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  2. Galactic Center - Wikipedia

    en.wikipedia.org/wiki/Galactic_Center

    The Black Hole at the Center of the Milky Way. London: Imperial College Press. ISBN 978-1-86094-567-0. Melia, Fulvio (2003). The Black Hole in the Center of Our Galaxy. Princeton: Princeton University Press. ISBN 978-0-691-09505-9. Melia, Fulvio (2007). The Galactic Supermassive Black Hole. Princeton: Princeton University Press. ISBN 978-0-691 ...

  3. The Black Hole (1979 film) - Wikipedia

    en.wikipedia.org/wiki/The_Black_Hole_(1979_film)

    The Black Hole is a 1979 American science fiction film directed by Gary Nelson and produced by Walt Disney Productions.The film stars Maximilian Schell, Robert Forster, Joseph Bottoms, Yvette Mimieux, Anthony Perkins and Ernest Borgnine, while the voices of the main robot characters are provided by Roddy McDowall and Slim Pickens (both uncredited).

  4. 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.

  5. Black–Scholes model - Wikipedia

    en.wikipedia.org/wiki/Black–Scholes_model

    In the standard Black–Scholes model, one can interpret the premium of the binary option in the risk-neutral world as the expected value = probability of being in-the-money * unit, discounted to the present value. The Black–Scholes model relies on symmetry of distribution and ignores the skewness of the

  6. Spaghettification - Wikipedia

    en.wikipedia.org/wiki/Spaghettification

    For small black holes whose Schwarzschild radius is much closer to the singularity, the tidal forces would kill even before the astronaut reaches the event horizon. [ 9 ] [ 10 ] For example, for a black hole of 10 Sun masses [ note 2 ] the above-mentioned rod breaks at a distance of 320 km, well outside the Schwarzschild radius of 30 km.

  7. N-body simulation - Wikipedia

    en.wikipedia.org/wiki/N-body_simulation

    An N-body simulation of the cosmological formation of a cluster of galaxies in an expanding universe. In physics and astronomy, an N-body simulation is a simulation of a dynamical system of particles, usually under the influence of physical forces, such as gravity (see n-body problem for other applications).

  8. Quasi-star - Wikipedia

    en.wikipedia.org/wiki/Quasi-star

    Size comparison of a hypothetical quasi-star to some of the largest known stars. A quasi-star rendered with Celestia. A quasi-star (also called black hole star) is a hypothetical type of extremely massive and luminous star that may have existed early in the history of the Universe.

  9. Ruth Gregory - Wikipedia

    en.wikipedia.org/wiki/Ruth_Gregory

    Gregory was given the 2006 Maxwell Medal and Prize by the Institute of Physics for her contributions to physics at the interface of general relativity and string theory, in particular for her work on the physics of cosmic strings and black holes.

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