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  2. Baryogenesis - Wikipedia

    en.wikipedia.org/wiki/Baryogenesis

    The Standard Model can incorporate baryogenesis, though the amount of net baryons (and leptons) thus created may not be sufficient to account for the present baryon asymmetry. There is a required one excess quark per billion quark-antiquark pairs in the early universe in order to provide all the observed matter in the universe. [3]

  3. Affleck–Dine mechanism - Wikipedia

    en.wikipedia.org/wiki/Affleck–Dine_mechanism

    The Affleck–Dine mechanism (AD mechanism) is a postulated mechanism for explaining baryogenesis during the primordial Universe immediately following the Big Bang.Thus, the AD mechanism may explain the asymmetry between matter and antimatter in the current Universe.

  4. Cosmological phase transition - Wikipedia

    en.wikipedia.org/wiki/Cosmological_phase_transition

    Particle physics models which account for dark matter or which lead to successful baryogenesis may predict a strongly first-order electroweak phase transition. [20] The electroweak baryogenesis model may explain the baryon asymmetry in the universe, the observation that the amount of matter vastly exceeds the amount of matter. [4]

  5. Baryon asymmetry - Wikipedia

    en.wikipedia.org/wiki/Baryon_asymmetry

    In physical cosmology, the baryon asymmetry problem, also known as the matter asymmetry problem or the matter–antimatter asymmetry problem, [1] [2] is the observed imbalance in baryonic matter (the type of matter experienced in everyday life) and antibaryonic matter in the observable universe.

  6. Template:Big Bang timeline - Wikipedia

    en.wikipedia.org/wiki/Template:Big_Bang_timeline

    Download as PDF; Printable version; In other projects Wikidata item; Appearance. move to sidebar hide This page was last edited on 18 September 2021, at 19:15 ...

  7. Weakless universe - Wikipedia

    en.wikipedia.org/wiki/Weakless_universe

    Baryogenesis and leptogenesis within the Standard Model rely on the weak interaction: For matter not to be wiped off by anti-matter at the very early universe, the universe must either have to start with a different amount of each (i.e. initial non-zero baryon number), or admit Sakharov's conditions to baryogenesis. In the latter case, there ...

  8. CPLEAR experiment - Wikipedia

    en.wikipedia.org/wiki/CPLEAR_experiment

    A possible answer to this question is baryogenesis, the hypothetical physical process that took place during the early universe that produced baryonic asymmetry, i.e. the imbalance of matter (baryons) and antimatter (antibaryons) in the observed universe. However, baryogenesis is only possible under the following conditions proposed by Andrei ...

  9. Astroparticle physics - Wikipedia

    en.wikipedia.org/wiki/Astroparticle_physics

    Another question for astroparticle physicists is why is there so much more matter than antimatter in the universe today. Baryogenesis is the term for the hypothetical processes that produced the unequal numbers of baryons and antibaryons in the early universe, which is why the universe is made of matter today, and not antimatter. [6]