New Concepts for Old Black Holes
Leonard Susskind
TL;DR
The paper confronts the AMPS firewall paradox by proposing a framework in which the black hole interior is encoded as a fault-tolerant quantum message within the Hawking radiation, rather than requiring a firewall. Central to this approach are the ER=EPR connection, precursors, and timefolds, which together enable nonlocal encoding and boundary–bulk mappings that preserve complementarity while maintaining unitarity. A key contribution is the construction of a concrete coding picture, including reference systems and negative-information qubits, that explains how interior information can remain accessible to infalling observers without violating causality or leading to firewalls. The work also analyzes gauge invariance behind horizons, the role of scrambling, and a laboratory string-qubit model to illustrate easy versus hard operators, proposing that horizon dynamics can self-heal on scrambling times. Overall, the paper offers a cohesive, if speculative, route to reconciling information preservation with smooth horizons, with implications for holography, quantum error correction, and the nonlocal structure of spacetime behind black hole horizons.
Abstract
It has been argued that the AMPS paradox implies catastrophic breakdown of the equivalence principle in the neighborhood of a black hole horizon, or even the non-existence of any spacetime at all behind the horizon. Maldacena and the author suggested a different resolution of the paradox based on the close relationship between Einstein-Rosen bridges and Einstein-Podolsky-Rosen entanglement. In this paper the new mechanisms required by the proposal are reviewed: the ER=EPR connection: precursors: timefolds: and the black hole interior as a fault-tolerant, negative information message. Along the way a model of an ADS black hole as a single long-string is explained, and used to clarify the relation between Wilson loops and precursors.
