from Pulsars Spiky or Smooth?: Continuous and Multiple Electron/Positron Injections. ApJ, 710:958963, February 2010.
[39]
K. Fang, B.-B. Wang, X.-J. Bi, S.-J. Lin, and P.-F. Yin, ApJ, 836: 172 (2017)
[40]
B.-B. Wang, X.-J. Bi, S.-J. Lin, and P.-f. Yin, Explanations of the DAMPE high energy electron/positron spectrum in the dark matter annihilation and pulsar scenarios, ArXiv e-prints, July 2017
[41]
Q. Yuan, L. Feng, P.-F. Yin et al, Interpretations of the DAMPE electron data, ArXiv e-prints, November 2017
[42]
K. Fang, X.-J. Bi, P.-F. Yin, and Q. Yuan, Two-zone diffusion of electrons and positrons from Geminga explains the positron anomaly, ArXiv e-prints, March 2018
[43]
C. Jin, W. Liu, H.-B. Hu, and Y.-Q. Guo, On the PeV knee of cosmic rays spectrum and TeV cutoff of electron spectrum, ArXiv e-prints, November 2016
[44]
S. P. Reynolds, ARAA, 46: 89126 (2008)
[45]
G. Dubner and E. Giacani, AA Rev., 23: 3 (2015)
[46]
P. Slane, A. Bykov, D. C. Ellison, G. Dubner, and D. Castro, Space Sci. Rev., 188: 187210 (2015)
[47]
A. M. Bykov, D. C. Ellison, A. Marcowith, and S. M. Osipov, Space Sci. Rev., 214: 41 (2018)
[48]
D. A. Green, Bulletin of the Astronomical Society of India, 42: 4758 (2014)
[49]
M. Pohl and J. A. Esposito, ApJ, 507: 327338 (1998)
[50]
I. Bsching, M. Pohl, and R. Schlickeiser, AA, 377: 1056-1062 (2001)
[51]
Q. Yuan, B. Zhang, and X.-J. Bi, Phys. Rev. D, 84(4): 043002 (2011)
[52]
M. A. Malkov, P. H. Diamond, and R. Z. Sagdeev, Nature Communications, 2: 194 (2011)
[53]
D. Maurin, R. Taillet, F. Donato et al, Galactic Cosmic Ray Nuclei as a Tool for Astroparticle Physics, ArXiv Astrophysics e-prints, December 2002
[54]
A. W. Strong, I. V. Moskalenko, and V. S. Ptuskin, Annual Review of Nuclear and Particle Science, 57: 285327 (2007)
[55]
L. J. Gleeson and W. I. Axford, ApJ, 154: 1011 (1968)
[56]
M. Aguilar, D. Aisa, B. Alpat et al, Physical Review Letters, 113(22): 221102 (2014)
[57]
E. G. Berezhko and G. F. Krymskii, Soviet Physics Uspekhi, 31: 2751 (1988)
[58]
P. A. Becker, T. Le, and C. D. Dermer, ApJ, 647: 539551 (2006)
[59]
V. N. Zirakashvili and F. Aharonian, AA, 465: 695702 (2007)
[60]
P. Blasi, MNRAS, 402: 28072816 (2010)
[61]
T. Kobayashi, Y. Komori, K. Yoshida, and J. Nishimura, ApJ, 601: 340351 (2004)
[62]
A. U. Abeysekara, A. Albert, R. Alfaro et al, Science, 358: 911914 (2017)