Holography in a quantum spacetime

dc.creatorMarkopoulou, Fotini
dc.creatorSmolin, Lee
dc.date1999-10-18
dc.date.accessioned2026-07-07T04:27:12Z
dc.date.available2026-07-07T04:27:12Z
dc.descriptionWe propose a formulation of the holographic principle, suitable for a background independent quantum theory of cosmology. It is stated as a relationship between the flow of quantum information and the causal structure of a quantum spacetime. Screens are defined as sets of events at which the observables of a holographic cosmological theory may be measured, and such that information may flow across them in two directions. A discrete background independent holographic theory may be formulated in terms of information flowing in a causal network of such screens. Geometry is introduced by defining the area of a screen to be a measure of its capacity as a channel of quantum information from its null past to its null future. We call this a ``weak'' form of the holographic principle, as no use is made of a bulk theory.
dc.description16 pages, LaTeX
dc.identifierhttps://arxiv.org/abs/hep-th/9910146
dc.identifierhttp://arxiv.org/abs/hep-th/9910146
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/56329
dc.subjectHigh Energy Physics - Theory
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleHolography in a quantum spacetime
dc.typetext

Files

Collections