
The neutrino-dominated accretion flow (NDAF) model successfully explains the observed blackbody components in the gamma-ray burst (GRB) spectra, supporting the theory that these bursts are powered by a black hole engine.


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testing-the-neutrino-dominated-accretion-flow-model-of-gamma-ray-bursts-using-blackbody-components


Testing the Neutrino-Dominated Accretion Flow Model of Gamma-Ray Bursts Using Blackbody Components


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Close binary star systems with black hole accretion disk engines offer a compelling explanation for the formation of long-duration gamma-ray bursts (lGRBs), low-luminosity GRBs, ultra-long GRBs, and broad-lined Type Ic supernovae (Ic-BL SNe).


the-formation-of-long-duration-gamma-ray-bursts-and-broad-lined-supernovae-from-close-binary-stars-with-black-hole-engines


The Formation of Long-Duration Gamma-Ray Bursts and Broad-Lined Supernovae from Close Binary Stars with Black Hole Engines
