Brownian Motion in the Hilbert Space of Quantum States along with the Ricci Flow and Stochastically Emergent Einstein-Hilbert Action: Formulating a Well-Defined Feynman Path-Integral Measure for Quantum Fields in the Presence of Gravity
A. A. Varshovi

TL;DR
This paper links quantum field theory in curved spacetime with Ricci flow and Brownian motion, deriving a well-defined path-integral measure that incorporates gravity and suggests gravity's thermodynamic origin.
Contribution
It introduces a novel approach connecting Ricci flow and stochastic processes to formulate a consistent quantum gravity path integral measure.
Findings
Wiener measure contains Einstein-Hilbert action at first order
Emergence of Einstein-Hilbert action is geometric, not matter-dependent
Derived explicit formula for the cosmological constant
Abstract
In this paper, we aim to interpret the background gravitational effects appearing in quantum field theory on curved space-time by studying the Brownian motion of quantum states along with the Hamilton-Perelman Ricci flow. It has been shown that the Wiener measure automatically contains the Einstein-Hilbert action and the path-integral formulation of the scalar quantum field theory on curved space-time at the first order of local approximations. This provides a well-defined formulation of the path-integral measure for quantum field theory in the presence of gravity. However, we establish that the emergence of Einstein-Hilbert action is independent of the matter field interactions and is a merely entropic/geometric effect stemming from the nature of the Ricci flow of the universe geometry. We also extract an explicit formula for the cosmological constant in terms of the Ricci flow and the…
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Taxonomy
TopicsCosmology and Gravitation Theories · Quantum Mechanics and Applications · Advanced Thermodynamics and Statistical Mechanics
