Modeling Simulated Emissions from Galactic Binary Stars

TL;DR

This paper develops a hadronic model to predict neutrino and gamma-ray emissions from black hole binary jets, incorporating particle interactions and absorption processes for realistic intensity estimates.

Contribution

It introduces a comprehensive hadronic model for jet emissions that accounts for particle interactions and gamma-ray absorption, improving prediction accuracy.

Findings

Predicted neutrino and gamma-ray intensities from black hole binary jets.

Incorporated gamma-ray absorption processes into emission modeling.

Enhanced realism in emission predictions for astrophysical jets.

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.