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baryogenesis | A Wisdom Archive on baryogenesis | | baryogenesis A selection of articles related to baryogenesis | |
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baryogenesis, Baryogenesis, Baryogenesis - Background, Baryogenesis - Matter content in the Universe, Baryogenesis - The Sakharov conditions, Baryogenesis - A naïve estimation of the baryon asymmetry of the Universe, Baryogenesis - Articles, Baryogenesis - Textbooks, Baryogenesis - The baryon asymmetry parameter, Leptons., CP-symmetry, CP violation.
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| ARTICLES RELATED TO baryogenesis | | | | |  baryogenesis: Encyclopedia II - Big Bang - Observational evidenceIt is generally stated that there are three observational pillars that support the Big Bang theory of cosmology. These are the Hubble-type expansion seen in the redshifts of galaxies, the detailed measurements of the cosmic microwave background, and the abundance of light elements. (See Big Bang nucleosynthesis.) Additionally, the observed correlation function of large-scale structure of the cosmos fits well with standard Big Bang theory.
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See also:Big Bang, Big Bang - History, Big Bang - Overview, Big Bang - Theoretical underpinnings, Big Bang - Observational evidence, Big Bang - Hubble's law expansion, Big Bang - Cosmic microwave background radiation, Big Bang - Abundance of primordial elements, Big Bang - Galactic evolution and distribution, Big Bang - Features issues and problems, Big Bang - Horizon problem, Big Bang - Flatness problem, Big Bang - Magnetic monopoles, Big Bang - Baryon asymmetry, Big Bang - Globular cluster age, Big Bang - Dark matter, Big Bang - Dark energy, Big Bang - The future according to the Big Bang theory, Big Bang - Speculative physics beyond the Big Bang, Big Bang - Philosophical and religious interpretations Read more here: » Big Bang: Encyclopedia II - Big Bang - Observational evidence |
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| | | | | baryogenesis: Encyclopedia II - Big Bang - History The Big Bang theory developed from observations and theoretical considerations. Observationally, it was determined that most spiral nebulae were receding from Earth, but those who made the observation weren't aware of the cosmological implications, nor that the supposed nebulae were actually galaxies outside our own Milky Way. In 1927, the Belgian Catholic priest Georges Lemaître independently derived the Friedmann-Lemaître-Robertson-Walker equations and proposed, on the basis of the recession of spiral nebulae, that the Universe began with the "explosion" of a "primeval atom"†...
See also:Big Bang, Big Bang - History, Big Bang - Overview, Big Bang - Theoretical underpinnings, Big Bang - Observational evidence, Big Bang - Hubble's law expansion, Big Bang - Cosmic microwave background radiation, Big Bang - Abundance of primordial elements, Big Bang - Galactic evolution and distribution, Big Bang - Features issues and problems, Big Bang - Horizon problem, Big Bang - Flatness problem, Big Bang - Magnetic monopoles, Big Bang - Baryon asymmetry, Big Bang - Globular cluster age, Big Bang - Dark matter, Big Bang - Dark energy, Big Bang - The future according to the Big Bang theory, Big Bang - Speculative physics beyond the Big Bang, Big Bang - Philosophical and religious interpretations Read more here: » Big Bang: Encyclopedia II - Big Bang - History |
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| | | | | baryogenesis: Encyclopedia II - Big Bang - The future according to the Big Bang theory Before observations of dark energy, cosmologists considered two scenarios for the future of the Universe. If the mass density of the universe is above the critical density, then the Universe would reach a maximum size and then begin to collapse. It would become denser and hotter again, ending with a state that was similar to that in which it started—a Big Crunch. Alternatively, if the density in the Universe is equal to or below the critical density, the expansion would slow down, but never stop. Star formation would cease as the Universe ...
See also:Big Bang, Big Bang - History, Big Bang - Overview, Big Bang - Theoretical underpinnings, Big Bang - Observational evidence, Big Bang - Hubble's law expansion, Big Bang - Cosmic microwave background radiation, Big Bang - Abundance of primordial elements, Big Bang - Galactic evolution and distribution, Big Bang - Features issues and problems, Big Bang - Horizon problem, Big Bang - Flatness problem, Big Bang - Magnetic monopoles, Big Bang - Baryon asymmetry, Big Bang - Globular cluster age, Big Bang - Dark matter, Big Bang - Dark energy, Big Bang - The future according to the Big Bang theory, Big Bang - Speculative physics beyond the Big Bang, Big Bang - Philosophical and religious interpretations Read more here: » Big Bang: Encyclopedia II - Big Bang - The future according to the Big Bang theory |
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| | | | | baryogenesis: Encyclopedia II - Big Bang - Speculative physics beyond the Big Bang While the Big Bang model is well established in cosmology, it is likely to be refined in the future. Little is known about the earliest Universe, when inflation is hypothesized to have occurred. There may also be parts of the Universe well beyond what can be observed in principle. In the case of inflation this is required: exponential expansion has pushed large regions of space beyond our observable horizon. It may be possible to deduce what happened when we better understand physics at very high energy scales. Sp ...
See also:Big Bang, Big Bang - History, Big Bang - Overview, Big Bang - Theoretical underpinnings, Big Bang - Observational evidence, Big Bang - Hubble's law expansion, Big Bang - Cosmic microwave background radiation, Big Bang - Abundance of primordial elements, Big Bang - Galactic evolution and distribution, Big Bang - Features issues and problems, Big Bang - Horizon problem, Big Bang - Flatness problem, Big Bang - Magnetic monopoles, Big Bang - Baryon asymmetry, Big Bang - Globular cluster age, Big Bang - Dark matter, Big Bang - Dark energy, Big Bang - The future according to the Big Bang theory, Big Bang - Speculative physics beyond the Big Bang, Big Bang - Philosophical and religious interpretations Read more here: » Big Bang: Encyclopedia II - Big Bang - Speculative physics beyond the Big Bang |
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