Gamma-ray bursts as VHE-UHE sources

Peter Mészáros

Research output: Contribution to journalArticlepeer-review


Gamma-ray bursts are capable of accelerating cosmic rays up to GZK energies Ep ∼ 1020 eV, which can lead to a flux at Earth comparable to that observed by large EAS arrays such as Auger. The semi-relativistic outflows inferred in GRB-related hypernovae are also likely sources of somewhat lower energy cosmic rays. Leptonic processes, such as synchrotron and inverse Compton, as well as hadronic processes, can lead to GeV-TeV gamma-rays measurable by GLAST, AGILE, or ACTs, providing useful probes of the burst physics and model parameters. Photo-meson interactions also produce neutrinos at energies ranging from sub-TeV to EeV, which will be probed with forthcoming experiments such as IceCube, ANITA and KM3NeT. This would provide information about the fundamental interaction physics, the acceleration mechanism, the nature of the sources and their environment.

Original languageEnglish (US)
Pages (from-to)1319-1332
Number of pages14
JournalInternational Journal of Modern Physics D
Issue number9
StatePublished - Sep 2008

All Science Journal Classification (ASJC) codes

  • Mathematical Physics
  • Astronomy and Astrophysics
  • Space and Planetary Science


Dive into the research topics of 'Gamma-ray bursts as VHE-UHE sources'. Together they form a unique fingerprint.

Cite this