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Akhil Sivakumar (International Centre for Theoretical Science - TIFR, Bangalore)
Date & Time
Wed, 18 November 2020, 11:00 to 12:30
ICTS virtual seminar

Blackholes are interesting mainly due to two reasons. The first is that they give rise to irreversible dynamics - event horizons mark a region of no return. Secondly they produce Hawking radiation. While the first dissipative behaviour is well studied, the physics of fluctuations or Hawking radiation is not. In this talk I will present preliminary results on understanding the real-time Hawking fluctuations around an AdS blackbrane. The techniques we develop give a clean separation of short lived and long lived dynamics of the blackbrane.

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Recordings of past talks can be found here: