pith. sign in

arxiv: hep-th/0510046 · v4 · submitted 2005-10-05 · ✦ hep-th · gr-qc

Inflation in AdS/CFT

classification ✦ hep-th gr-qc
keywords statemixedboundarycorrelatorsdescribedinflatinginflationable
0
0 comments X
read the original abstract

We study the AdS/CFT correspondence as a probe of inflation. We assume the existence of a string landscape containing at least one stable AdS vacuum and a (nearby) metastable de Sitter state. Standard arguments imply that the bulk physics in the vicinity of the AdS minimum is described by a boundary CFT. We argue that large enough bubbles of the dS phase, including those able to inflate, are described by mixed states in the CFT. Inflating degrees of freedom are traced over and do not appear explicitly in the boundary description. They nevertheless leave a distinct imprint on the mixed state. In the supergravity approximation, analytic continuation connects AdS/CFT correlators to dS/CFT correlators. This provides a framework for extracting further information as well. Our work also shows that no scattering process can create an inflating region, even by quantum tunneling, since a pure state can never evolve into a mixed state under unitary evolution.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.

Forward citations

Cited by 3 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Monitoring a de Sitter universe through an anti-de Sitter window

    hep-th 2026-06 unverdicted novelty 7.0

    Proposes a duality between AdS3 gravity with dS2 branes and CFT2 with non-unitary boundary conditions to realize dS holography via complex saddles and state preparation in unitary AdS/CFT.

  2. Emergent Closed Universes in Symmetric Orbifold CFTs

    hep-th 2026-06 unverdicted novelty 6.0

    Large N symmetric orbifold CFTs decompose into superselection sectors that behave as closed universes, with each physical sector becoming one-dimensional after gauging, matching gravitational expectations.

  3. A Menagerie of Wormholes and Cosmologies in the Gravitational Path Integral

    hep-th 2026-02 unverdicted novelty 6.0

    The paper identifies a variety of Euclidean saddle solutions including wormholes and oscillatory configurations in Einstein-Scalar-Maxwell models, demonstrates how oscillations are controlled by lifting flat potential...