Exact Solutions in Poincaré Gauge Gravity Theory

In the framework of the gauge theory based on the Poincaré symmetry group, the gravitational field is described in terms of the coframe and the local Lorentz connection. Considered as gauge field potentials, they give rise to the corresponding field strength which are naturally identified w...

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Main Author: Yuri N. Obukhov
Format: Article
Language:English
Published: MDPI AG 2019-05-01
Series:Universe
Subjects:
Online Access:https://www.mdpi.com/2218-1997/5/5/127
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author Yuri N. Obukhov
author_facet Yuri N. Obukhov
author_sort Yuri N. Obukhov
collection DOAJ
description In the framework of the gauge theory based on the Poincaré symmetry group, the gravitational field is described in terms of the coframe and the local Lorentz connection. Considered as gauge field potentials, they give rise to the corresponding field strength which are naturally identified with the torsion and the curvature on the Riemann−Cartan spacetime. We study the class of quadratic Poincaré gauge gravity models with the most general Yang−Mills type Lagrangian which contains all possible parity-even and parity-odd invariants built from the torsion and the curvature. Exact vacuum solutions of the gravitational field equations are constructed as a certain deformation of de Sitter geometry. They are black holes with nontrivial torsion.
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spelling doaj.art-d1a0abae59a943959ad505d13ee2a4862022-12-22T02:21:48ZengMDPI AGUniverse2218-19972019-05-015512710.3390/universe5050127universe5050127Exact Solutions in Poincaré Gauge Gravity TheoryYuri N. Obukhov0Russian Academy of Sciences, Nuclear Safety Institute (IBRAE), B. Tulskaya 52, 115191 Moscow, RussiaIn the framework of the gauge theory based on the Poincaré symmetry group, the gravitational field is described in terms of the coframe and the local Lorentz connection. Considered as gauge field potentials, they give rise to the corresponding field strength which are naturally identified with the torsion and the curvature on the Riemann−Cartan spacetime. We study the class of quadratic Poincaré gauge gravity models with the most general Yang−Mills type Lagrangian which contains all possible parity-even and parity-odd invariants built from the torsion and the curvature. Exact vacuum solutions of the gravitational field equations are constructed as a certain deformation of de Sitter geometry. They are black holes with nontrivial torsion.https://www.mdpi.com/2218-1997/5/5/127gauge gravity theoryPoincaré groupcoframeLorentz connectionodd parity
spellingShingle Yuri N. Obukhov
Exact Solutions in Poincaré Gauge Gravity Theory
Universe
gauge gravity theory
Poincaré group
coframe
Lorentz connection
odd parity
title Exact Solutions in Poincaré Gauge Gravity Theory
title_full Exact Solutions in Poincaré Gauge Gravity Theory
title_fullStr Exact Solutions in Poincaré Gauge Gravity Theory
title_full_unstemmed Exact Solutions in Poincaré Gauge Gravity Theory
title_short Exact Solutions in Poincaré Gauge Gravity Theory
title_sort exact solutions in poincare gauge gravity theory
topic gauge gravity theory
Poincaré group
coframe
Lorentz connection
odd parity
url https://www.mdpi.com/2218-1997/5/5/127
work_keys_str_mv AT yurinobukhov exactsolutionsinpoincaregaugegravitytheory