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...
| Main Authors: | , , , |
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| Drugi avtorji: | |
| Format: | Journal article |
| Jezik: | English |
| Izdano: |
Elsevier
2023
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