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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Wiley
2018-01-01
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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. |
format | Article |
id | doaj-art-32c0f601f66245beaf7998cea6e82b05 |
institution | Kabale University |
issn | 1687-7357 1687-7365 |
language | English |
publishDate | 2018-01-01 |
publisher | Wiley |
record_format | Article |
series | Advances in High Energy Physics |
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 |
work_keys_str_mv | AT odysseaskosmas simulationsofgammarayemissionfrommagnetizedmicroquasarjets AT theodorossmponias simulationsofgammarayemissionfrommagnetizedmicroquasarjets |