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  2. Schwarzschild radius - Wikipedia

    en.wikipedia.org/wiki/Schwarzschild_radius

    The Schwarzschild radius or the gravitational radius is a physical parameter in the Schwarzschild solution to Einstein's field equations that corresponds to the radius defining the event horizon of a Schwarzschild black hole. It is a characteristic radius associated with any quantity of mass.

  3. File:Kruskal diagram of Schwarzschild chart.svg - Wikipedia

    en.wikipedia.org/wiki/File:Kruskal_diagram_of...

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  4. Kruskal–Szekeres coordinates - Wikipedia

    en.wikipedia.org/wiki/Kruskal–Szekeres_coordinates

    In the Schwarzschild coordinates, the Schwarzschild radius = is the radial coordinate of the event horizon = =. In the Kruskal–Szekeres coordinates the event horizon is given by =. Note that the metric is perfectly well defined and non-singular at the event horizon.

  5. File:Schwarzschild cross section.svg - Wikipedia

    en.wikipedia.org/wiki/File:Schwarzschild_cross...

    English: The Schwarzschild interior (blue) and exterior (black) solutions. r s : Schwarzschild radius; r g : r -coordinate on the body's surface; ℛ 2 = r g 3 / r s ; sin η g = r g /ℛ Date

  6. Eddington–Finkelstein coordinates - Wikipedia

    en.wikipedia.org/wiki/Eddington–Finkelstein...

    In these coordinates, the horizon is the black hole horizon (nothing can come out). The diagram for u-r coordinates is the same diagram turned upside down and with u and v interchanged on the diagram. In that case the horizon is the white hole horizon, which matter and light can come out of, but nothing can go in.

  7. Isotropic coordinates - Wikipedia

    en.wikipedia.org/wiki/Isotropic_coordinates

    where = (,) are coordinates and is the Riemannian metric on the 2 sphere of unit radius. That is, these nested coordinate spheres do in fact represent geometric spheres, but the appearance of b ( r 0 ) r {\displaystyle b(r_{0})\,r} rather than r {\displaystyle r} shows that the radial coordinate do not correspond to area in the same way as for ...

  8. File:Schwarzchild-metric.jpg - Wikipedia

    en.wikipedia.org/wiki/File:Schwarzchild-metric.jpg

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  9. Two-body problem in general relativity - Wikipedia

    en.wikipedia.org/wiki/Two-body_problem_in...

    For example, the Schwarzschild radius r s of the Earth is roughly 9 mm (3 ⁄ 8 inch); at the surface of the Earth, the corrections to Newtonian gravity are only one part in a billion. The Schwarzschild radius of the Sun is much larger, roughly 2953 meters, but at its surface, the ratio r s / r is roughly 4 parts in a million.