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...
Asıl Yazarlar: | Matthews, JH, Taylor, AM |
---|---|
Materyal Türü: | Conference item |
Dil: | English |
Baskı/Yayın Bilgisi: |
Sissa Medialab
2023
|
Benzer Materyaller
-
Cosmic ray acceleration to ultrahigh energy in radio galaxies
Yazar:: Matthews, J, ve diğerleri
Baskı/Yayın Bilgisi: (2019) -
Intergalactic propagation of ultrahigh energy cosmic ray nuclei: An analytic approach
Yazar:: Hooper, D, ve diğerleri
Baskı/Yayın Bilgisi: (2008) -
Cosmic ray acceleration to ultrahigh energy in radio galaxies
Yazar:: Matthews James H., ve diğerleri
Baskı/Yayın Bilgisi: (2019-01-01) -
Open questions in cosmic-ray research at ultrahigh energies
Yazar:: Alves Batista, R, ve diğerleri
Baskı/Yayın Bilgisi: (2019) -
Clustering of ultrahigh energy cosmic rays and their sources
Yazar:: Evans, N, ve diğerleri
Baskı/Yayın Bilgisi: (2003)