A semiclassical Euclidean charged wormhole with an anti-de Sitter boundary can, in a fine-tuned potential, assign higher probability to a longer inflationary period, but it does not beat the Hartle-Hawking no-boundary state.
The holographic F theorem
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abstract
The F theorem states that, for a unitary three dimensional quantum field theory, the F quantity defined in terms of the partition function on a three sphere is positive, stationary at fixed point and decreases monotonically along a renormalization group flow. We construct holographic renormalization group flows corresponding to relevant deformations of three-dimensional conformal field theories on spheres, working to quadratic order in the source. For these renormalization group flows, the F quantity at the IR fixed point is always less than F at the UV fixed point, but F increases along the RG flow for deformations by operators of dimension $3/2 < \Delta < 5/2$. Therefore the strongest version of the F theorem is in general violated.
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gr-qc 1years
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Prepare inflationary universe via the Euclidean charged wormhole
A semiclassical Euclidean charged wormhole with an anti-de Sitter boundary can, in a fine-tuned potential, assign higher probability to a longer inflationary period, but it does not beat the Hartle-Hawking no-boundary state.