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Exploring the superwind mechanism for generating ultrahigh-energy cosmic rays using large-scale modeling of starbursts
- Source :
- Phys. Rev. D 102, 023034 (2020)
- Publication Year :
- 2020
-
Abstract
- The Pierre Auger Collaboration has provided a compelling indication for a possible correlation between the arrival directions of ultrahigh-energy cosmic rays and nearby starburst galaxies. Herein we show how the latest large-scale modeling of starburst galaxies is compatible with the cosmic rays producing the anisotropy signal being accelerated at the terminal shock of superwinds.<br />Comment: Matching version to be published in Physical Review D; 9 pages revtex, 5 .pdf figures
Details
- Database :
- arXiv
- Journal :
- Phys. Rev. D 102, 023034 (2020)
- Publication Type :
- Report
- Accession number :
- edsarx.2004.09378
- Document Type :
- Working Paper
- Full Text :
- https://doi.org/10.1103/PhysRevD.102.023034