Stationary spacetimes with time-dependent real scalar fields
DOI10.1088/1361-6382/ABF896zbMath1480.83079arXiv2101.05816OpenAlexW3126114103MaRDI QIDQ5163273
Publication date: 3 November 2021
Published in: Classical and Quantum Gravity (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2101.05816
Black holes (83C57) Closed and approximate solutions to the Schrödinger, Dirac, Klein-Gordon and other equations of quantum mechanics (81Q05) Classes of solutions; algebraically special solutions, metrics with symmetries for problems in general relativity and gravitational theory (83C20) Covariant wave equations in quantum theory, relativistic quantum mechanics (81R20) Kaluza-Klein and other higher-dimensional theories (83E15) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05)
Related Items (1)
Cites Work
- Unnamed Item
- Generating time dependent conformally coupled Einstein-scalar solutions
- Conditions for non-existence of static or stationary, Einstein-Maxwell, non-inheriting black-holes
- Static spherically-symmetric scalar-field theory in general relativity
- Massless scalar static spheres
- Killing vector fields and the Einstein-Maxwell field equations in general relativity
- Killing vector fields and the Einstein-Maxwell field equations with perfect fluid source
- The structure of groups of motions admitted by Einstein-Maxwell space-times
- Does three-dimensional electromagnetic field inherit the spacetime symmetries?
- Asymptotically flat black holes with scalar hair: A review
- Gravitational Chern–Simons Lagrangian terms and spherically symmetric spacetimes
- Symmetry inheritance of scalar fields
- Kerr-like metric in Brans–Dicke theory
- Janis–Newman–Winicour and Wyman Solutions are the Same
- Black Hole Uniqueness Theorems
- On symmetry inheritance of nonminimally coupled scalar fields
- New no-scalar-hair theorem for black holes
- Geometrization conditions for perfect fluids, scalar fields, and electromagnetic fields
- Note on the Kerr Spinning-Particle Metric
- General Relativity
This page was built for publication: Stationary spacetimes with time-dependent real scalar fields