Second Order Langevin Equation and Definition of Quantum Gravity By Stochastic Quantisation
Laurent Baulieu, Siye Wu

TL;DR
This paper explores a novel approach to quantum gravity using second order Langevin equations in stochastic quantisation, proposing a transition from quantum to classical cosmology and implications for black hole formation and dark matter.
Contribution
It introduces a second order Langevin equation framework for stochastic quantisation of quantum gravity and explicitly defines second order stochastic quantisation in a solvable model.
Findings
Transition from oscillating quantum phase to semi-classical phase with Lorentz time emergence
Black hole formation and decay consistent with inflation and dark matter observations
Explicit calculation of second order Langevin equation in a zero-dimensional model
Abstract
Euclidean quantum gravity might be defined by stochastic quantisation that is governed by a higher order Langevin equation rather than a first order stochastic equation. In a transitory phase where the Lorentz time cannot be defined, the parameter that orders the evolution of quantum gravity phenomena is the stochastic time. This changes the definition of causality in the period of primordial cosmology. The prediction of stochastically quantised gravity is that there will a transition from an oscillating quantum phase to a semi-classical one, when the Lorentz time emerges. The end of the transition, as it can be observed from now and described by inflation models, is a diluted Universe, following the inflation phenomenological evolution. It is filled at the beginning with scattered classical primordial black holes. The smallest ones will quickly decay in matter, with a standard quantum…
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Taxonomy
TopicsNoncommutative and Quantum Gravity Theories · Cosmology and Gravitation Theories · Particle physics theoretical and experimental studies
