Recent progress in our understanding of black hole evaporation has mostly occurred in the context of black holes coupled to an external, non-gravitating bath. In order to compare and contrast to what happens to black holes in asymptotically flat space it is imperative to understand whether the non-gravitating bath is just some external spectator or actively changes the physics in this system. Equivalently, one can wonder to what extent the results generalize to the case of a gravitating bath. We use Randall-Sundrum braneworlds, and their holographic interpretation, to answer this important question.
Please register at docs.google.com/forms/d/e/1FAIpQLSf0jLgoqiOgDnxbEBGiuIWiOmh9WX8caH-pr13qDBZOO91lmg/viewform (Links to join the seminars will be sent to your registered email address.)
Recordings of past talks can be found here: www.youtube.com/channel/UCw9LdPQ5t7Q7muD0qzn70TA