Magnetic horizons of ultra-high energy cosmic rays
The propagation of ultra-high energy cosmic rays in extragalactic magnetic fields can be diffusive, depending on the strength and properties of the fields. In some cases the propagation time of the particles can be comparable to the age of the universe, causing a suppression in the flux measured on...
Main Authors: | Batista, R, Sigl, G |
---|---|
Format: | Conference item |
Published: |
Deutsches Elektronen-Synchrotron
2014
|
Similar Items
-
On the measurement of the helicity of intergalactic magnetic fields using ultra-high-energy cosmic rays
by: Alves Batista, R, et al.
Published: (2019) -
Implications of strong intergalactic magnetic fields
for ultrahigh-energy cosmic-ray astronomy
by: Batista, R, et al.
Published: (2017) -
The Anisotropy of the Ultra-High Energy Cosmic Rays
by: Evans, W, et al.
Published: (2001) -
The propagation of ultra high energy cosmic rays
by: Taylor, A, et al.
Published: (2007) -
Ultra-high energy cosmic rays and new physics
by: Sarkar, S
Published: (2002)