Geometric properties of a certain class of compact dynamical horizons in locally rotationally symmetric class II spacetimes
DOI10.1142/S0219887821500109arXiv2009.09966MaRDI QIDQ6193856
Abbas Mohamed Sherif, Peter K. S. Dunsby
Publication date: 19 March 2024
Published in: International Journal of Geometric Methods in Modern Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2009.09966
compact Riemannian manifoldsRicci flowdynamical horizonslocally rotationally symmetric class II spacetimes
Black holes (83C57) Applications of differential geometry to physics (53Z05) Methods of global Riemannian geometry, including PDE methods; curvature restrictions (53C21) Non-Euclidean differential geometry (53A35) Ricci flows (53E20)
Cites Work
- Unnamed Item
- Stability of marginally outer trapped surfaces and existence of marginally outer trapped tubes
- Four-manifolds with positive curvature operator
- Proof of the positive mass theorem. II
- Isolated and dynamical horizons and their applications
- Three-manifolds with positive Ricci curvature
- Some uniqueness results for dynamical horizons
- The general theory of space-like congruences with an application to vorticity in relativistic hydrodynamics
- Conformal changes of Riemannian metrics
- Riemannian manifolds with positive mean curvature
- Dynamical Horizons: Energy, Angular Momentum, Fluxes, and Balance Laws
- Horizon energy and angular momentum from a Hamiltonian perspective
- Marginally trapped tubes and dynamical horizons
- Covariant perturbations of Schwarzschild black holes
- Scalar field and electromagnetic perturbations on locally rotationally symmetric spacetimes
- Some results on cosmological and astrophysical horizons and trapped surfaces
- Republication of: Relativistic cosmology
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