References
Method paper
If grplinst contributes to your work, please cite:
“Simulations of Electromagnetic Cascades in the Intergalactic Medium with Plasma Instabilities: the
grplinstcode”
R. Alves Batista, A. Saveliev
[doi] || [arXiv]
The citation for the first version of the code, much simpler than the current design, is this:
“The impact of plasma instabilities on the spectra of TeV blazars”
R. Alves Batista, A. Saveliev, E. M. de Gouveia Dal Pino
Monthly Notices of the Royal Astronomical Society 2019, 489, 3836
[doi] || [arXiv]
Implemented model prescriptions
Each row corresponds to a PlasmaInstability* class (see Models).
Bret et al. 2010
“Multidimensional electron beam-plasma instabilities in the relativistic regime”
A. Bret, L. Gremillet, M. E. Dieckmann
Physics of Plasmas, 2010, 17, 12
[doi]
Broderick et al. 2012
“The Cosmological Impact of Luminous TeV Blazars. I. Implications of Plasma Instabilities for the Intergalactic Magnetic Field and Extragalactic Gamma-Ray Background”
A. E. Broderick, P. Chang, C. Pfrommer
The Astrophysical Journal, 2012, 752, 1
[arXiv] | [doi]
Schlickeiser et al. 2012
“Plasma Effects on Fast Pair Beams in Cosmic Voids”
R. Schlickeiser, D. Ibscher, M. Supsar
The Astrophysical Journal, 2012, 758
[doi]
Miniati & Elyiv 2013
“Relaxation of Blazar-induced Pair Beams in Cosmic Voids”
F. Miniati, A. Elyiv
The Astrophysical Journal, 2013, 770, 1
[arXiv] | [doi]
Sironi et al. 2014
“Relativistic Pair Beams from TeV Blazars: A Source of Reprocessed GeV Emission rather than Intergalactic Heating”
L. Sironi, D. Giannios
The Astrophysical Journal, 2014, 787, 1
[arXiv] | [doi]
Vafin et al. 2018
“The Electrostatic Instability for Realistic Pair Distributions in Blazar/EBL Cascades”
S. Vafin, I. Rafighi, M. Pohl, J. Niemiec
The Astrophysical Journal, 2018, 857, 1
[arXiv] | [doi]
Shalaby et al. 2020
“The growth of the longitudinal beam-plasma instability in the presence of an inhomogeneous background”
M. Shalaby, A. E. Broderick, P. Chang, C. Pfrommer, E. Puchwein, A. Lamberts
Journal of Plasma Physics, 2020, 86, 2
[doi] | [arXiv]