BEGIN:VCALENDAR
VERSION:2.0
PRODID:-//CERN//INDICO//EN
BEGIN:VEVENT
SUMMARY:Causal Space-Time Structure and non-Hausdorff Extension of Schwarz
 schild Black Hole Interior
DTSTART;VALUE=DATE-TIME:20261030T095000Z
DTEND;VALUE=DATE-TIME:20261030T100500Z
DTSTAMP;VALUE=DATE-TIME:20261026T233033Z
UID:indico-contribution-6268@cern.ch
DESCRIPTION:Speakers: Asya Aynbund (MIPT)\nCones of future and past are ri
 gorously constructed under the horizon of black hole by completions of geo
 desics continued from causally connected space-time regions outside the bl
 ack hole interior. Treating the Schwarzschild black hole as a zero charge 
 limit of Reissner—Nordsrom black hole reforms the Penrose—Carter diagr
 am into the infinite band that excludes the closed proper-time cycles unde
 r the  geodesic motion. The marginal trajectories between the cones of fut
 ure and past compose paths common with a compact non-Hausdorff spherical e
 xtension of black hole interior forming the thermal bath for particles fal
 len to the black hole.\n\nhttps://indico.particle.mephi.ru/event/626/contr
 ibutions/6268/
LOCATION: Conference Hall 1
URL:https://indico.particle.mephi.ru/event/626/contributions/6268/
END:VEVENT
END:VCALENDAR