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  2. Hawking radiation - Wikipedia

    en.wikipedia.org/wiki/Hawking_radiation

    Hawking radiation is the theoretical thermal black-body radiation released outside a black hole's event horizon.This is counterintuitive because once ordinary electromagnetic radiation is inside the event horizon, it cannot escape.

  3. Blackhole exploit kit - Wikipedia

    en.wikipedia.org/wiki/Blackhole_exploit_kit

    Blackhole exploit kit was released on "Malwox", an underground Russian hacking forum. It made its first appearance in 2010. [5]The supposedly Russian creators use the names "HodLuM" and "Paunch".

  4. Black hole cosmology - Wikipedia

    en.wikipedia.org/wiki/Black_hole_cosmology

    A black hole cosmology (also called Schwarzschild cosmology or black hole cosmological model) is a cosmological model in which the observable universe is the interior of a black hole. Such models were originally proposed by theoretical physicist Raj Kumar Pathria, [1] and concurrently by mathematician I. J. Good. [2]

  5. The Five Ages of the Universe - Wikipedia

    en.wikipedia.org/wiki/The_Five_Ages_of_the_Universe

    The Black Hole Era is defined as "40 < n < 100". In this era, according to the book, organized matter will remain only in the form of black holes. Black holes themselves slowly "evaporate" away the matter contained in them, by the quantum mechanical process of Hawking radiation. By the end of this era, only extremely low-energy photons ...

  6. TON 618 - Wikipedia

    en.wikipedia.org/wiki/TON_618

    Size comparison of the event horizons of the black holes of TON 618 and Phoenix A.The orbit of Neptune (white oval) is included for comparison. As a quasar, TON 618 is believed to be the active galactic nucleus at the center of a galaxy, the engine of which is a supermassive black hole feeding on intensely hot gas and matter in an accretion disc.

  7. List of least massive black holes - Wikipedia

    en.wikipedia.org/wiki/List_of_least_massive...

    97% chance of prompt collapse into a black hole immediately after merger. Alternative study suggests collapse 2.5 hours later. NGC 3201-1: 4.36 ± 0.41: 15,600 (see Notes) Spectroscopic radial velocity measurements of noninteracting companion. In globular cluster NGC 3201. Companion is 0.8M ☉ main sequence turn-off. GRO J1719-24/

  8. Black hole (networking) - Wikipedia

    en.wikipedia.org/wiki/Black_hole_(networking)

    Download QR code; Wikidata item; Print/export Download as PDF; ... A null route or black hole route is a network route (routing table entry) that goes nowhere.

  9. Event horizon - Wikipedia

    en.wikipedia.org/wiki/Event_horizon

    Closer to the black hole spacetime starts to deform. In some convenient coordinate systems, there are more paths going towards the black hole than paths moving away. [Note 1] Inside the event horizon all future time paths bring the particle closer to the center of the black hole.