Role of Quantum Entropy and Establishment of H-Theorems in the Presence of Graviton Sinks for Manifestly-Covariant Quantum Gravity
Based on the introduction of a suitable quantum functional, identified here with the Boltzmann–Shannon entropy, entropic properties of the quantum gravitational field are investigated in the framework of manifestly-covariant quantum gravity theory. In particular, focus is given to gravitat...
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doaj-311a1b1831684109975265a873fbfe042020-11-24T21:46:51ZengMDPI AGEntropy1099-43002019-04-0121441810.3390/e21040418e21040418Role of Quantum Entropy and Establishment of H-Theorems in the Presence of Graviton Sinks for Manifestly-Covariant Quantum GravityMassimo Tessarotto0Claudio Cremaschini1Department of Mathematics and Geosciences, University of Trieste, Via Valerio 12, 34127 Trieste, ItalyInstitute of Physics and Research Center for Theoretical Physics and Astrophysics, Faculty of Philosophy and Science, Silesian University in Opava, Bezručovo nám.13, CZ-74601 Opava, Czech RepublicBased on the introduction of a suitable quantum functional, identified here with the Boltzmann–Shannon entropy, entropic properties of the quantum gravitational field are investigated in the framework of manifestly-covariant quantum gravity theory. In particular, focus is given to gravitational quantum states in a background de Sitter space-time, with the addition of possible quantum non-unitarity effects modeled in terms of an effective quantum graviton sink localized near the de Sitter event horizon. The theory of manifestly-covariant quantum gravity developed accordingly is shown to retain its emergent-gravity features, which are recovered when the generalized-Lagrangian-path formalism is adopted, yielding a stochastic trajectory-based representation of the quantum wave equation. This permits the analytic determination of the quantum probability density function associated with the quantum gravity state, represented in terms of a generally dynamically-evolving shifted Gaussian function. As an application, the study of the entropic properties of quantum gravity is developed and the conditions for the existence of a local H-theorem or, alternatively, of a constant H-theorem are established.https://www.mdpi.com/1099-4300/21/4/418covariant quantum gravityGaussian solutionsBoltzmann–Shannon entropyH-theorem |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
Massimo Tessarotto Claudio Cremaschini |
spellingShingle |
Massimo Tessarotto Claudio Cremaschini Role of Quantum Entropy and Establishment of H-Theorems in the Presence of Graviton Sinks for Manifestly-Covariant Quantum Gravity Entropy covariant quantum gravity Gaussian solutions Boltzmann–Shannon entropy H-theorem |
author_facet |
Massimo Tessarotto Claudio Cremaschini |
author_sort |
Massimo Tessarotto |
title |
Role of Quantum Entropy and Establishment of H-Theorems in the Presence of Graviton Sinks for Manifestly-Covariant Quantum Gravity |
title_short |
Role of Quantum Entropy and Establishment of H-Theorems in the Presence of Graviton Sinks for Manifestly-Covariant Quantum Gravity |
title_full |
Role of Quantum Entropy and Establishment of H-Theorems in the Presence of Graviton Sinks for Manifestly-Covariant Quantum Gravity |
title_fullStr |
Role of Quantum Entropy and Establishment of H-Theorems in the Presence of Graviton Sinks for Manifestly-Covariant Quantum Gravity |
title_full_unstemmed |
Role of Quantum Entropy and Establishment of H-Theorems in the Presence of Graviton Sinks for Manifestly-Covariant Quantum Gravity |
title_sort |
role of quantum entropy and establishment of h-theorems in the presence of graviton sinks for manifestly-covariant quantum gravity |
publisher |
MDPI AG |
series |
Entropy |
issn |
1099-4300 |
publishDate |
2019-04-01 |
description |
Based on the introduction of a suitable quantum functional, identified here with the Boltzmann–Shannon entropy, entropic properties of the quantum gravitational field are investigated in the framework of manifestly-covariant quantum gravity theory. In particular, focus is given to gravitational quantum states in a background de Sitter space-time, with the addition of possible quantum non-unitarity effects modeled in terms of an effective quantum graviton sink localized near the de Sitter event horizon. The theory of manifestly-covariant quantum gravity developed accordingly is shown to retain its emergent-gravity features, which are recovered when the generalized-Lagrangian-path formalism is adopted, yielding a stochastic trajectory-based representation of the quantum wave equation. This permits the analytic determination of the quantum probability density function associated with the quantum gravity state, represented in terms of a generally dynamically-evolving shifted Gaussian function. As an application, the study of the entropic properties of quantum gravity is developed and the conditions for the existence of a local H-theorem or, alternatively, of a constant H-theorem are established. |
topic |
covariant quantum gravity Gaussian solutions Boltzmann–Shannon entropy H-theorem |
url |
https://www.mdpi.com/1099-4300/21/4/418 |
work_keys_str_mv |
AT massimotessarotto roleofquantumentropyandestablishmentofhtheoremsinthepresenceofgravitonsinksformanifestlycovariantquantumgravity AT claudiocremaschini roleofquantumentropyandestablishmentofhtheoremsinthepresenceofgravitonsinksformanifestlycovariantquantumgravity |
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1725899581371187200 |