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We will review progress over the last 15 years on a new form of gravitational entropy, that extends the traditional Bekenstein-Hawking entropy of black holes. This has lead to a new result for the entropy of Hawking radiation which is in agreement with information preservation, as opposed to information loss. It also gives a new picture for how to think about the interior of a black hole.
Zoom connection info:
https://cern.zoom.us/j/92295382938?pwd=aVd6dUt2OE1lRWZNempYWVMyWUludz09
Meeting ID: 922 9538 2938
Password: 465395