A Fluctuation-Dissipation Relation for Semiclassical Cosmology
B. L. Hu, Sukanya Sinha

TL;DR
This paper derives a fluctuation-dissipation relation in semiclassical cosmology, linking quantum matter fluctuations to spacetime dynamics, and demonstrates its implications for particle creation and anisotropy dissipation in the universe.
Contribution
It establishes a general fluctuation-dissipation theorem for semiclassical gravity, connecting dissipation and noise kernels via the influence functional, and applies it to cosmological models.
Findings
Derivation of an Einstein-Langevin equation for semiclassical gravity.
Illustration of fluctuation-dissipation relation in a Bianchi Type-I universe.
Explanation of particle creation and anisotropy dissipation as fluctuation-dissipation phenomena.
Abstract
Using the concept of open systems where the classical geometry is treated as the system and the quantum matter field as the environment, we derive a fluctuation-dissipation theorem for semiclassical cosmology. This theorem which exists under very general conditions for dissipations in the dynamics of the system, and the noise and fluctuations in the environment, can be traced to the formal mathematical relation between the dissipation and noise kernels of the influence functional depicting the open system, and is ultimately a consequence of the unitarity of the closed system. In particular, for semiclassical gravity, it embodies the backreaction effect of matter fields on the dynamics of spacetime. The backreaction equation derivable from the influence action is in the form of a Einstein-Langevin equation. It contains a dissipative term in the equation of motion for the dynamics of…
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