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2024 1

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Prepare inflationary universe via the Euclidean charged wormhole

gr-qc · 2024-11-21 · conditional · novelty 5.0

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.

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  • Prepare inflationary universe via the Euclidean charged wormhole gr-qc · 2024-11-21 · conditional · none · ref 7

    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.