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  2. White hole - Wikipedia

    en.wikipedia.org/wiki/White_hole

    Like black holes, white holes have properties such as mass, charge, and angular momentum.They attract matter like any other mass, but objects falling towards a white hole would never actually reach the white hole's event horizon (though in the case of the maximally extended Schwarzschild solution, discussed below, the white hole event horizon in the past becomes a black hole event horizon in ...

  3. Category:White holes - Wikipedia

    en.wikipedia.org/wiki/Category:White_holes

    This page was last edited on 16 November 2024, at 05:54 (UTC).; Text is available under the Creative Commons Attribution-ShareAlike 4.0 License; additional terms may apply.

  4. White hole (disambiguation) - Wikipedia

    en.wikipedia.org/wiki/White_hole_(disambiguation)

    A white hole is a hypothetical region of spacetime which cannot be entered from the outside, although matter and light can escape from it. White hole may also refer to: Arts and entertainment

  5. Kruskal–Szekeres coordinates - Wikipedia

    en.wikipedia.org/wiki/Kruskal–Szekeres_coordinates

    The negative T singularity is the time-reversed black hole, sometimes dubbed a "white hole". Particles can escape from a white hole but they can never return. The maximally extended Schwarzschild geometry can be divided into 4 regions each of which can be covered by a suitable set of Schwarzschild coordinates.

  6. Category:Fiction about white holes - Wikipedia

    en.wikipedia.org/wiki/Category:Fiction_about...

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  7. Igor Dmitriyevich Novikov - Wikipedia

    en.wikipedia.org/wiki/Igor_Dmitriyevich_Novikov

    Novikov put forward the idea of white holes in 1964. He also formulated the Novikov self-consistency principle in the mid-1980s, a contribution to the theory of time travel. Novikov moved to Copenhagen, Denmark, where he worked and taught at the Niels Bohr Institute. He returned to Russia in 2001.

  8. Eddington–Finkelstein coordinates - Wikipedia

    en.wikipedia.org/wiki/Eddington–Finkelstein...

    The horizon r = 2GM and finite v (the black hole horizon) is different from that with r = 2GM and finite u (the white hole horizon) . The metric in Kruskal–Szekeres coordinates covers all of the extended Schwarzschild spacetime in a single coordinate system. Its chief disadvantage is that in those coordinates the metric depends on both the ...

  9. Compact object - Wikipedia

    en.wikipedia.org/wiki/Compact_object

    In astronomy, the term compact object (or compact star) refers collectively to white dwarfs, neutron stars, and black holes.It could also include exotic stars if such hypothetical, dense bodies are confirmed to exist.