Towards searching for photons with energies beyond the PeV range from galactic PeVatrons

Kód výsledku v IS VaVaI
<a href="https://www.isvavai.cz/riv?ss=detail&h=RIV%2F68378271%3A90232%2F25%3A00641911" target="_blank" >RIV/68378271:90232/25:00641911 - isvavai.cz</a>
Výsledek na webu
<a href="https://doi.org/10.1016/j.astropartphys.2024.103074" target="_blank" >https://doi.org/10.1016/j.astropartphys.2024.103074</a>
DOI - Digital Object Identifier
<a href="http://dx.doi.org/10.1016/j.astropartphys.2024.103074" target="_blank" >10.1016/j.astropartphys.2024.103074</a>

Jazyk výsledku
angličtina
Název v původním jazyce
Towards searching for photons with energies beyond the PeV range from galactic PeVatrons
Popis výsledku v původním jazyce
Several gamma-ray observatories have discovered photons of cosmic origin with energies in the PeV ( 10 15 eV) range. Photons at these energies might be produced as by-products from particle acceleration in so-called PeVatrons, which are widely assumed to be the sources of a large part of galactic cosmic rays. Based on recent measurements of these PeV y-sources by LHAASO and HAWC, we extrapolate the energy spectra of selected sources up to the ultra-high-energy (UHE, >= 10 PeV) regime.
Název v anglickém jazyce
Towards searching for photons with energies beyond the PeV range from galactic PeVatrons
Popis výsledku anglicky
Several gamma-ray observatories have discovered photons of cosmic origin with energies in the PeV ( 10 15 eV) range. Photons at these energies might be produced as by-products from particle acceleration in so-called PeVatrons, which are widely assumed to be the sources of a large part of galactic cosmic rays. Based on recent measurements of these PeV y-sources by LHAASO and HAWC, we extrapolate the energy spectra of selected sources up to the ultra-high-energy (UHE, >= 10 PeV) regime.

Rok uplatnění
2025
Kód důvěrnosti údajů
S - Úplné a pravdivé údaje o projektu nepodléhají ochraně podle zvláštních právních předpisů

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