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.
Please click on the link https://zoom.us/j/99198634658?pwd=VDFPRXhYTkVqUkVLQnFuRExjQVl2Zz09 to join the meeting
Meeting ID: 991 9863 4658
Recordings of past talks can be found here: https://www.youtube.com/channel/UCw9LdPQ5t7Q7muD0qzn70TA