Speaker
Jose Carpio Dumler
Description
Microquasars, compact binary systems with an accreting stellar-mass black hole or neutron star, are promising candidates for high-energy particle acceleration. Recently, LHAASO reported the detection of 5 microquasars emitting $>100$ TeV $\gamma$-rays, suggesting that these sources are efficient particle accelerators. High-energy $\gamma$-rays can be achieved in large-scale jets or winds. In this work, we explore the X-ray, $\gamma$-ray and neutrino emission from SS433, V4641 Sgr and GRS 1905+105. We consider leptonic and hadronic models to explain the spectra observed by LHAASO and other high-energy $\gamma$-ray detectors. We also study neutrino detection prospects from the hadronic component.
Author
Co-authors
Ali Kheirandish
Bing Zhang
(UNLV)
