Rotating Kerr-Newman space-times in Metric-Affine Gravity
arXiv:2108.12414 · doi:10.1088/1475-7516/2022/01/011
Abstract
We present new rotating vacuum configurations endowed with both dynamical torsion and nonmetricity fields in the framework of Metric-Affine gauge theory of gravity. For this task, we consider scalar-flat Weyl-Cartan geometries and obtain an axisymmetric Kerr-Newman solution in the decoupling limit between the orbital and the spin angular momentum. The corresponding Kerr-Newman-de Sitter solution is also compatible with a cosmological constant and additional electromagnetic fields.
13 pages, 0 figures, minor changes, references added. It matches the version published in JCAP
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Cited by in corpus (5)
- Black Holes in Gravity: Exact and Perturbed Solutions
- Black hole solutions in scalar-tensor symmetric teleparallel gravity
- New black hole solutions with a dynamical traceless nonmetricity tensor in Metric-Affine Gravity
- Spontaneous Scalarization of Black Holes in Gauss-Bonnet Teleparallel Gravity
- Vector stability in quadratic metric-affine theories