Stochastic collapse
From MaRDI portal
Publication:5067808
DOI10.1088/1475-7516/2020/01/026zbMath1489.83082arXiv1910.10000OpenAlexW2981630370MaRDI QIDQ5067808
David Wands, Tays Miranda, Emmanuel Frion
Publication date: 4 April 2022
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1910.10000
Geometrodynamics and the holographic principle (83E05) Phase-space methods including Wigner distributions, etc. applied to problems in quantum mechanics (81S30) PDEs with randomness, stochastic partial differential equations (35R60) Exponential and trigonometric functions (33B10)
Related Items (2)
Non-standard primordial clocks from induced mass in alternative to inflation scenarios ⋮ Hamiltonian formalism for cosmological perturbations: the separate-universe approach
Cites Work
- Bouncing cosmologies: progress and problems
- A critical review of classical bouncing cosmologies
- A new type of isotropic cosmological models without singularity
- G-bounce inflation: towards nonsingular inflation cosmology with galileon field
- Cosmic no-hair theorem in homogeneous spacetimes. I. Bianchi models
- Cosmology with positive and negative exponential potentials
- Quantum diffusion during inflation and primordial black holes
- Can all the infrared secular growth really be understood as increase of classical statistical variance?
- Stochastic inflation in phase space: is slow roll a stochastic attractor?
- Stochastic inflation beyond slow roll
- Inflationary universe: A possible solution to the horizon and flatness problems
- Renormalisation group improvement in the stochastic formalism
- Coarse-grained field wave function in stochastic inflation
- Coarse-grained effective action and renormalization group theory in semiclassical gravity and cosmology
This page was built for publication: Stochastic collapse
