Simulations of Gamma-Ray Emission from Magnetized Microquasar Jets

In this work, we simulate γ-rays created in the hadronic jets of the compact object in binary stellar systems known as microquasars. We utilize as the main computational tool the 3D relativistic magnetohydrodynamical code PLUTO combined with in-house derived codes. Our simulated experiments refer to...

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Main Authors: Odysseas Kosmas, Theodoros Smponias
Format: Article
Language:English
Published: Wiley 2018-01-01
Series:Advances in High Energy Physics
Online Access:http://dx.doi.org/10.1155/2018/9602960
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author Odysseas Kosmas
Theodoros Smponias
author_facet Odysseas Kosmas
Theodoros Smponias
author_sort Odysseas Kosmas
collection DOAJ
description In this work, we simulate γ-rays created in the hadronic jets of the compact object in binary stellar systems known as microquasars. We utilize as the main computational tool the 3D relativistic magnetohydrodynamical code PLUTO combined with in-house derived codes. Our simulated experiments refer to the SS433 X-ray binary, a stellar system in which hadronic jets have been observed. We examine two new model configurations that employ hadron-based emission mechanisms. The simulations aim to explore the dependence of the γ-ray emissions on the dynamical as well as the radiative properties of the jet (hydrodynamic parameters of the mass-flow density, gas-pressure, temperature of the ejected matter, high energy proton population inside the jet plasma, etc.). The results of the two new scenarios of initial conditions for the microquasar stellar system studied are compared to those of previously considered scenarios.
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spelling doaj-art-32c0f601f66245beaf7998cea6e82b052025-02-03T06:15:13ZengWileyAdvances in High Energy Physics1687-73571687-73652018-01-01201810.1155/2018/96029609602960Simulations of Gamma-Ray Emission from Magnetized Microquasar JetsOdysseas Kosmas0Theodoros Smponias1Modelling and Simulation Centre, MACE, University of Manchester, Sackville Street, Manchester, UKDivision of Theoretical Physics, University of Ioannina, 45110 Ioannina, GreeceIn this work, we simulate γ-rays created in the hadronic jets of the compact object in binary stellar systems known as microquasars. We utilize as the main computational tool the 3D relativistic magnetohydrodynamical code PLUTO combined with in-house derived codes. Our simulated experiments refer to the SS433 X-ray binary, a stellar system in which hadronic jets have been observed. We examine two new model configurations that employ hadron-based emission mechanisms. The simulations aim to explore the dependence of the γ-ray emissions on the dynamical as well as the radiative properties of the jet (hydrodynamic parameters of the mass-flow density, gas-pressure, temperature of the ejected matter, high energy proton population inside the jet plasma, etc.). The results of the two new scenarios of initial conditions for the microquasar stellar system studied are compared to those of previously considered scenarios.http://dx.doi.org/10.1155/2018/9602960
spellingShingle Odysseas Kosmas
Theodoros Smponias
Simulations of Gamma-Ray Emission from Magnetized Microquasar Jets
Advances in High Energy Physics
title Simulations of Gamma-Ray Emission from Magnetized Microquasar Jets
title_full Simulations of Gamma-Ray Emission from Magnetized Microquasar Jets
title_fullStr Simulations of Gamma-Ray Emission from Magnetized Microquasar Jets
title_full_unstemmed Simulations of Gamma-Ray Emission from Magnetized Microquasar Jets
title_short Simulations of Gamma-Ray Emission from Magnetized Microquasar Jets
title_sort simulations of gamma ray emission from magnetized microquasar jets
url http://dx.doi.org/10.1155/2018/9602960
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