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  2. Black hole - Wikipedia

    en.wikipedia.org/wiki/Black_hole

    The size of a black hole, as determined by the radius of the event horizon, ... The extra energy is taken from the rotational energy of the black hole.

  3. Micro black hole - Wikipedia

    en.wikipedia.org/wiki/Micro_black_hole

    At this stage, a black hole would have a Hawking temperature of ⁠ T P / 8π ⁠ (5.6 × 10 30 K), which means an emitted Hawking particle would have an energy comparable to the mass of the black hole. Thus, a thermodynamic description breaks down. Such a micro black hole would also have an entropy of only 4 π nats, approximately the minimum ...

  4. Large extra dimensions - Wikipedia

    en.wikipedia.org/wiki/Large_extra_dimensions

    For larger numbers of dimensions, fixing the Planck scale at 1 TeV, the size of the extra-dimensions become smaller and as small as 1 femtometer for six extra dimensions. By reducing the fundamental scale to the weak scale, the fundamental theory of quantum gravity , such as string theory , might be accessible at colliders such as the Tevatron ...

  5. Higher-dimensional Einstein gravity - Wikipedia

    en.wikipedia.org/wiki/Higher-dimensional...

    The black ring is a solution of five-dimensional general relativity. It inherits its name from the fact that its event horizon is topologically S 1 × S 2. This is in contrast to other known black hole solutions in five dimensions which have horizon topology S 3.

  6. List of most massive black holes - Wikipedia

    en.wikipedia.org/wiki/List_of_most_massive_black...

    The supermassive black hole at the core of Messier 87, here shown by an image by the Event Horizon Telescope, is among the black holes in this list.. This is an ordered list of the most massive black holes so far discovered (and probable candidates), measured in units of solar masses (M ☉), approximately 2 × 10 30 kilograms.

  7. Schwarzschild radius - Wikipedia

    en.wikipedia.org/wiki/Schwarzschild_radius

    A classification of black holes by mass: Micro black hole and extra-dimensional black hole; Planck length; Primordial black hole, a hypothetical leftover of the Big Bang; Stellar black hole, which could either be a static black hole or a rotating black hole; Supermassive black hole, which could also either be a static black hole or a rotating ...

  8. Supermassive black hole - Wikipedia

    en.wikipedia.org/wiki/Supermassive_black_hole

    [71] [72] An empirical correlation between the size of supermassive black holes and the stellar velocity dispersion of a galaxy bulge [73] is called the M–sigma relation. An AGN is now considered to be a galactic core hosting a massive black hole that is accreting matter and displays a sufficiently strong luminosity.

  9. Sagittarius A* - Wikipedia

    en.wikipedia.org/wiki/Sagittarius_A*

    Sagittarius A*, abbreviated as Sgr A* (/ ˈ s æ dʒ ˈ eɪ s t ɑːr / SADGE-AY-star [3]), is the supermassive black hole [4] [5] [6] at the Galactic Center of the Milky Way.Viewed from Earth, it is located near the border of the constellations Sagittarius and Scorpius, about 5.6° south of the ecliptic, [7] visually close to the Butterfly Cluster (M6) and Lambda Scorpii.