Sensitivity of the Cherenkov Telescope Array to spectral signatures of hadronic PeVatrons with application to Galactic Supernova Remnants
<p>The local Cosmic Ray (CR) energy spectrum exhibits a spectral softening at energies around 3 PeV. Sources which are capable of accelerating hadrons to such energies are called hadronic PeVatrons. However, hadronic PeVatrons have not yet been firmly identified within the Galaxy. Several sour...
| Hlavní autoři: | , , , |
|---|---|
| Další autoři: | |
| Médium: | Journal article |
| Jazyk: | English |
| Vydáno: |
Elsevier
2023
|