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...
المؤلفون الرئيسيون: | Matthews, JH, Taylor, AM |
---|---|
التنسيق: | Conference item |
اللغة: | English |
منشور في: |
Sissa Medialab
2023
|
مواد مشابهة
-
Cosmic ray acceleration to ultrahigh energy in radio galaxies
حسب: Matthews, J, وآخرون
منشور في: (2019) -
Intergalactic propagation of ultrahigh energy cosmic ray nuclei: An analytic approach
حسب: Hooper, D, وآخرون
منشور في: (2008) -
Open questions in cosmic-ray research at ultrahigh energies
حسب: Alves Batista, R, وآخرون
منشور في: (2019) -
Clustering of ultrahigh energy cosmic rays and their sources
حسب: Evans, N, وآخرون
منشور في: (2003) -
Open Questions in Cosmic-Ray Research at Ultrahigh Energies
حسب: Rafael Alves Batista, وآخرون
منشور في: (2019-06-01)