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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:20260706T071815Z
UID:indico-event-230@indico.nitep.omu.ac.jp
DESCRIPTION:Date: July 22\, 2026\nTime: 17:00-18:15\nPlace: 杉本キャ
 ンパス 理学部E棟1階E101室\n(This is an on-site seminar\, and wil
 l not be broadcasted on Zoom.)\n\nSpeaker:  Wei-Hsiang Shao (RIKEN iTHEMS
 )\nTitle: Does Hawking Radiation Survive Beyond the Scrambling Time?\n\nAb
 stract:\nIt is widely assumed that the standard Hawking radiation persists
  as long as a black hole remains much larger than the Planck length. In th
 is talk\, I will explore how UV physics can nevertheless dramatically modi
 fy the conventional properties of Hawking radiation\, even in this semicla
 ssical regime.\nIn particular\, I will show that nonlocal UV features expe
 cted in quantum gravity (and especially in string theory) can render Hawki
 ng radiation a transient phenomenon that is largely suppressed after the s
 crambling time\, much earlier than the conventionally expected black hole 
 lifetime. This suggests a major departure from the usual picture of black 
 hole evaporation and may offer fresh insight into alternative resolutions 
 of the information paradox.\n\nhttps://indico.nitep.osaka-cu.ac.jp/event/2
 30/
LOCATION:
URL:https://indico.nitep.osaka-cu.ac.jp/event/230/
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