Astronomy and Astrophysics – Astrophysics
Scientific paper
2000-12-12
AIP Conf.Proc. 579 (2001) 53-57
Astronomy and Astrophysics
Astrophysics
5 pages; talk presented at First International Workshop on Radio Detection of High-Energy Particles (RADHEP-2000), UCLA, Los A
Scientific paper
10.1063/1.1398160
The temperature of the cosmic microwave background increases with redshift; at sufficiently high redshift it becomes possible for ultrahigh-energy photons and electrons to produce muons and pions through interactions with background photons. At the same time, energy losses due to interactions with radio background and intergalactic magnetic fields are negligible. The energetic muons and pions decay, yielding a flux of ``signature'' neutrinos with energies $E_\nu \sim 10^{17}$eV. Detection of these neutrinos can help understand the origin of ultrahigh-energy cosmic rays.
No associations
LandOfFree
"Signature" neutrinos from photon sources at high redshift does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with "Signature" neutrinos from photon sources at high redshift, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and "Signature" neutrinos from photon sources at high redshift will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-652149