Zobrazeno 1 - 7
of 7
pro vyhledávání: '"Anton Prosekin"'
The detection of the pulsed $\sim 1 $~TeV gamma-ray emission from the Crab pulsar reported by MAGIC and VERITAS collaborations demands a substantial revision of existing models of particle acceleration in the pulsar magnetosphere. In this regard mode
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::8501025b37f8c3855922e6d117e31caa
http://arxiv.org/abs/1902.01191
http://arxiv.org/abs/1902.01191
Publikováno v:
AIP Conference Proceedings.
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b6d0055f7ce2bbc67ac7aacdedf0966f
https://doi.org/10.1063/1.4969038
https://doi.org/10.1063/1.4969038
Publikováno v:
Physical Review D. 94
We study the polarization properties of the jitter and synchrotron radiation produced by electrons in highly turbulent anisotropic magnetic fields. The net polarization is provided by the geometry of the magnetic field the directions of which are par
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::06cfe80ea14f6452a43805b6c8be138a
https://doi.org/10.1103/physrevd.94.063010
https://doi.org/10.1103/physrevd.94.063010
Publikováno v:
Physical Review D
A stationary distribution function that describes the entire process of the propagation of relativistic particles, including the transition between the ballistic and diffusion regimes, is obtained. The spacial component of the constructed function sa
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::7047b29536dbf0eb7c69bde6e3c21496
https://hdl.handle.net/11858/00-001M-0000-0028-FF44-811858/00-001M-0000-0028-FF42-C
https://hdl.handle.net/11858/00-001M-0000-0028-FF44-811858/00-001M-0000-0028-FF42-C
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:
Astrophysical Journal
Blazars are expected to produce both gamma rays and cosmic rays. Therefore, observed high-energy gamma rays from distant blazars may contain a significant contribution from secondary gamma rays produced along the line of sight by the interactions of
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::e5cd35c0e1ba97cfe814b59f0789a6fe
http://arxiv.org/abs/1203.3787
http://arxiv.org/abs/1203.3787
At TeV energies, the gamma-ray horizon of the universe is limited to redshifts z<1 is lacking at present, the growing number of TeV blazars with redshifts as large as z~0.5 suggests the possibility that the standard blazar models may have to be recon
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::4999f55631530a421c0bd86c5406333d