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De Sitter Holography and the Cosmic Microwave Background

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arxiv hep-th/0202127 v2 pith:3LUO734P submitted 2002-02-20 hep-th astro-ph

classification hep-thastro-ph
keywords fieldtheorybackgroundcosmiccosmologicaldualmicrowavealbeit
verification ladder T0 review T1 audit T2 compute T3 formal
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We interpret cosmological evolution holographically as a renormalisation group flow in a dual Euclidean field theory, as suggested by the conjectured dS/CFT correspondence. Inflation is described by perturbing around the infra-red fixed point of the dual field theory. The spectrum of the cosmic microwave background radiation is determined in terms of scaling violations in the field theory. The dark energy allows similar, albeit less predictive, considerations. We discuss the cosmological fine-tuning problems from the holographic perspective.

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Cited by 1 Pith paper

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

  1. Energy momentum tensor correlators in $\phi^4$ theory II: The spin-two sector

    hep-th 2025-07 conditional novelty 7.0 of 10

    A four-loop calculation shows the energy-momentum tensor charge C_T separates into a fixed-point value plus corrections proportional to the beta function.

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