Computing first-passage times with the functional renormalisation group
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Publication:6103568
DOI10.1088/1475-7516/2023/04/046zbMath1523.83062arXiv2211.09649OpenAlexW4366265071MaRDI QIDQ6103568
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Publication date: 5 June 2023
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2211.09649
Unified quantum theories (81V22) Black holes (83C57) Spectrum, resolvent (47A10) Geometrodynamics and the holographic principle (83E05) Axiomatic quantum field theory; operator algebras (81T05) Renormalization group methods applied to problems in quantum field theory (81T17) Effective quantum field theories (81T12)
Cites Work
- Stochastic quantum gravitational inflation
- Non-perturbative renormalization flow in quantum field theory and statistical physics
- The nonperturbative functional renormalization group and its applications
- THE EXACT RENORMALIZATION GROUP AND APPROXIMATE SOLUTIONS
- An Introduction to the Nonperturbative Renormalization Group
- Introduction to the Functional RG and Applications to Gauge Theories
- Tables for Computing Bivariate Normal Probabilities
- Quantum diffusion during inflation and primordial black holes
- Effective long wavelength scalar dynamics in de Sitter
- Scalar correlation functions in de Sitter space from the stochastic spectral expansion
- A manifestly covariant theory of multifield stochastic inflation in phase space: solving the discretisation ambiguity in stochastic inflation
- Numerical simulations of stochastic inflation using importance sampling
- Primordial black holes from spectator field bubbles
- Inflation is always semi-classical: diffusion domination overproduces Primordial Black Holes
- Scalar correlation functions for a double-well potential in de Sitter space
- Implications of stochastic effects for primordial black hole production in ultra-slow-roll inflation
- Generating the curvature perturbation at the end of inflation
- Ultra-slow-roll inflation with quantum diffusion
- Effects of cosmological moduli fields on cosmic microwave background
- Generating the curvature perturbation without an inflaton
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