Remarks on the Taub-NUT solution in Chern-Simons modified gravity
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Publication:2399116
DOI10.1016/j.physletb.2016.11.055zbMath1369.83071arXiv1610.09952OpenAlexW2544698852MaRDI QIDQ2399116
Publication date: 21 August 2017
Published in: Physics Letters. B (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1610.09952
Classes of solutions; algebraically special solutions, metrics with symmetries for problems in general relativity and gravitational theory (83C20) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05)
Related Items (5)
Non-perturbative spinning black holes in dynamical Chern-Simons gravity ⋮ Nutty black holes in Galileon scalar-tensor gravity ⋮ Slow Kerr-NUT black hole solution in dynamical Chern-Simons modified gravity ⋮ The scalarised Schwarzschild-NUT spacetime ⋮ Gravitational instantons with conformally coupled scalar fields
Cites Work
- Geodesics for the NUT metric and gravitational monopoles
- Rehabilitating space-times with NUTs
- Classical monopoles: Newton, NUT space, gravomagnetic lensing, and atomic spectra
- Mass, dual mass, and gravitational entropy
- Collocation Software for Boundary-Value ODEs
- Peccei-Quinn Mechanism in Gravity and the Nature of the Barbero-Immirzi Parameter
- Physical interpretation of the NUT family of solutions
- Empty-Space Generalization of the Schwarzschild Metric
- The Gregory-Laflamme instability and non-uniform generalizations of NUT strings
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