How, where and when do cosmic rays reach ultrahigh energies?

How, where and when do cosmic rays reach ultrahigh energies?

Understanding the origins of ultrahigh energy cosmic rays (UHECRs) -- which reach energies in excess of 1020 eV -- stretches particle acceleration physics to its very limits. In this review, we discuss how such energies can be reached, using general arguments that can often be derived on the back o...

Disgrifiad llawn

Manylion Llyfryddiaeth
Prif Awduron:	Matthews, JH, Taylor, AM
Fformat:	Conference item
Iaith:	English
Cyhoeddwyd:	Sissa Medialab 2023

Eitemau Tebyg

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Intergalactic propagation of ultrahigh energy cosmic ray nuclei: An analytic approach
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Constraints on Ultrahigh-Energy Cosmic-Ray Sources from a Search for Neutrinos above 10 PeV with IceCube
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A Method to Estimate the Primary Mass of Ultrahigh-energy Cosmic Rays from Measurements of the Depth of the Shower Maximum and the Muon Content
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Constraints on ultrahigh-energy cosmic-ray sources from a search for neutrinos above 10 PeV with IceCube
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The intergalactic propagation of ultra-high energy cosmic ray nuclei
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Search for correlations between the arrival directions of IceCube neutrino events and ultrahigh-energy cosmic rays detected by the Pierre Auger Observatory and the Telescope Array
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