Speaker
Yu Wang
Description
Binary driven hypernova (BdHN) models long gamma-ray bursts (GRBs) as occurring in the binary systems involving a carbon-oxygen core and a companion compact star. This model, first proposed in 2012, succeeds and improves upon the fireshell model and the induced gravitational collapse paradigm. After nearly a decade of development, the BdHN model has reached a nearly mature structure. In this talk, on behalf of the group, I will present a summary of the BdHN model and the physical processes at work in each of the episodes during its occurrence and lifetime, and to give examples by GRB 180728A and 190829A.
Primary author
Yu Wang
