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SUMMARY:Does Hawking Radiation Survive Beyond the Scrambling Time?
DTSTART;VALUE=DATE-TIME:20260722T080000Z
DTEND;VALUE=DATE-TIME:20260722T091500Z
DTSTAMP;VALUE=DATE-TIME:20260704T084338Z
UID:indico-event-228@indico.nitep.omu.ac.jp
DESCRIPTION:Date: July 22\, 2026\nTime: 17:00-18:15\nPlace: 理学部E棟1
 階E101室\n\nSpeaker:  Wei-Hsiang Shao (RIKEN iTHEMS)\nTitle: Does Hawki
 ng Radiation Survive Beyond the Scrambling Time?\n\nAbstract:\nIt is widel
 y assumed that the standard Hawking radiation persists as long as a black 
 hole remains much larger than the Planck length. In this talk\, I will exp
 lore how UV physics can nevertheless dramatically modify the conventional 
 properties of Hawking radiation\, even in this semiclassical regime.\nIn p
 articular\, I will show that nonlocal UV features expected in quantum grav
 ity (and especially in string theory) can render Hawking radiation a trans
 ient phenomenon that is largely suppressed after the scrambling time\, muc
 h earlier than the conventionally expected black hole lifetime. This sugge
 sts a major departure from the usual picture of black hole evaporation and
  may offer fresh insight into alternative resolutions of the information p
 aradox.\n\nhttps://indico.nitep.omu.ac.jp/event/228/
LOCATION:
URL:https://indico.nitep.omu.ac.jp/event/228/
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