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SUMMARY:Nonlinear stability of extremal Reissner–Nordström black holes 
 in spherical symmetry - Ryan Unger (Stanford)
DTSTART:20241014T130000Z
DTEND:20241014T140000Z
UID:TALK222634@talks.cam.ac.uk
CONTACT:Dr Greg Taujanskas
DESCRIPTION:Extremal black holes are exceptional solutions of Einstein’s
  equations that arise on the phase transition between gravitational collap
 se and dispersion. In this talk\, I will discuss forthcoming work proving 
 the codimension-one nonlinear asymptotic stability of the extremal Reissne
 r–Nordström family of black holes in the spherically symmetric Einstein
 –Maxwell-neutral scalar field model\, up to and including the event hori
 zon. This work rigorously confirms numerical results of Murata—Reall—T
 anahashi from 2013. Joint work with Yannis Angelopoulos (Caltech) and Chri
 stoph Kehle (MIT). 
LOCATION:MR13
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