Modeling Simulated Emissions from Galactic Binary Stars

Theodora V. Papavasileiou; Odysseas T. Kosmas; Ioannis Sinatkas

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arXiv · 2210.01188

Modeling Simulated Emissions from Galactic Binary Stars

Theodora V. Papavasileiou·Odysseas T. Kosmas·Ioannis Sinatkas

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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 $p-p$ 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.

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Theodora V. Papavasileiou, Odysseas T. Kosmas, Ioannis Sinatkas. 2022-10-03. Modeling Simulated Emissions from Galactic Binary Stars. https://arxiv.org/abs/2210.01188

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