GENERAL RELATIVISTIC MHD SIMULATIONS OF BLACK HOLE ACCRETION
GENERAL RELATIVISTIC MHD SIMULATIONS OF BLACK HOLE ACCRETION. with: Kris Beckwith, Jean-Pierre De Villiers, John Hawley, Shigenobu Hirose, Scott Noble, and Jeremy Schnittman. Stellar Structure Basic problem: generation of heat Before 1939, no mechanism, reliance on scaling laws
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