pith. sign in

arxiv: 1106.3556 · v1 · pith:J3CN5FDWnew · submitted 2011-06-17 · ✦ hep-th · hep-ph

AdS/CFT and the cosmological constant problem

classification ✦ hep-th hep-ph
keywords constantcorrelatorscosmologicaltermsbulkexpansionfine-tuninglarge
0
0 comments X
read the original abstract

Within the context of the AdS/CFT correspondence we attempt to formulate the cosmological constant problem in the dual conformal field theory. The fine-tuning of the bulk cosmological constant is related to an apparent fine-tuning in the effective description of the CFT in terms of its light operators: while the correlators of single particle operators satisfy a large N expansion, the expansion does not appear to be natural. Individual terms contributing to correlators have parametrically larger value than the one dictated by large N counting. The final 1/N suppression of correlators is achieved via delicate cancellations between such terms. We speculate on the existence of underlying principles which might make the bulk theory (secretly) natural.

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 1 Pith paper

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

  1. A Holographic Constraint on Scale Separation

    hep-th 2025-12 conditional novelty 7.0

    A holographic consistency condition derived from large-N factorization requires vanishing cubic couplings for extremal-dimension operators and is non-trivially satisfied in DGKT AdS4 string vacua.