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  2. The First Three Minutes: A Modern View of the Origin of the ...

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  3. Boltzmann brain - Wikipedia

    en.wikipedia.org/wiki/Boltzmann_brain

    In this scenario, the universe spends the vast majority of eternity in a featureless state of heat death; however, over enough eons, eventually a very rare thermal fluctuation will occur where atoms bounce off each other in exactly such a way as to form a substructure equivalent to our entire observable universe. Boltzmann argues that, while ...

  4. Timelapse of the Future - Wikipedia

    en.wikipedia.org/wiki/Timelapse_of_the_Future

    The music video is a refreshed art installation-like version of Timelapse of the Future, similar to the draft version tweeted by Boswell in 2018, with some points omitted to fit the song's duration, and with some points shuffled to fit the lyrics. Some of the videos on the other songs on the EP of the same name also

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  6. The First Three Minutes - Wikipedia

    en.wikipedia.org/wiki/The_First_Three_Minutes

    The First Three Minutes attempts to explain the early stages of the universe after the Big Bang.Weinberg begins by recounting a creation myth from the Younger Edda and goes on to explain how, in the first half of the twentieth century, cosmologists have come to know something of the real history of the universe.

  7. Rare Earth hypothesis - Wikipedia

    en.wikipedia.org/wiki/Rare_Earth_hypothesis

    The Rare Earth hypothesis argues that planets with complex life, like Earth, are exceptionally rare.. In planetary astronomy and astrobiology, the Rare Earth hypothesis argues that the origin of life and the evolution of biological complexity, such as sexually reproducing, multicellular organisms on Earth, and subsequently human intelligence, required an improbable combination of astrophysical ...

  8. Universe - Wikipedia

    en.wikipedia.org/wiki/Universe

    Perhaps unsurprisingly, our universe has just the right mass–energy density, equivalent to about 5 protons per cubic meter, which has allowed it to expand for the last 13.8 billion years, giving time to form the universe as observed today. [64] [65] There are dynamical forces acting on the particles in the universe which affect the expansion ...

  9. Nucleosynthesis - Wikipedia

    en.wikipedia.org/wiki/Nucleosynthesis

    After about 20 minutes, the universe had expanded and cooled to a point at which these high-energy collisions among nucleons ended, so only the fastest and simplest reactions occurred, leaving our universe containing hydrogen and helium. The rest is traces of other elements such as lithium and the hydrogen isotope deuterium. Nucleosynthesis in ...