Multimessenger Emission from Microquasars Modeled

This paper investigates the multimessenger emission from microquasars, focusing on high-energy gamma rays and neutrinos. It uses the AMES simulator to model the emission, considering different interaction scenarios and emission region configurations. The study's significance lies in its ability to explain observed TeV and PeV gamma-ray detections and provide testable predictions for future observations, particularly in the 0.1-10 TeV range. The paper also explores the variability and neutrino emission from these sources, offering insights into their complex behavior and detectability.