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  2. Big Bounce - Wikipedia

    en.wikipedia.org/wiki/Big_Bounce

    Such an interaction avoids the unphysical Big Bang singularity, replacing it with a cusp-like bounce at a finite minimum scale factor, before which the universe was contracting. This scenario also explains why the present Universe at the largest scales appears spatially flat, homogeneous, and isotropic, providing a physical alternative to ...

  3. Ultimate fate of the universe - Wikipedia

    en.wikipedia.org/wiki/Ultimate_fate_of_the_universe

    When Einstein found that his general relativity equations could easily be solved in such a way as to allow the universe to be expanding at the present and contracting in the far future, he added to those equations what he called a cosmological constant ⁠— ⁠essentially a constant energy density, unaffected by any expansion or contraction ...

  4. Cosmic Jackpot - Wikipedia

    en.wikipedia.org/wiki/Cosmic_Jackpot

    In Cosmic Jackpot, Davies argues that certain universal fundamental physical constants are precisely adjusted to make life in the Universe possible: that we have, in a sense, won a "cosmic jackpot," and that conditions are "just right" for life, as in The Story of the Three Bears. As Davies writes elsewhere, "There is now broad agreement among ...

  5. Anthropic principle - Wikipedia

    en.wikipedia.org/wiki/Anthropic_principle

    The absurd universe: Our universe just happens to be the way it is. The unique universe: There is a deep underlying unity in physics that necessitates the Universe being the way it is. A Theory of Everything will explain why the various features of the Universe must have exactly the values that have been recorded.

  6. Big Crunch - Wikipedia

    en.wikipedia.org/wiki/Big_Crunch

    The Big Crunch is a hypothetical scenario for the ultimate fate of the universe, in which the expansion of the universe eventually reverses and the universe recollapses, ultimately causing the cosmic scale factor to reach absolute zero, an event potentially followed by a reformation of the universe starting with another Big Bang.

  7. Here’s why Victoria Kjaer Theilvig’s Miss Universe win has ...

    www.aol.com/why-victoria-kjaer-theilvig-miss...

    A Danish model was crowned Miss Universe on Saturday, and avid watchers of the famed competition are celebrating the winner being a biological woman following the pageant’s decision permitting ...

  8. The dreams of a 60-year-old beauty contestant come to an ...

    www.aol.com/news/dreams-60-old-beauty-contestant...

    A 60-year-old woman saw her dreams of becoming the oldest Miss Universe contestant in history melt away in a haze of sequins and selfies Saturday at Argentina’s annual beauty pageant. Alejandra ...

  9. Friedmann–Lemaître–Robertson–Walker metric - Wikipedia

    en.wikipedia.org/wiki/Friedmann–Lemaître...

    The Friedmann–Lemaître–Robertson–Walker metric (FLRW; / ˈ f r iː d m ə n l ə ˈ m ɛ t r ə ... /) is a metric that describes a homogeneous, isotropic, expanding (or otherwise, contracting) universe that is path-connected, but not necessarily simply connected.