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  2. 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.

  3. Cosmological natural selection - Wikipedia

    en.wikipedia.org/wiki/Cosmological_natural_selection

    Black holes have a role in natural selection. In fecund theory a collapsing [clarification needed] black hole causes the emergence of a new universe on the "other side", whose fundamental constant parameters (masses of elementary particles, Planck constant, elementary charge, and so forth) may differ slightly from those of the universe where the black hole collapsed.

  4. 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.

  5. Ultimate fate of the universe - Wikipedia

    en.wikipedia.org/wiki/Ultimate_fate_of_the_universe

    The ultimate fate of the universe is a topic in physical cosmology, whose theoretical restrictions allow possible scenarios for the evolution and ultimate fate of the universe to be described and evaluated. Based on available observational evidence, deciding the fate and evolution of the universe has become a valid cosmological question, being ...

  6. Inhomogeneous cosmology - Wikipedia

    en.wikipedia.org/wiki/Inhomogeneous_cosmology

    An inhomogeneous cosmology is a physical cosmological theory (an astronomical model of the physical universe's origin and evolution) which, unlike the dominant cosmological concordance model, assumes that inhomogeneities in the distribution of matter across the universe affect local gravitational forces (i.e., at the galactic level) enough to skew our view of the Universe. [3]

  7. Fractal cosmology - Wikipedia

    en.wikipedia.org/wiki/Fractal_cosmology

    The universe has been observed to be homogeneous and isotropic (i.e. is smoothly distributed) at very large scales, as is expected in a standard Big Bang or Friedmann-Lemaître-Robertson-Walker cosmology, and in most interpretations of the Lambda-Cold Dark Matter model.

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

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

    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 ...

  9. Woman, Culture, and Society - Wikipedia

    en.wikipedia.org/wiki/Woman,_Culture,_and_Society

    Woman, Culture, and Society, first published in 1974 (Stanford University Press), is a book consisting of 16 papers contributed by female authors and an introduction by the editors Michelle Zimbalist Rosaldo and Louise Lamphere.

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