Abstract

We study the dual 3d Euclidean RG flow of single-field slow-roll Inflation using the postulates of the dS/CFT correspondence. For that purpose we solve for the inflationary fluctuation at all times using a matching procedure between two approximate solutions which are separately valid at different regions of the space of parameters but together cover all of it. The two modes of the full solution mix such that each of the modes at late times is a superposition of the modes in the quasi-de Sitter region. We find that the dual theory admits two phases of explicit and spontaneous breaking of conformal symmetry. We also find that the mixing effect between the two modes in the bulk implies that slow-roll inflation does not guarantee, but rather generically generates, a nearly scale invariant power spectrum, except in fine-tuned situations. We suggest that the mixing effect can have a unique signature on other cosmological observables such as the bispectrum.

Highlights

  • We find that the mixing effect between the two modes in the bulk implies that slowroll inflation does not guarantee, but rather generically generates, a nearly scale invariant power spectrum, except in fine-tuned situations

  • We study the dual 3d Euclidean renormalization group (RG) flow of single-field slow-roll Inflation using the postulates of the dS/CFT correspondence

  • We find that the dual theory admits two phases of explicit and spontaneous breaking of conformal symmetry

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Summary

Single field inflation

It is possible to study the asymptotic forms of the solution near the fixed points. Let us start by looking exactly at a fixed point of the potential, where its derivative is zero. At this point the potential takes a constant value. The value of the potential at each of the fixed points is different and the potential interpolates between two de Sitter spaces with different Hubble constants. Near a fixed point the potential can be expanded as follows d(d − 1) H2 + 2 Plugging this into (2.4), and defining δφ ≡ φ − φ0, we find the following equation for the scalar δφ + dHδφ + m2δφ = 0. Note that the value of m2 is different in each fixed point (and, in particular, is negative for a maximum of the potential)

Fluctuations
Low momentum solution
Quasi-de Sitter region
The matching
The dual flow
Asymptotically late times
The two-point function
Explicit breaking
Spontaneous breaking
Gravitational waves
Concluding remarks and future directions
A The Hankel function
Full Text
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