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arXiv · 0907.5542

Holography for Cosmology

Paul McFadden·Kostas Skenderis
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Abstract

We propose a holographic description of four-dimensional single-scalar inflationary universes, and show how cosmological observables, such as the primordial power spectrum, are encoded in the correlation functions of a three-dimensional QFT. The holographic description correctly reproduces standard inflationary predictions in the limit where a perturbative quantization of fluctuations is justified. In the opposite limit, wherein gravity is strongly coupled at early times, we propose a holographic description in terms of perturbative large N QFT. Initiating a holographic phenomenological approach, we show that models containing only two parameters, N and a dimensionful coupling constant, are capable of satisfying the current observational constraints.

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Paul McFadden, Kostas Skenderis. 2009-07-31. Holography for Cosmology. https://doi.org/10.1103/physrevd.81.021301

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