Slow Kerr-NUT black hole solution in dynamical Chern-Simons modified gravity
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Publication:6095260
DOI10.1016/J.NUCLPHYSB.2023.116325arXiv2308.06487OpenAlexW4385741755MaRDI QIDQ6095260
Gamal G. L. Nashed, Kazuharu Bamba
Publication date: 7 September 2023
Published in: Nuclear Physics. B (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2308.06487
Black holes (83C57) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05)
Cites Work
- Spinning black holes in shift-symmetric Horndeski theory
- A class of solutions of Einstein-Maxwell equations
- Gödel and Gödel-type universes in Brans-Dicke theory
- Erratum to: Leading higher-derivative corrections to Kerr geometry
- Remarks on the Taub-NUT solution in Chern-Simons modified gravity
- MAXWELL-CHERN-SIMONS ELECTRODYNAMICS ON A DISK
- Energy and momentum of a spherically symmetric dilaton frame as regularized by teleparallel gravity
- Classical monopoles: Newton, NUT space, gravomagnetic lensing, and atomic spectra
- First-order perturbations of Gödel-type metrics in non-dynamical Chern–Simons modified gravity
- MacDowell–Mansouri gravity and Cartan geometry
- Peccei-Quinn Mechanism in Gravity and the Nature of the Barbero-Immirzi Parameter
- Charged spherically symmetric Taub–NUT black hole solutions in $f(R)$ gravity
- Gravitational waves propagation in nondynamical Chern–Simons gravity
- Modern Canonical Quantum General Relativity
- A NEW LOOK AT THE PLEBAŃSKI–DEMIAŃSKI FAMILY OF SOLUTIONS
- Empty-Space Generalization of the Schwarzschild Metric
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