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  2. Missing baryon problem - Wikipedia

    en.wikipedia.org/wiki/Missing_baryon_problem

    In cosmology, the missing baryon problem is an observed discrepancy between the amount of baryonic matter detected from shortly after the Big Bang and from more recent epochs. Observations of the cosmic microwave background and Big Bang nucleosynthesis studies have set constraints on the abundance of baryons in the early universe, finding that ...

  3. Big Bang - Wikipedia

    en.wikipedia.org/wiki/Big_Bang

    The Big Bang is a physical theory that describes how the universe expanded from an initial state of high density and temperature. [1] The notion of an expanding universe was first scientifically originated by physicist Alexander Friedmann in 1922 with the mathematical derivation of the Friedmann equations. [2][3][4][5]

  4. Lambda-CDM model - Wikipedia

    en.wikipedia.org/wiki/Lambda-CDM_model

    Astronomy portal. v. t. e. The Lambda-CDM, Lambda cold dark matter, or ΛCDM model is a mathematical model of the Big Bang theory with three major components: a cosmological constant, denoted by lambda (Λ), associated with dark energy. the postulated cold dark matter, denoted by CDM. ordinary matter. It is referred to as the standard model of ...

  5. Baryogenesis - Wikipedia

    en.wikipedia.org/wiki/Baryogenesis

    Astronomy portal. v. t. e. In physical cosmology, baryogenesis (also known as baryosynthesis[1][2]) is the physical process that is hypothesized to have taken place during the early universe to produce baryonic asymmetry, i.e. the imbalance of matter (baryons) and antimatter (antibaryons) in the observed universe. [3]

  6. Neutrino decoupling - Wikipedia

    en.wikipedia.org/wiki/Neutrino_decoupling

    Neutrino decoupling. In Big Bang cosmology, neutrino decoupling was the epoch at which neutrinos ceased interacting with other types of matter, [1] and thereby ceased influencing the dynamics of the universe at early times. [2] Prior to decoupling, neutrinos were in thermal equilibrium with protons, neutrons and electrons, which was maintained ...

  7. History of the Big Bang theory - Wikipedia

    en.wikipedia.org/wiki/History_of_the_Big_Bang_theory

    The history of the Big Bang theory began with the Big Bang 's development from observations and theoretical considerations. Much of the theoretical work in cosmology now involves extensions and refinements to the basic Big Bang model. The theory itself was originally formalised by Father Georges Lemaître in 1927. [1]

  8. Ralph Alpher - Wikipedia

    en.wikipedia.org/wiki/Ralph_Alpher

    Physical cosmology. Ralph Asher Alpher (February 3, 1921 – August 12, 2007) was an American cosmologist, who carried out pioneering work in the early 1950s on the Big Bang model, including Big Bang nucleosynthesis and predictions of the cosmic microwave background radiation.

  9. Georges Lemaître - Wikipedia

    en.wikipedia.org/wiki/Georges_Lemaître

    Lemaître's theory became better known as the "Big Bang theory," a picturesque term playfully coined during a 1949 BBC radio broadcast by the astronomer Fred Hoyle, [26] [27] who was a proponent of the steady state universe and remained so until his death in 2001. Lemaître's proposal met with skepticism from his fellow scientists.