Modeling Simulated Emissions from Galactic Binary Stars
High Energy Astrophysical Phenomena
2022-10-05 v1
Abstract
Relativistic plasma flows from the jets of black hole binary systems consist the environment of multiple particle production and radiation emission including neutrinos and gamma-rays. We implement a hadronic model based on interactions with the purpose of predicting the produced secondary particle distributions inside the jet. Our ultimate goal is the neutrino and gamma-ray intensities calculation while taking into account the most important gamma-ray absorption processes in order to present more realistic results.
Cite
@article{arxiv.2210.01188,
title = {Modeling Simulated Emissions from Galactic Binary Stars},
author = {Theodora V. Papavasileiou and Odysseas T. Kosmas and Ioannis Sinatkas},
journal= {arXiv preprint arXiv:2210.01188},
year = {2022}
}
Comments
6 pages, 6 figures