Automatic quenching of high energy gamma-ray sources by synchrotron photons
arXiv:astro-ph/0701633 · doi:10.1086/518417
Abstract
We investigate a magnetized plasma in which injected high energy gamma-rays annihilate on a soft photon field, that is provided by the synchrotron radiation of the created pairs. For a very wide range of magnetic fields, this process involves gamma-rays between 0.3 GeV and 30 TeV. We derive a simple dynamical system for this process, analyze its stability to runaway production of soft photons and paris, and find conditions for it to automatically quench by reaching a steady state with an optical depth to photon-photon annihilation larger than unity. We discuss applications to broad-band gamma-ray emitters, in particular supermassive black holes. Automatic quenching limits the gamma-ray luminosity of these objects and predicts substantial pair loading of the jets of less active sources.
11 pages, 2 figures included. Revised version, accepted for publication in ApJL
References in corpus (2)
Cited by in corpus (13)
- The Spitzer c2d Survey of Large, Nearby, Interstellar Clouds. XI. Lupus Observed With IRAC and MIPS
- The time-dependent one-zone hadronic model - First principles
- Mrk 421 as a case study for TeV and X-ray variability in leptohadronic models
- Radiation from relativistic jets in blazars and the efficient dissipation of their bulk energy via photon breeding
- Temporal signatures of leptohadronic feedback mechanisms in compact sources
- On proton synchrotron blazar models: the case of quasar 3C 279
- Implications of automatic photon quenching on compact gamma-ray sources
- Spectral evolution of non-thermal electron distributions in intense radiation fields
- Hadronic supercriticality as a trigger for GRB emission
- A numerical study of long-term multi-wavelength blazar variability
- A roadmap to hadronic supercriticalities: a comprehensive study of the parameter space for high-energy astrophysical sources
- Spontaneously quenched gamma-ray spectra from compact sources
- VHE gamma-ray Emission from Passive Supermassive Black Holes: Constraints for NGC 1399