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Monte Carlo studies of quantum cosmology by the generalized Lefschetz thimble method

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arxiv 2407.17724 v3 pith:GM7H5CPD submitted 2024-07-25 gr-qc hep-lathep-thquant-ph

Monte Carlo studies of quantum cosmology by the generalized Lefschetz thimble method

classification gr-qc hep-lathep-thquant-ph
keywords quantumcosmologyboundarycarlogeneralizedgeometryhartle-hawkingissue
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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Quantum cosmology aims at elucidating the beginning of our Universe. Back in early 80's, Vilenkin and Hartle-Hawking put forward the "tunneling from nothing" and "no boundary" proposals. Recently there has been renewed interest in this subject from the viewpoint of defining the oscillating path integral for Lorentzian quantum gravity using the Picard-Lefschetz theory. Aiming at going beyond the mini-superspace and saddle-point approximations, we perform Monte Carlo calculations using the generalized Lefschetz thimble method to overcome the sign problem. In particular, we confirm that either Vilenkin or Hartle-Hawking saddle point becomes relevant if one uses the Robin boundary condition depending on its parameter. We also clarify some fundamental issues in quantum cosmology, such as an issue related to the integration domain of the lapse function and an issue related to reading off the real geometry from the complex geometry obtained at the saddle point.

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Cited by 4 Pith papers

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    gr-qc 2026-07 conditional novelty 6.0

    Tunneling wave function of a closed universe is recovered as the ε o0 limit of a Neumann-plus-small-domain path integral with radiation-induced throat, excluding the unsuppressed outer saddle.

  3. The yes boundaries wavefunctions of the universe

    hep-th 2026-04 unverdicted novelty 6.0

    Using two timelike boundaries and a nearly maximally entangled thermofield double state from dressed de Sitter Hamiltonian theories, the authors construct wavefunctions for extended cosmological spacetimes that includ...

  4. IR behaviour of one-loop complex $\mathbb{R}\times S^3$ saddles

    hep-th 2026-04 unverdicted novelty 5.0

    One-loop metric fluctuations produce secularly growing IR divergences in the Hartle-Hawking wavefunction for complex saddles on R x S3, identical in leading order to the Lorentzian de Sitter case after UV renormalization.