High Energy Neutrinos from Charm in Astrophysical Sources

Details High Energy Neutrinos from Charm in Astrophysical Sources High Energy Neutrinos from Charm in Astrophysical Sources

Dec 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aipc.1182...40s&link_type=abstract

10TH CONFERENCE ON THE INTERSECTIONS OF PARTICLE AND NUCLEAR PHYSICS. AIP Conference Proceedings, Volume 1182, pp. 40-43 (2009)

Astronomy and Astrophysics

Astronomy

Neutrinos, Astronomy, Supernovae, Neutrino, Muon, Pion, And Other Elementary Particles, Cosmic Rays, Astronomical Catalogs, Atlases, Sky Surveys, Databases, Retrieval Systems, Archives, Etc., Supernovae

Scientific paper

We show that charm provides significant enhancement of the very high energy neutrino flux, when neutrinos originate in astrophysical sources with jets driven by central engines, such as gamma ray bursts or supernovae with jets. The neutrino flux from semi-leptonic decays of charmed mesons is subject to much less hadronic and radiative cooling than the conventional flux from pion and kaon decays and therefore has a dominant contribution at higher energies, of relevance to future ultrahigh energy neutrino experiments.

Affiliated with

Also associated with

No associations

Rating

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

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1881921