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  2. Ring singularity - Wikipedia

    en.wikipedia.org/wiki/Ring_singularity

    Description of a ring singularity. Event horizons and ergospheres of a rotating black hole; the ringularity is located at the equatorial kink of the inner ergosphere at R=a. When a spherical non-rotating body of a critical radius collapses under its own gravitation under general relativity, theory suggests it will collapse to a 0-dimensional ...

  3. Gravitational singularity - Wikipedia

    en.wikipedia.org/wiki/Gravitational_singularity

    While in a non-rotating black hole the singularity occurs at a single point in the model coordinates, called a "point singularity", in a rotating black hole, also known as a Kerr black hole, the singularity occurs on a ring (a circular line), known as a "ring singularity". Such a singularity may also theoretically become a wormhole. [18]

  4. Fuzzball (string theory) - Wikipedia

    en.wikipedia.org/wiki/Fuzzball_(string_theory)

    Fuzzballs are hypothetical objects in superstring theory, intended to provide a fully quantum description of the black holes predicted by general relativity.. The fuzzball hypothesis dispenses with the singularity at the heart of a black hole by positing that the entire region within the black hole's event horizon is actually an extended object: a ball of strings, which are advanced as the ...

  5. Naked singularity - Wikipedia

    en.wikipedia.org/wiki/Naked_singularity

    In general relativity, a naked singularity is a hypothetical gravitational singularity without an event horizon.. When there exists at least one causal geodesic that, in the future, extends to an observer either at infinity or to an observer comoving with the collapsing cloud, and in the past terminates at the gravitational singularity, then that singularity is referred to as a naked ...

  6. Accretion disk - Wikipedia

    en.wikipedia.org/wiki/Accretion_disk

    An accretion disk is a structure (often a circumstellar disk) formed by diffuse material [a] in orbital motion around a massive central body. The central body is most frequently a star. Friction, uneven irradiance, magnetohydrodynamic effects, and other forces induce instabilities causing orbiting material in the disk to spiral inward toward ...

  7. Timeline of black hole physics - Wikipedia

    en.wikipedia.org/wiki/Timeline_of_black_hole_physics

    1967 — Jocelyn Bell discovers and analyzes the first radio pulsar, direct evidence for a neutron star [ 2] 1967 — Werner Israel presents the proof of the no-hair theorem at King's College London. 1967 — John Wheeler introduces the term "black hole" in his lecture to the American Association for the Advancement of Science [ 1] 1968 ...

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