Pointlike Gamma Ray Sources as Signatures of Distant Accelerators of Ultrahigh Energy Cosmic Rays
Abstract
We discuss the possibility of observing distant accelerators of ultrahigh energy cosmic rays in synchrotron gamma rays. Protons propagating away from their acceleration sites produce extremely energetic electrons during photopion interactions with cosmic microwave background photons. If the accelerator is embedded in a magnetized region, these electrons will emit high energy synchrotron radiation. The resulting synchrotron source is expected to be pointlike, steady, and detectable in the GeV-TeV energy range if the magnetic field is at the nanoGauss level.
- Publication:
-
Physical Review Letters
- Pub Date:
- December 2005
- DOI:
- 10.1103/PhysRevLett.95.251102
- arXiv:
- arXiv:astro-ph/0505462
- Bibcode:
- 2005PhRvL..95y1102G
- Keywords:
-
- 98.70.Sa;
- 98.70.Rz;
- Cosmic rays;
- gamma-ray sources;
- gamma-ray bursts;
- Astrophysics
- E-Print:
- 4 pages 2 figures. To be published in PRL