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Spacetime Reconstruction from a Non-Relativistic Boundary
March 31, 20142:00 pm – 3:00 pm (CDT)

Spacetime Reconstruction from a Non-Relativistic Boundary

Speaker:

Cindy Keeler (University of Michigan)

Location:

Address:

Mitchell Institute for Fundamental Physics & Astronomy

College Station, Texas 77843

Event Details

We study the reconstructability of **(d+2)-**dimensional bulk spacetime from **(d+1)-**dimensional boundary data, particularly concentrating on backgrounds, which break **(d+1)-**dimensional Lorentz invariance. For a large class of such spacetimes, there exist null geodesics, which do not reach the boundary. Therefore classically one might guess some information is trapped in the bulk and thus invisible at the boundary. We show that this classical intuition correctly predicts the quantum situation: whenever there are null geodesics, which do not reach the boundary, there are also “trapped scalar modes” whose boundary imprint is exponentially suppressed. We use these modes to show that no smearing function exists for pure Lifshitz spacetime, nor for any flow, which includes a Lifshitz region. We will briefly comment on the corresponding insensitivity of the Green’s function to changes in **IR** boundary conditions, as well as on the situation in Schroedinger spacetimes.

Video Recording

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