Patterns of variability in supercritical hadronic systems
arXiv:1804.00188 · doi:10.1093/mnras/sty833
Abstract
A unique and often overlooked property of a source loaded with relativistic protons is that it can become supercritical, i.e. it can undergo an abrupt transition from a radiatively inefficient to a radiatively efficient state once its proton energy density exceeds a certain threshold. In this paper, we investigate the temporal variability of hadronic systems in this hardly explored regime. We show that there exists a range of proton densities that prevent the system from reaching a steady state, but drive it instead in a quasi-periodic mode. The escaping radiation then exhibits limit cycles, even if all physical parameters are held constant in time. We extend our analysis to cases where the proton injection rate varies with time and explore the variability patterns of escaping radiation as the system moves in and out from the supercritical regime. We examine the relevance of our results to the variability of the prompt gamma-ray burst emission and show that, at least on a phenomenological level, some interesting analogies exist.
10 pages, 7 figures, accepted for publication in MNRAS
References in corpus (5)
- Photohadronic origin of -ray BL Lac emission: implications for IceCube neutrinos
- Search for Prompt Neutrino Emission from Gamma-Ray Bursts with IceCube
- Prompt GeV-TeV Emission of Gamma-Ray Bursts Due to High-Energy Protons, Muons and Electron-Positron Pairs
- Implications of a PeV neutrino spectral cutoff in GRB models
- Hadronic supercriticality as a trigger for GRB emission
Cited by in corpus (6)
- Multi-Epoch Modeling of TXS 0506+056 and Implications for Long-Term High-Energy Neutrino Emission
- AM: An Open-Source Tool for Time-Dependent Lepto-Hadronic Modeling of Astrophysical Sources
- A marginally fast-cooling proton-synchrotron model for prompt GRBs
- A roadmap to hadronic supercriticalities: a comprehensive study of the parameter space for high-energy astrophysical sources
- Inductive acceleration of ions in Poynting-flux dominated outflows
- Hadronic supercriticality in spherically expanding sources: application to GRB prompt emission