Nonequilibrium Schwinger-Keldysh formalism for density matrix states: analytic properties and implications in cosmology
Andrei O. Barvinsky, Nikita Kolganov

TL;DR
This paper develops a nonequilibrium Schwinger-Keldysh formalism for density matrix states, revealing analytic properties and implications for cosmology, especially in the context of the universe's quantum state and its evolution.
Contribution
It introduces a generalized in-in formalism for Gaussian density matrices and explores their analytic and symmetry properties in cosmological settings.
Findings
Positive/negative frequency basis functions are selected by particle interpretation.
Wightman functions satisfy KMS conditions despite nonequilibrium.
Analytic structure shows Euclidean-Lorentzian evolution and quantum state decay.
Abstract
Motivated by cosmological Hartle-Hawking and microcanonical density matrix prescriptions for the quantum state of the Universe we develop Schwinger-Keldysh in-in formalism for generic nonequilibrium dynamical systems with the initial density matrix. We build the generating functional of in-in Green's functions and expectation values for a generic density matrix of the Gaussian type and show that the requirement of particle interpretation selects a distinguished set of positive/negative frequency basis functions of the wave operator of the theory, which is determined by the density matrix parameters. Then we consider a special case of the density matrix determined by the Euclidean path integral of the theory, which in the cosmological context can be considered as a generalization of the no-boundary pure state to the case of the microcanonical ensemble, and show that in view of a special…
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Taxonomy
TopicsCosmology and Gravitation Theories · Black Holes and Theoretical Physics · Noncommutative and Quantum Gravity Theories
