GRBs as Ultra-High Energy Cosmic Ray Sources: Clues From Fermi
Abstract
If gamma-ray bursts are sources of ultra-high energy cosmic rays then radiative signatures of hadronic acceleration are expected in GRB data. Observations with the Fermi Gamma-ray Space Telescope (Fermi) offer the best means to search for evidence of UHECRs in GRBs through electromagnetic channels. Various issues related to UHECR acceleration in GRBs are reviewed, with a focus on the question of energetics.
Document Details
- Document Type
- Technical Report
- Publication Date
- Mar 27, 2010
- Accession Number
- ADA522743
Entities
People
- C. Dermer
Organizations
- United States Naval Research Laboratory