Patterns of variability in supercritical hadronic systems

@article{Petropoulou2018PatternsOV,
  title={Patterns of variability in supercritical hadronic systems},
  author={Maria Petropoulou and Apostolos Mastichiadis},
  journal={Monthly Notices of the Royal Astronomical Society},
  year={2018},
  volume={477},
  pages={2917-2925}
}
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… 

Figures and Tables from this paper

The Onset of Hadronic Supercriticality in ExpandingSources

An overlooked property of hadronic models is that they can become supercritical by abruptly transforming the energy stored in the relativistic protons into radiation. Supercriticality manifests

A roadmap to hadronic supercriticalities: a comprehensive study of the parameter space for high-energy astrophysical sources

Hadronic supercriticalities are radiative instabilities that appear when large amounts of energy are stored in relativistic protons. When the proton energy density exceeds some critical value, a

An expanding hadronic supercritical model for $-ray burst emission

Relativistic hadronic plasmas have an intriguing property, coined as hadronic supercriticality, according to which they can abruptly and efficiently release the energy stored in protons through

A marginally fast-cooling proton–synchrotron model for prompt GRBs

A small fraction of gamma-ray bursts (GRBs) with available data down to soft X-rays (∼0.5 keV) has been shown to feature a spectral break in the low-energy part (∼1–10 keV) of their prompt emission

Inductive Acceleration of Ions in Poynting-flux-dominated Outflows

Two-fluid (electron–positron) plasma modeling has shown that inductive acceleration can convert Poynting flux directly into bulk kinetic energy in the relativistic flows driven by rotating magnetized

Multi-epoch Modeling of TXS 0506+056 and Implications for Long-term High-energy Neutrino Emission

The IceCube report of a excess of 13 ± 5 neutrino events in the direction of the blazar TXS 0506+056 in 2014–2015 and the 2017 detection of a high-energy neutrino event, IceCube-170922A, during a

References

SHOWING 1-10 OF 32 REFERENCES

Hadronic supercriticality as a trigger for γ-ray burst emission

We explore a one-zone hadronic model that may be able to reproduce $\gamma$-ray burst (GRB) prompt emission with a minimum of free parameters. Assuming only that GRBs are efficient high-energy proton

Temporal signatures of leptohadronic feedback mechanisms in compact sources

The hadronic model of active galactic nuclei and other compact high-energy astrophysical sources assumes that ultra-relativistic protons, electron–positron pairs and photons interact via various

Spectral and temporal signatures of ultrarelativistic protons in compact sources. I. Effects of Bethe-Heitler pair production

We present calculations of the spectral and temporal radiative signatures expected from ultrarelativistic protons in compact sources. The coupling between the protons and the leptonic component is

The “Supercritical Pile” Model for Gamma-Ray Bursts: Getting the νFν Peak at 1 MeV

We propose that the internal energy of the gamma-ray burst (GRB) blast waves, thought to be stored in the form of relativistic protons comoving with the blast wave, is converted explosively (i.e., on

The time-dependent one-zone hadronic model: first principles

We present a time-dependent approach to the one-zone hadronic model in the case where the photon spectrum is produced by ultrarelativistic protons interacting with soft photons that are produced from

Mrk 421 as a case study for TeV and X-ray variability in leptohadronic models

We investigate the origin of high-energy emission in blazars within the context of the leptohadronic one-zone model. We find that γ -ray emission can be attributed to synchrotron radiation either

Individual power density spectra of Swift gamma-ray bursts

Context. Timing analysis can be a powerful tool with which to shed light on the still obscure emission physics and geometry of the prompt emission of gamma-ray bursts (GRBs). Fourier power density

THE ROLE OF STOCHASTIC ACCELERATION IN THE PROMPT EMISSION OF GAMMA-RAY BURSTS: APPLICATION TO HADRONIC INJECTION

We study effects of particle re-acceleration (or heating) in the post-shock region via magnetohydrodynamic/plasma turbulence, in the context of a mixed hadronic–leptonic model for the prompt emission

On proton synchrotron blazar models: the case of quasar 3C 279

In this work we propose an innovative estimation method for the minimum Doppler factor and energy content of the γ-ray emitting region of quasar 3C 279, using a standard proton synchrotron blazar