We find a new exact vacuum solution in the framework of the Poincar\'e Gauge
field theory with massive torsion. In this model, torsion operates as an
independent field and introduces corrections to the vacuum structure present in
General Relativity. The new static and spherically symmetric configuration
shows a Reissner-Nordstr\"om-like geometry characterized by a spin charge. It
extends the known massless torsion solution to the massive case. The
corresponding Reissner-Nordstr\"om-de Sitter solution is also compatible with a
cosmological constant and additional U(1) gauge fields.Comment: 12 pages, 0 figures, minor changes, references adde

Cembranos, Jose A. R.

Valcarcel, Jorge Gigante

Physics Letters B

English

arXiv

© 2018 The Authors. Published by Elsevier B.V. The authors acknowledge F. W. Hehl for useful discussions. This work was partly supported by the projects FIS2014-52837-P (Spanish MINECO) and FIS2016-78859-P (AEI/FEDER, UE), and Consolider-Ingenio MULTIDARK CSD2009-00064.We find a new exact vacuum solution in the framework of the Poincaré Gauge field theory with massive torsion. In this model, torsion operates as an independent field and introduces corrections to the vacuum structure present in General Relativity. The new static and spherically symmetric configuration shows a Reissner–Nordström-like geometry characterized by a spin charge. It extends the known massless torsion solution to the massive case. The corresponding Reissner–Nordström–de Sitter solution is also compatible with a cosmological constant and additional U(1) gauge fields.Ministerio de Economía y Competitividad (MINECO)AEI/FEDER, UEConsolider-Ingenio MULTIDARKDepto. de Física TeóricaFac. de Ciencias FísicasTRUEpu

Ruiz Cembranos, José Alberto

Gigante Valcarcel, Jorge

Docta Complutense

Extended Reissner-Nordstrom solutions sourced by dynamical torsion

We find a new exact vacuum solution in the framework of the Poincaré Gauge field theory with massive torsion. In this model, torsion operates as an independent field and introduces corrections to the vacuum structure present in General Relativity. The new static and spherically symmetric configuration shows a Reissner–Nordström-like geometry characterized by a spin charge. It extends the known massless torsion solution to the massive case. The corresponding Reissner–Nordström–de Sitter solution is also compatible with a cosmological constant and additional U(1) gauge fields. Keywords: Black Holes, Gravity, Torsion, Poincaré Gauge theor

Extended Reissner-Nordstr\"om solutions sourced by dynamical torsion

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