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  2. Sasha Haco - Wikipedia

    en.wikipedia.org/wiki/Sasha_Haco

    In 2020, Haco was heavily featured in the Netflix documentary Black Holes: The Edge of All We Know, which chronicled the use of the Event Horizon Telescope to take the first photograph of a black hole, as well as the work of Haco, Hawking, Perry and Strominger as they attempted to better understand the black hole information paradox. [3] [4]

  3. Oppenheimer–Snyder model - Wikipedia

    en.wikipedia.org/wiki/Oppenheimer–Snyder_model

    While Oppenheimer is remembered in history as the “father of the atomic bomb”, his greatest contribution as a physicist was on the physics of black holes. The work of Oppenheimer and Hartland Snyder helped transform black holes from figments of mathematics to real, physical possibilities – something to be found in the cosmos out there.

  4. List of black holes - Wikipedia

    en.wikipedia.org/wiki/List_of_black_holes

    OJ 287 core black holes — a BL Lac object with a candidate binary supermassive black hole core system [23] PG 1302-102 – the first binary-cored quasar — a pair of supermassive black holes at the core of this quasar [24] [25] SDSS J120136.02+300305.5 core black holes — a pair of supermassive black holes at the centre of this galaxy [26]

  5. 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]

  6. No-hair theorem - Wikipedia

    en.wikipedia.org/wiki/No-hair_theorem

    The no-hair theorem (which is a hypothesis) states that all stationary black hole solutions of the Einstein–Maxwell equations of gravitation and electromagnetism in general relativity can be completely characterized by only three independent externally observable classical parameters: mass, angular momentum, and electric charge.

  7. Black hole starship - Wikipedia

    en.wikipedia.org/wiki/Black_hole_starship

    A black hole weighing 606,000 metric tons (6.06 × 10 8 kg) would have a Schwarzschild radius of 0.9 attometers (0.9 × 10 –18 m, or 9 × 10 –19 m), a power output of 160 petawatts (160 × 10 15 W, or 1.6 × 10 17 W), and a 3.5-year lifespan. With such a power output, the black hole could accelerate to 10% the speed of light in 20 days ...

  8. AdS black hole - Wikipedia

    en.wikipedia.org/wiki/AdS_black_hole

    Download QR code; Print/export Download as PDF; ... black hole is a black hole solution of general relativity or its extensions which represents an isolated ...

  9. Black Holes and Baby Universes and Other Essays - Wikipedia

    en.wikipedia.org/wiki/Black_Holes_and_Baby...

    This book is a collection of essays and lectures written by Hawking, mainly about the makeup of black holes, and why they might be nodes from which other universes grow. Hawking discusses black hole thermodynamics , special relativity , general relativity , and quantum mechanics .