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  2. Baryogenesis - Wikipedia

    en.wikipedia.org/wiki/Baryogenesis

    Once the universe expanded and cooled to a critical temperature of approximately 2 × 10 12 K, [3] quarks combined into normal matter and antimatter and proceeded to annihilate up to the small initial asymmetry of about one part in five billion, leaving the matter around us. [3] Free and separate individual quarks and antiquarks have never been ...

  3. Baryon asymmetry - Wikipedia

    en.wikipedia.org/wiki/Baryon_asymmetry

    Neither the standard model of particle physics nor the theory of general relativity provides a known explanation for why this should be so, and it is a natural assumption that the universe is neutral with all conserved charges. [3] The Big Bang should have produced equal amounts of matter and antimatter. Since this does not seem to have been ...

  4. Flatness problem - Wikipedia

    en.wikipedia.org/wiki/Flatness_problem

    The local geometry of the universe is determined by whether the relative density Ω is less than, equal to or greater than 1. From top to bottom: a spherical universe with greater than critical density (Ω>1, k>0); a hyperbolic, underdense universe (Ω<1, k<0); and a flat universe with exactly the critical density (Ω=1, k=0).

  5. Here’s why the universe has more matter than antimatter - AOL

    www.aol.com/news/why-universe-more-matter...

    All the particles that make up the matter around us, such electrons and protons, have antimatter versions which are nearly identical, but with mirrored properties such as the opposite electric charge.

  6. Leptogenesis - Wikipedia

    en.wikipedia.org/wiki/Leptogenesis

    Why does the observable universe have more matter than antimatter? (more unsolved problems in physics) In physical cosmology , leptogenesis is the generic term for hypothetical physical processes that produced an asymmetry between leptons and antileptons in the very early universe , resulting in the present-day dominance of leptons over ...

  7. Right again, Einstein! Study shows how antimatter ... - AOL

    www.aol.com/news/again-einstein-study-shows...

    The researchers reduced the magnetic fields to set the antimatter free in order to observe whether or not it would fall once the influence of gravity became apparent. It did, behaving as hydrogen ...

  8. B–Bbar oscillation - Wikipedia

    en.wikipedia.org/wiki/B–Bbar_oscillation

    mixing phenomena led physicists to propose the construction of the so-named "B factories" in the early 1990s. They realized that a precise B – B oscillation measure could pin down the unitarity triangle and perhaps explain the excess of matter over antimatter in the universe.

  9. NYT ‘Connections’ Hints and Answers Today, Sunday, December 15

    www.aol.com/nyt-connections-hints-answers-today...

    Spoilers ahead! We've warned you. We mean it. Read no further until you really want some clues or you've completely given up and want the answers ASAP. Get ready for all of today's NYT ...