A GeV-TeV particle component and the barrier of cosmic-ray sea in the Central Molecular Zone
Galactic center is one of the most important cosmic-ray sources. Here, the authors show GeV-TeV cosmic ray density in the central molecular zone is lower than the cosmic ray sea component, suggesting presence of high energy particle accelerator at the galactic center and existence of barrier.
Guardado en:
Autores principales: | Xiaoyuan Huang, Qiang Yuan, Yi-Zhong Fan |
---|---|
Formato: | article |
Lenguaje: | EN |
Publicado: |
Nature Portfolio
2021
|
Materias: | |
Acceso en línea: | https://doaj.org/article/23f2b3affe9941c98e08046fdfcfaed1 |
Etiquetas: |
Agregar Etiqueta
Sin Etiquetas, Sea el primero en etiquetar este registro!
|
Ejemplares similares
-
Flavoured resonant leptogenesis at sub-TeV scales
por: A. Granelli, et al.
Publicado: (2021) -
Dense GeV electron–positron pairs generated by lasers in near-critical-density plasmas
por: Xing-Long Zhu, et al.
Publicado: (2016) -
Effect of Reactive Ion Etching on the Luminescence of GeV Color Centers in CVD Diamond Nanocrystals
por: Sergey A. Grudinkin, et al.
Publicado: (2021) -
Emittance preserving thin film plasma mirrors for GeV scale laser plasma accelerators
por: A. Zingale, et al.
Publicado: (2021) -
Interpretation of LHC excesses in ditop and ditau channels as a 400-GeV pseudoscalar resonance
por: Ernesto Arganda, et al.
Publicado: (2021)