The Geodesics Less Traveled: Nonminimal RT Surfaces and Holographic Scattering
Jacqueline Caminiti, Caroline Lima, Robert C. Myers
TL;DR
This work clarifies when bulk scattering in holography can be diagnosed purely from boundary entanglement. It proves that in pure $AdS_3$ the 2-to-2 converse to the connected wedge theorem holds: a connected entanglement wedge is necessary and sufficient for bulk $2\to2$ scattering, and this extends to a broad class of asymptotically $AdS_3$ vacuum geometries via local AdS$_3$ regions. The analysis, including a shell model with interior AdS$_3$ and exterior conical defects, shows that matter can disrupt this tight relation, with simple counterexamples where nonminimal RT surface inequalities fail to imply scattering. For higher $n$-to-$n$ scattering, the authors show there is no general converse even in pure $AdS_3$: the threshold conditions do not align with RT-phase boundaries except in select cases (e.g., $n=2$, or $n=3$ with special angular arrangements). Overall, the results delineate the limits of the CWT as a diagnostic for bulk scattering and motivate refined boundary-entanglement diagnostics, potentially through focusing arguments or new surface constructs like a proposed $ ilde{u}$, with implications for entwinement and holographic reconstruction.
Abstract
The connected wedge theorem states that in order to have a scattering process in the bulk, it is necessary to have $O(1/G_N)$ mutual information between certain "decision" regions in the boundary theory. While this large mutual information is not generally sufficient to imply scattering, arxiv:2404.15400 showed that for a certain class of geometries, bulk scattering is implied by a certain relation between two (possibly non-minimal) Ryu-Takayanagi surfaces. Here, we show that the 2-to-2 version of the theorem becomes an equivalence in pure AdS$_3$: large mutual information between appropriate boundary subregions is both necessary and sufficient for bulk scattering. This result allows us to extend the findings of arxiv:2404.15400 to a broader class of asymptotically AdS$_3$ spacetimes, which we illustrate with the spinning conical defect geometry. In contrast, we find that matter sources can disrupt this converse relation, and that the $n$-to-$n$ version of the theorem with $n>2$ lacks a converse even in the AdS$_3$ vacuum.
