Astrophysical High Energy Neutrinos

Details Astrophysical High Energy Neutrinos Astrophysical High Energy Neutrinos

Nov 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007aipc..944..130r&link_type=abstract

NEXT GENERATION NUCLEON DECAY AND NEUTRINO DETECTORS: NNN06. AIP Conference Proceedings, Volume 944, pp. 130-139 (2007).

Astronomy and Astrophysics

Astrophysics

Gamma-Ray Sources, Gamma-Ray Bursts, Cosmic Rays, Supernovae, Neutrino Mass And Mixing

Scientific paper

Astrophysical candidate sources of ultrahigh-energy cosmic-rays are also expected to produce high-energy neutrinos in situ and around their acceleration sites by interacting with abundant soft photons or nucleons. Detection of these neutrinos then may identify the yet unknown sources of the cosmic rays. I discuss different models of high-energy neutrino signals from astrophysical objects such as gamma-ray bursts and hyper-novae, and how detection/non-detection of these astronomical messengers may constrain the source models. I also discuss the detectability of these neutrinos in upcoming neutrino telescopes and how flavor tagging may be used to learn about the astrophysics of the sources.

Affiliated with

Also associated with

No associations

Rating

Astrophysical High Energy Neutrinos 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 Astrophysical High Energy Neutrinos, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Astrophysical High Energy Neutrinos will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1696113