Can Stochastic Clocks in FLRW Minisuperspace Prevent Dynamical Singularities?
arXiv:2608.19695 · doi:10.1088/1361-6382/ae3424
Abstract
We develop a stochastic extension of the Wheeler--DeWitt equation in FLRW minisuperspace and show that quantum backreaction can dynamically regulate the big bang singularity without imposing external boundary conditions. Using Laplace--Beltrami quantisation and an open-system treatment of coarse-grained graviton modes, we obtain a stochastic Hamiltonian evolution equation in which the diffusion coefficient takes the form . This multiplicative noise vanishes at the origin and renders an entrance boundary in Feller's classification, leading to super-exponential suppression of the Laplace--Beltrami weighted stationary density and zero probability flux into the singular point. At large scale factor, the global behaviour depends on the cosmological sector: de Sitter and positive potential-dominated regimes exhibit power-law stationary tails, whereas confining potentials or negative effective cosmological constant lead to an entrance boundary at infinity and a globally normalizable steady state. Taken together, these results indicate that stochastic backreaction arising from semiclassical coarse-graining provides a consistent and dynamical mechanism for singularity avoidance in minisuperspace quantum cosmology.
19 pages, 2 figures
References in corpus (15)
- Quantum Nature of the Big Bang
- Equilibrium State of a Massless Self-Interacting Scalar Field in the De Sitter Background
- Correlation Functions in Stochastic Inflation
- Noise and Fluctuations in Semiclassical Gravity
- Environment--Induced Decoherence, Classicality and Consistency of Quantum Histories
- Stochastic Gravity: Theory and Applications
- The one-loop effective action and trace anomaly in four dimensions
- Backreaction in Semiclassical Cosmolgy: The Einstein Langevin Equation
- Stochastic dynamics of correlations in quantum field theory: From Schwinger-Dyson to Boltzmann-Langevin equation
- Coarse-Grained Effective Action and Renormalization Group Theory in Semiclassical Gravity and Cosmology
- Symmetric path integrals for stochastic equations with multiplicative noise
- Consistent Probabilities in Wheeler-DeWitt Quantum Cosmology
- Effective Hamiltonian for Isotropic Loop Quantum Cosmology
- Stochastic Emergent Quantum Gravity
- Clock Time in Quantum Cosmology