Zobrazeno 1 - 8
of 8
pro vyhledávání: '"Xiao-Chuan Chang"'
Publikováno v:
Nuclear Physics B, Vol 934, Iss , Pp 396-407 (2018)
In November 2017, the DAMPE collaboration announced their first measurement of the electron spectrum between energies of 25 GeV and 4.6 TeV, including a narrow peak at ∼1.4 TeV with marginal significance. However, this feature is not observed in th
Externí odkaz:
https://doaj.org/article/c323d0f4c53d4eb8909e4b249a0eabe3
Autor:
C. W. Yang, Wei Liu, Hai-Ming Zhang, Hongbo Hu, Hua-Yang Li, Yi-Bin Pan, B. Q. Qiao, Ming-Ming Kang, Xiao-Chuan Chang, Yi-Qing Guo, Yu-Hua Yao
Publikováno v:
The Astrophysical Journal. 901:106
High-precision measurement of the isotropic diffuse γ-ray background (IGRB) has been extrapolated to the TeV energy region using the Fermi-LAT experiment. Various kinds of astrophysical sources are candidates for its origin. However, a consensus on
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::dad96d1a9a51b6fd8263d3580fa5358a
https://doi.org/10.3847/1538-4357/abb024
https://doi.org/10.3847/1538-4357/abb024
Star-forming galaxies, due to their high star-formation rates and hence large number of supernova remnants therein, are huge reservoirs of cosmic rays (CRs). These CRs collide with gases in the galaxies and produce high-energy neutrinos through $pp$
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4e6d84fad7b801c93591f3b3467fa534
http://arxiv.org/abs/1412.8361
http://arxiv.org/abs/1412.8361
Autor:
Xiang-Yu Wang, Xiao-Chuan Chang
One attractive scenario for the excess of sub-PeV/PeV neutrinos recently reported by IceCube is that they are produced by cosmic rays in starburst galaxies colliding with the dense interstellar medium. These proton-proton ($pp$) collisions also produ
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::561d4d855c497c5ae823e7bf6de6b989
http://arxiv.org/abs/1406.1099
http://arxiv.org/abs/1406.1099
Publikováno v:
The Astrophysical Journal. 833:200
Recent HESS observations of the ~200 pc scale diffuse gamma-ray emission from the central molecular zone (CMZ) suggest the presence of a PeV cosmic-ray accelerator (PeVatron) located in the inner 10 pc region of the Galactic Center. Interestingly, th
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::169026bc2efd3d687bd464ee652492dd
https://doi.org/10.3847/1538-4357/833/2/200
https://doi.org/10.3847/1538-4357/833/2/200
Publikováno v:
The Astrophysical Journal. 825:148
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::5aaa499008e5383a02ce9cbb7c2f3357
https://doi.org/10.3847/0004-637x/825/2/148
https://doi.org/10.3847/0004-637x/825/2/148
Publikováno v:
Astrophysical Journal; 7/10/2013, Vol. 825 Issue 2, p1-1, 1p
Publikováno v:
Astrophysical Journal; 6/1/2015, Vol. 805 Issue 2, p1-1, 1p