The Sixth Zeldovich meeting

GRB-SN Association within the Binary-Driven Hypernova Model

15 Jul 2026, 15:35

35m

ICRANet, Pescara, Italy

Invited talk Observations across electromagnetic spectrum: from gamma to radio

Speaker

Dr Yerlan Aimuratov (Fesenkov Astrophysical Institute)

Description

Observations of supernovae (SNe) Ic occurring after the prompt emission of long gamma-ray bursts (GRBs) are addressed within the binary-driven hypernova (BdHN) model, where GRBs originate from a binary composed of 10 solar masses carbon–oxygen (CO) star and a neutron star (NS). We report on recent progress in understanding the phenomenon and draw some prospects on GRB-SN research.