Multimessenger Emission from Microquasars Modeled
Published:Dec 29, 2025 06:19
•1 min read
•ArXiv
Analysis
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.
Key Takeaways
- •Models explain observed TeV and PeV gamma-ray detections from microquasars.
- •Predictions are made for the 0.1-10 TeV energy range, offering testable scenarios.
- •Variability and neutrino emission are explored, providing insights into source behavior.
Reference
“The paper predicts unique, observationally testable predictions in the 0.1-10 TeV energy range, where current observations provide only upper limits.”