Space-time second-quantization effects and the quantum origin of cosmological constant in covariant quantum gravity
Claudio Cremaschini, Massimo Tessarotto

TL;DR
This paper derives quantum corrections to Einstein's equations within a covariant quantum gravity framework, revealing that the cosmological constant originates from quantum gravitational fluctuations and may be non-stationary.
Contribution
It introduces a non-perturbative, covariant quantum gravity approach with a generalized Lagrangian path formalism to derive quantum-modified Einstein equations and explore the quantum origin of the cosmological constant.
Findings
Quantum gravitational effects modify Einstein's equations.
The cosmological constant arises from quantum vacuum fluctuations.
The quantum cosmological constant may be non-stationary.
Abstract
Space-time quantum contributions to the classical Einstein equations of General Relativity are determined. The theoretical background is provided by the non-perturbative theory of manifestly-covariant quantum gravity and the trajectory-based representation of the related quantum wave equation in terms of the Generalized Lagrangian path formalism. To reach the target an extended functional setting is introduced, permitting the treatment of a non-stationary background metric tensor allowed to depend on both space-time coordinates and a suitably-defined invariant proper-time parameter. Based on the Hamiltonian representation of the corresponding quantum hydrodynamic equations occurring in such a context, the quantum-modified Einstein field equations are obtained. As an application, the quantum origin of the cosmological constant is investigated. This is shown to be ascribed to the…
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