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Patterns of variability in supercritical hadronic systems

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arxiv 1804.00188 v1 pith:DHMEN2YN submitted 2018-03-31 astro-ph.HE

classification astro-ph.HE
keywords variabilityprotonsupercriticalescapinghadronicpatternsradiationradiatively
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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.

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Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Inductive acceleration of ions in Poynting-flux dominated outflows

    astro-ph.HE 2019-08 accept novelty 6.0 of 10

    Adding ions to a magnetized relativistic wind lets inductive acceleration push both ions and leptons to Hillas-limit energies in a shorter distance than lepton-only winds.

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