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  2. Rotating black hole - Wikipedia

    en.wikipedia.org/wiki/Rotating_black_hole

    A rotating black hole is a black hole that possesses angular momentum. In particular, it rotates about one of its axes of symmetry. All celestial objects – planets, stars , galaxies, black holes – spin. [1] [2] [3] The boundaries of a Kerr black hole relevant to astrophysics. Note that there are no physical "surfaces" as such.

  3. Kerr metric - Wikipedia

    en.wikipedia.org/wiki/Kerr_metric

    The Kerr metric or Kerr geometry describes the geometry of empty spacetime around a rotating uncharged axially symmetric black hole with a quasispherical event horizon.The Kerr metric is an exact solution of the Einstein field equations of general relativity; these equations are highly non-linear, which makes exact solutions very difficult to find.

  4. A Scientist Says Time Travel Is Possible With Ring Lasers - AOL

    www.aol.com/scientist-says-time-travel-possible...

    That’s what a rotating black hole does. In Einstein’s theory, space and time relate to each other. That’s why it’s called space-time. So as the black hole is rotating, it’s actually ...

  5. Closed timelike curve - Wikipedia

    en.wikipedia.org/wiki/Closed_timelike_curve

    the interior of a rotating BTZ black hole; the van Stockum dust (which models a cylindrically symmetric configuration of dust) the Gödel lambda dust (which models a dust with a carefully chosen cosmological constant term) the Tipler cylinder (a cylindrically symmetric metric with CTCs) Bonnor-Steadman solutions describing laboratory situations ...

  6. Outline of black holes - Wikipedia

    en.wikipedia.org/wiki/Outline_of_black_holes

    Ergosphere – region located outside a rotating black hole. Hawking radiation – black-body radiation that is predicted to be emitted by black holes, due to quantum effects near the event horizon. [2] Penrose process – process theorised by Roger Penrose wherein energy can be extracted from a rotating black hole.

  7. Mass in general relativity - Wikipedia

    en.wikipedia.org/wiki/Mass_in_general_relativity

    The Schwarzschild metric of a black hole and the Kerr metric of a rotating black hole are common examples of stationary spacetimes. By definition, a stationary spacetime exhibits time translation symmetry. This is technically called a time-like Killing vector. Because the system has a time translation symmetry, Noether's theorem guarantees that ...

  8. Henriette Elvang - Wikipedia

    en.wikipedia.org/wiki/Henriette_Elvang

    [7] [8] Elvang identified that black holes and black rings can coexist if they are spinning. [9] She named the combination of a spherical black hole surrounded by a black ring a 'Black Saturn'. [10] After her fellowship, Elvang joined the Institute for Advanced Study as a postdoctoral researcher. [7]

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    Get AOL Mail for FREE! Manage your email like never before with travel, photo & document views. Personalize your inbox with themes & tabs. You've Got Mail!

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