Cite this article: |
$author.xingMing_EN. [J]. Modern Physics, 2019, 31(2): 3-8.
|
[1]
|
Hess VF. Über beobachtungen der durchdringenden Strahlung bei sieben Freiballonfahren. Phys. Z. 1912, 13:1084 https://en.wikipedia.org/wiki/Cosmic_ray
|
[2]
|
Baade W, Zwicky F. Cosmic rays from super-novae. Astronomy, 1934, 20:259
|
[3]
|
Dubner G, Giacani E. Radio emission from supernova remnants. Astron Astrophysics Rev, 2015, 23:3
|
[4]
|
Koyama K, et al. Evidence for shock acceleration of high-energy electrons in the supernova remnant SN1006. Nature, 1995, 378:255
|
[5]
|
Ackermann M, et al. Detection of characteristic Pion-decay signature in supernova remnants. Science, 2013, 339:807
|
[6]
|
Funk S. Space-and ground-based Gamma-ray astrophysics. Annual Reviews of Nuclear and Particle Science, 2015, 65:245
|
[7]
|
刘四明. 宇宙中高能带电粒子的加速. 中国科学:物理学力学天文学, 2015, 45(11):119509
|
[8]
|
Fermi E. On the Origin of the Cosmic Radiation. Physical Review, 1949, 75:1169
|
[9]
|
Yuan Q, et al. A statistical model for the γ-ray variability of the crab nebula. ApJ, 2011, 730:L15
|
[10]
|
Zhang YR, Liu SM, Yuan Q. Anomalous Distributions of Primary Cosmic Rays as Evidence for Time-dependent Particle Acceleration in Supernova Remnants. ApJ, 2017, 844:L3
|
[11]
|
Kachelrieb M, Neronov A, Semikoz DV. Cosmic ray signatures of a 2-3 Myr old local supernova. Physical Review D, 2018, 97:063011
|
[12]
|
Zhang YR, Liu SM. Global constraints on diffusive particle acceleration by strong non-relativistic shocks. MNRAS, 2018, doi:10.1093/mnras/sty3136
|
|
|