TeV energies gamma-rays, measurable by the imaging Cherenkov technique, are the most interesting for searching for hadronic CRs in SNRs because they provide information about CRs of the highest possible energies 10 13 -10 14 eV. Direct information about high-energy CR population in SNRs can be obtai
β¦ LIBER β¦
Contribution to the local cosmic-ray flux from the Geminga supernova
β Scribed by P.A. Johnson
- Publisher
- Elsevier Science
- Year
- 1994
- Tongue
- English
- Weight
- 390 KB
- Volume
- 2
- Category
- Article
- ISSN
- 0927-6505
No coin nor oath required. For personal study only.
β¦ Synopsis
The contribution to the local cosmic-ray flux from the Geminga supernova is calculated assuming shock acceleration to 1014 eV in a remnant which was formed several ld years ago along with the Gerninga pulsar. The particles am propagated to Earth using a simple diffusion model. In the region below the knee in the spectrum, it is found the supernova may contribute 10% of the local cosmic-ray flux, assuming plausible explosion parameters. The contribution to the amplitude of the anisotropy is not in conflict with the data in this energy region.
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