We are excited to announce that this week's colloquium talk will be in 10-250 with a remote webcast option (details below).

Grab and go cookies + drinks and casual conversation Pappalardo Room 4-349 @ 3:45pm*

Geoff Penington

UC Berkeley

 
“Black holes, information and wormholes”

In the 1970s, Hawking showed that black holes are finite-temperature objects that radiate energy and eventually evaporate away entirely. However, his calculations suggested something very weird: that, unlike any other physical system, this radiation contained no information about the initial state of the black hole. Information that fell into the black hole appeared to be lost forever. This contradiction between Hawking's calculations and the ordinary rules of quantum mechanics has been a driving force behind much of the research in quantum gravity over the ensuing decades. Finally, in the last couple of years, we have begun to understand where Hawking's calculation went wrong, and to derive precise predictions, consistent with unitary quantum mechanics, for the information content of Hawking radiation. However, the new calculations, which involve weird spacetime topologies called 'spacetime wormholes', lead to as many new questions as answers...

*You must wear a mask unless actively taking a bite of food or a sip of a drink.