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...
Päätekijät: | Matthews, JH, Taylor, AM |
---|---|
Aineistotyyppi: | Conference item |
Kieli: | English |
Julkaistu: |
Sissa Medialab
2023
|
Samankaltaisia teoksia
-
Cosmic ray acceleration to ultrahigh energy in radio galaxies
Tekijä: Matthews, J, et al.
Julkaistu: (2019) -
Intergalactic propagation of ultrahigh energy cosmic ray nuclei: An analytic approach
Tekijä: Hooper, D, et al.
Julkaistu: (2008) -
Cosmic ray acceleration to ultrahigh energy in radio galaxies
Tekijä: Matthews James H., et al.
Julkaistu: (2019-01-01) -
Open questions in cosmic-ray research at ultrahigh energies
Tekijä: Alves Batista, R, et al.
Julkaistu: (2019) -
Clustering of ultrahigh energy cosmic rays and their sources
Tekijä: Evans, N, et al.
Julkaistu: (2003)