Princeton University Gravity Initiative Seminar Series

Bob in a Black Hole, or: On Decoherence from Horizons

Abstract: Recently it was shown that black holes impart a fundamental rate of decoherence on all nearby quantum superpositions [Danielson, Satishchandran, Wald (DSW) 2022], eventually erasing all quantum information in their vicinity.  The effect can be understood from measurement and causality: An observer (Bob) in the black hole should be able to disturb outside quantum superpositions by measuring their superposed gravitational fields, but since his actions cannot (by causality) have this effect, the superpositions must automatically disturb themselves!  DSW calculated the rate of decoherence up to an unknown numerical factor for distant observers in Schwarzschild spacetime.  Working in the electromagnetic analog, we flesh out and generalize their calculation to obtain the precise decoherence rate for an observer at an arbitrary location on the symmetry axis of a Kerr black hole.  We find that the decoherence vanishes entirely in the extremal limit, due to the "Black hole Meissner effect" screening the Coulomb field from entering the black hole.  This supports the causality picture: Since Bob is unable to measure the field of the outside superposition, no decoherence is necessary--and indeed none occurs.

Date & Time

March 04, 2024 | 12:30pm – 1:30pm

Location

Princeton University, Jadwin Hall, Princeton Gravity Initiative, 4th Floor

Speakers

Sam Gralla, University of Arizona