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The unique spherically symmetric vacuum solution of the Einstein equation, with a black-hole exterior characterized by mass in its asymptotically flat form.
wp-physics-schwarzschild-spacetimenlab-schwarzschild-spacetimeeinstein-online-black-holeseinstein-equationEach relation below ends at this concept.
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The Schwarzschild black-hole spacetime is the static, spherically symmetric, asymptotically flat vacuum model of an uncharged nonrotating 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 Schwarzschild geometry solves the vacuum Einstein equation under spherical symmetry.
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 Schwarzschild solution is a Lorentzian manifold with a metric satisfying the vacuum Einstein equation and spherical symmetry.
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.
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