Density Profiles of Collapsed Rotating Massive Stars Favor Long Gamma-Ray Bursts

Density Profiles of Collapsed Rotating Massive Stars Favor Long Gamma-Ray Bursts

Long-duration gamma-ray bursts (lGRBs) originate in relativistic collimated outflows—jets—that drill their way out of collapsing massive stars. Accurately modeling this process requires realistic stellar profiles for the jets to propagate through and break out of. Most previous studies have used sim...

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Bibliographic Details
Main Authors:	Goni Halevi, Belinda Wu, Philipp Mösta, Ore Gottlieb, Alexander Tchekhovskoy, David R. Aguilera-Dena
Format:	Article
Language:	English
Published:	IOP Publishing 2023-01-01
Series:	The Astrophysical Journal Letters
Subjects:	Hydrodynamical simulations General relativity Stellar mass black holes Gamma-ray bursts Core-collapse supernovae
Online Access:	https://doi.org/10.3847/2041-8213/acb702

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