J 2018

Generalized Lagrangian Path Approach to Manifestly-Covariant Quantum Gravity Theory

TESSAROTTO, Massimo a Claudio CREMASCHINI

Základní údaje

Originální název

Generalized Lagrangian Path Approach to Manifestly-Covariant Quantum Gravity Theory

Autoři

TESSAROTTO, Massimo (380 Itálie, garant, domácí) a Claudio CREMASCHINI (380 Itálie, domácí)

Vydání

Entropy, 2018, 1099-4300

Další údaje

Jazyk

angličtina

Typ výsledku

Článek v odborném periodiku

Obor

10308 Astronomy

Stát vydavatele

Švýcarsko

Utajení

není předmětem státního či obchodního tajemství

Odkazy

Kód RIV

RIV/47813059:19240/18:A0000271

Organizační jednotka

Filozoficko-přírodovědecká fakulta v Opavě

UT WoS

000428507100059

Klíčová slova anglicky

quantum mechanics; generalized Lagrangian paths; covariant quantum gravity; emergent space-time; Gaussian-like solutions

Příznaky

Mezinárodní význam, Recenzováno

Návaznosti

GB14-37086G, projekt VaV.
Změněno: 4. 4. 2019 12:44, RNDr. Jan Hladík, Ph.D.

Anotace

V originále

A trajectory-based representation for the quantum theory of the gravitational field is formulated. This is achieved in terms of a covariant Generalized Lagrangian-Path (GLP) approach which relies on a suitable statistical representation of Bohmian Lagrangian trajectories, referred to here as GLP-representation. The result is established in the framework of the manifestly-covariant quantum gravity theory (CQG-theory) proposed recently and the related CQG-wave equation advancing in proper-time the quantum state associated with massive gravitons. Generally non-stationary analytical solutions for the CQG-wave equation with non-vanishing cosmological constant are determined in such a framework, which exhibit Gaussian-like probability densities that are non-dispersive in proper-time. As a remarkable outcome of the theory achieved by implementing these analytical solutions, the existence of an emergent gravity phenomenon is proven to hold. Accordingly, it is shown that a mean-field background space-time metric tensor can be expressed in terms of a suitable statistical average of stochastic fluctuations of the quantum gravitational field whose quantum-wave dynamics is described by GLP trajectories.