High energy emissions from gamma-ray bursts

Details High energy emissions from gamma-ray bursts High energy emissions from gamma-ray bursts

Mar 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007jphcs..60..111r&link_type=abstract

Journal of Physics: Conference Series, Volume 60, Issue 1, pp. 111-114 (2007).

Physics

1

Scientific paper

Gamma-ray bursts are the brightest transient sources of MeV γ-rays in the sky and are the leading candidate sources of the GZK cosmic rays. Physical conditions required to accelerate elementary particles to such high energies also, inevitably, lead to expected TeV energy γ-ray and neutrino emission from these sources. Although γ-rays of energy only up to 18 GeV have been detected from a few bursts, upcoming space- and ground-based detectors will probe these sources in the GeV-TeV energy range revealing their particle acceleration and emission mechanism(s) as well as constraining their astrophysical model(s).

Affiliated with

Also associated with

No associations

Rating

High energy emissions from gamma-ray bursts 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 emissions from gamma-ray bursts, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and High energy emissions from gamma-ray bursts will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-924332