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  2. BTZ black hole - Wikipedia

    en.wikipedia.org/wiki/BTZ_black_hole

    In 1992, Bañados, Teitelboim, and Zanelli discovered the BTZ black hole solution (Bañados, Teitelboim & Zanelli 1992).This came as a surprise, because when the cosmological constant is zero, a vacuum solution of (2+1)-dimensional gravity is necessarily flat (the Weyl tensor vanishes in three dimensions, while the Ricci tensor vanishes due to the Einstein field equations, so the full Riemann ...

  3. Kretschmann scalar - Wikipedia

    en.wikipedia.org/wiki/Kretschmann_scalar

    where is the Ricci curvature tensor and is the Ricci scalar curvature (obtained by taking successive traces of the Riemann tensor). The Ricci tensor vanishes in vacuum spacetimes (such as the Schwarzschild solution mentioned above), and hence there the Riemann tensor and the Weyl tensor coincide, as do their invariants.

  4. Eddington–Finkelstein coordinates - Wikipedia

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

    Schwarzschild solution in Schwarzschild coordinates, with two space dimensions suppressed, leaving just the time t and the distance from the center r. In red the incoming null geodesics. In blue outcoming null geodesics. In green the null light cones on which borders light moves, while massive objects move inside the cones.

  5. Weyl metrics - Wikipedia

    en.wikipedia.org/wiki/Weyl_metrics

    where (,) and (,) are two metric potentials dependent on Weyl's canonical coordinates {,}.The coordinate system {,,,} serves best for symmetries of Weyl's spacetime (with two Killing vector fields being = and =) and often acts like cylindrical coordinates, [2] but is incomplete when describing a black hole as {,} only cover the horizon and its exteriors.

  6. Ricci-flat manifold - Wikipedia

    en.wikipedia.org/wiki/Ricci-flat_manifold

    In 1916, Karl Schwarzschild found the Schwarzschild metrics, which are Ricci-flat Lorentzian manifolds of nonzero curvature. [3] Roy Kerr later found the Kerr metrics , a two-parameter family containing the Schwarzschild metrics as a special case. [ 4 ]

  7. This 3-Move, Full-Body Mobility Routine Will Boost Your Workouts

    www.aol.com/lifestyle/3-move-full-body-mobility...

    This three-exercise mobility routine takes only about 10 minutes and will help to improve joint health and movement for better workouts. This 3-Move, Full-Body Mobility Routine Will Boost Your ...

  8. The 66-year-old demonstrated a “three-minuteworkout to strengthen abs. The fitness star demonstrated a total of five simple moves, including punches, side crunches, and marching twists.

  9. Derivation of the Schwarzschild solution - Wikipedia

    en.wikipedia.org/wiki/Derivation_of_the...

    In deriving the Schwarzschild metric, it was assumed that the metric was vacuum, spherically symmetric and static. The static assumption is unneeded, as Birkhoff's theorem states that any spherically symmetric vacuum solution of Einstein's field equations is stationary; the Schwarzschild solution thus follows