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A stationary, axisymmetric, asymptotically flat vacuum solution describing the exterior geometry of an uncharged rotating black hole.
wp-physics-kerr-spacetimenlab-kerr-spacetimeeinstein-online-black-holeseinstein-equationEach relation below ends at this concept.
This is an authored directed relation from the source endpoint to the target endpoint.
The Kerr spacetime is the stationary, axisymmetric, asymptotically flat vacuum model used for an uncharged rotating black hole.
The target is a model, idealization, restricted ansatz, approximation scheme, phenomenological fit, or historical representation used for the source system or theory. It need not have a universal small error parameter and is not thereby a controlled limit or effective theory. The edge label and detail must identify the precise status.
einstein-online-black-holesnasa-black-holesThis is an authored directed relation from the source endpoint to the target endpoint.
The Kerr geometry is a rotating vacuum solution of the Einstein equation.
The target is a model, idealization, restricted ansatz, approximation scheme, phenomenological fit, or historical representation used for the source system or theory. It need not have a universal small error parameter and is not thereby a controlled limit or effective theory. The edge label and detail must identify the precise status.
einstein-equationeinstein-online-black-holesThis is an authored directed relation from the source endpoint to the target endpoint.
The Kerr solution is a Lorentzian manifold with a stationary, axisymmetric metric satisfying the vacuum Einstein equation.
A mathematical concept supplies part of the formal language, state space, representation, or analytic machinery used by a scientific or mathematical-physics concept. The source is the mathematical predecessor; this does not claim that physical content follows from mathematics alone.
lee-smooth-manifoldseinstein-equationEach relation below starts at this concept.
No direct relations are authored in this direction.