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DTSTART:19700308T020000
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BEGIN:VEVENT
DTSTAMP:20260202T201803Z
LOCATION:Art of HPC - Plaza Lobby
DTSTART;TZID=America/Chicago:20251116T080000
DTEND;TZID=America/Chicago:20251116T180000
UID:submissions.supercomputing.org_SC25_sess601_art117@linklings.com
SUMMARY:A Ravenous, Spinning Black Hole: Infall to Outflow
DESCRIPTION:Joseph A. Insley (Argonne National Laboratory (ANL)), Lizhong 
 Zhang and Christopher White (CCA at Flatiron Institute), and Kyle Felker (
 Argonne National Laboratory (ANL))\n\nGlobal view of super-Eddington accre
 tion onto a spinning stellar-mass black hole. The black hole is surrounded
  by a geometrically thick, dense accretion disk of hot plasma, mostly supp
 orted by radiation pressure against gravity. This puffy disk forms a spira
 ling structure as it falls inward and emits X-ray radiation. Relativistic 
 jets, driven by the interaction between electromagnetic fields and black h
 ole spin, are launched from the inner polar region and can propagate over 
 extreme distances. The system resembles ultraluminous X-ray sources (ULXs)
 , which are thought to be powered by such super-Eddington disks.\n\nTag: A
 rt of HPC\n\nRecording: Not Livestreamed, Not Recorded\n\nRegistration Cat
 egory: Technical Program Reg Pass, Workshop Reg Pass, Tutorial Reg Pass, E
 xhibits Reg Pass\n\n
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