2020
			
	    
	
	
    Quantum-Gravity Screening Effect of the Cosmological Constant in the DeSitter Space-Time
CREMASCHINI, Claudio and Massimo TESSAROTTOBasic information
Original name
Quantum-Gravity Screening Effect of the Cosmological Constant in the DeSitter Space-Time
	Authors
CREMASCHINI, Claudio (380 Italy, belonging to the institution) and Massimo TESSAROTTO (380 Italy, belonging to the institution)
			Edition
 Symmetry, 2020, 2073-8994
			Other information
Language
English
		Type of outcome
Article in a journal
		Field of Study
10300 1.3 Physical sciences
		Country of publisher
Switzerland
		Confidentiality degree
is not subject to a state or trade secret
		References:
Impact factor
Impact factor: 2.713
			RIV identification code
RIV/47813059:19630/20:A0000079
		Organization unit
Institute of physics in Opava
			UT WoS
000540222200042
		EID Scopus
2-s2.0-85084614976
		Keywords in English
covariant quantum gravity; cosmological constant; DeSitter space-time; massive gravitons
		Tags
International impact, Reviewed
		
				
				Changed: 23/3/2021 21:59, Mgr. Pavlína Jalůvková
				
		Abstract
In the original language
Small-amplitude quantum-gravity periodic perturbations of the metric tensor, occurring in sequences of phase-shifted oscillations, are investigated for vacuum conditions and in the context of the manifestly-covariant theory of quantum gravity. The theoretical background is provided by the Hamiltonian representation of the quantum hydrodynamic equations yielding, in turn, quantum modifications of the Einstein field equations. It is shown that in the case of the DeSitter space-time sequences of small-size periodic perturbations with prescribed frequency are actually permitted, each one with its characteristic initial phase. The same perturbations give rise to non-linear modifications of the Einstein field equations in terms of a suitable stochastic-averaged and divergence-free quantum stress-energy tensor. As a result, a quantum-driven screening effect arises which is shown to affect the magnitude of the cosmological constant. Observable features on the DeSitter space-time solution and on the graviton mass estimate are pointed out.