TESSAROTTO, Massimo and Claudio CREMASCHINI. On the Quantum Regularization of Singular Black-Hole Solutions in Covariant Quantum Gravity. SYMMETRY-BASEL. Švýcarsko, 2023, vol. 15, No 6, p. "1218-1"-"1218-18", 18 pp. ISSN 2073-8994. Available from: https://dx.doi.org/10.3390/sym15061218.
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Basic information
Original name On the Quantum Regularization of Singular Black-Hole Solutions in Covariant Quantum Gravity
Authors TESSAROTTO, Massimo (380 Italy, belonging to the institution) and Claudio CREMASCHINI (380 Italy, belonging to the institution).
Edition SYMMETRY-BASEL, Švýcarsko, 2023, 2073-8994.
Other information
Original language English
Type of outcome Article in a journal
Field of Study 10308 Astronomy
Country of publisher Switzerland
Confidentiality degree is not subject to a state or trade secret
WWW URL
RIV identification code RIV/47813059:19630/23:A0000299
Organization unit Institute of physics in Opava
Doi http://dx.doi.org/10.3390/sym15061218
UT WoS 001015754900001
Keywords in English quantum gravity;space-time singular solutions;quantum regularization
Tags RIV24, UF
Tags International impact, Reviewed
Changed by Changed by: Mgr. Pavlína Jalůvková, učo 25213. Changed: 22/1/2024 14:20.
Abstract
The theoretical prediction of the stochastic property of the quantum cosmological constant and the quantum stochastic nature of event horizons has crucial implications on the physics of space-time and black holes in particular. One of these consequences concerns a new mechanism, which is investigated here, for the stochastic regularization of singular black-hole solutions of classical general relativity. The problem is posed in the context of the theory of covariant quantum gravity (CQG-theory), namely the manifestly covariant, constraint-free and finite graviton-mass quantum Hamiltonian approach developed by Cremaschini and Tessarotto (2015-2022), which permits to cast the theory in a frame-independent setting. It is precisely the trajectory-dependence feature of the theory and the intrinsic stochastic property of quantum gravity which turn out to be crucial properties for reaching quantum regularization of classical singular solutions.
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