Articles Citing

Collapsar black hole spin evolution in 3D neutrino transport GRMHD simulations

Danat Issa1,2,*, Beverly Lowell1, Jonatan Jacquemin-Ide3,1, Matthew Liska4, and Alexander Tchekhovskoy1,5

  • 1Center for Interdisciplinary Exploration and Research in Astrophysics (CIERA), Physics and Astronomy, Northwestern University, Evanston, Illinois 60201, USA
  • 2MIT Kavli Institute for Astrophysics and Space Research, 77 Massachusetts Avenue, Cambridge, Massachusetts 02139, USA
  • 3JILA, University of Colorado and National Institute of Standards and Technology, 440 UCB, Boulder, Colorado 80309-0440, USA
  • 4Center for Relativistic Astrophysics, Georgia Institute of Technology, Howey Physics Building, 837 State Street Northwest, Atlanta, Georgia 30332, USA
  • 5NSF-Simons AI Institute for the Sky (SkAI), 172 East Chestnut Street, Chicago, Illinois 60611, USA

  • *Contact author: danat@mit.edu

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