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Timeline of the Big Bang - Structure formation | | Timeline of the Big Bang - Structure formation: Encyclopedia II - Timeline of the Big Bang - Structure formation | | Structure formation in the big bang model proceeds hierarchically, with smaller structures forming before larger ones. The first structures to form are quasars, which are thought to be bright, early active galaxies and population III stars. Before this epoch, the evolution of the universe could be understood through linear cosmological perturbation theory: that is, all structures could be understood as small deviations from a perfect homogeneous universe. This is computationally relatively easy to study. At this p ...
See also:Timeline of the Big Bang, Timeline of the Big Bang - The very early universe, Timeline of the Big Bang - The Planck epoch – 10-43 seconds, Timeline of the Big Bang - The Grand Unification Epoch – 10-33 seconds, Timeline of the Big Bang - Cosmic inflation, Timeline of the Big Bang - The early universe, Timeline of the Big Bang - The electroweak epoch – 10-12 s, Timeline of the Big Bang - The hadron epoch – 10-6 s–10-2 s, Timeline of the Big Bang - Nucleosynthesis – 1 s, Timeline of the Big Bang - Matter domination – 70000 years, Timeline of the Big Bang - Recombination – 500000 years, Timeline of the Big Bang - Dark ages, Timeline of the Big Bang - Structure formation, Timeline of the Big Bang - Reionization, Timeline of the Big Bang - Formation of stars, Timeline of the Big Bang - Formation of galaxies, Timeline of the Big Bang - Formation of groups clusters and superclusters, Timeline of the Big Bang - Formation of the solar system, Timeline of the Big Bang - Today, Timeline of the Big Bang - Ultimate fate of the universe, Timeline of the Big Bang - Heat death, Timeline of the Big Bang - Big crunch, Timeline of the Big Bang - Big rip, Timeline of the Big Bang - Vacuum metastability disaster | | | Timeline of the Big Bang, Timeline of the Big Bang - Big crunch, Timeline of the Big Bang - Big rip, Timeline of the Big Bang - Cosmic inflation, Timeline of the Big Bang - Dark ages, Timeline of the Big Bang - Formation of galaxies, Timeline of the Big Bang - Formation of groups clusters and superclusters, Timeline of the Big Bang - Formation of stars, Timeline of the Big Bang - Formation of the solar system, Timeline of the Big Bang - Heat death, Timeline of the Big Bang - Matter domination – 70000 years, Timeline of the Big Bang - Nucleosynthesis – 1 s, Timeline of the Big Bang - Recombination – 500000 years, Timeline of the Big Bang - Reionization, Timeline of the Big Bang - Structure formation, Timeline of the Big Bang - The Grand Unification Epoch – 10-33 seconds, Timeline of the Big Bang - The Planck epoch – 10-43 seconds, Timeline of the Big Bang - The early universe, Timeline of the Big Bang - The electroweak epoch – 10-12 s, Timeline of the Big Bang - The hadron epoch – 10-6 s–10-2 s, Timeline of the Big Bang - The very early universe, Timeline of the Big Bang - Today, Timeline of the Big Bang - Ultimate fate of the universe, Timeline of the Big Bang - Vacuum metastability disaster | | |
| | | Timeline of the Big Bang: Encyclopedia II - Timeline of the Big Bang - Structure formation
Timeline of the Big Bang - Structure formation
See also: Large-scale structure of the cosmos and Structure formation
Structure formation in the big bang model proceeds hierarchically, with smaller structures forming before larger ones. The first structures to form are quasars, which are thought to be bright, early active galaxies and population III stars. Before this epoch, the evolution of the universe could be understood through linear cosmological perturbation theory: that is, all structures could be understood as small deviations from a perfect homogeneous universe. This is computationally relatively easy to study. At this point non-linear structures begin to form, and the computational problem becomes much more difficult, involving, for example, N-body simulations with billions of particles.
Timeline of the Big Bang - Reionization
See also: Reionization and 21 centimeter radiation
The first quasars form from gravitational collapse. The intense radiation they emit reionizes the surrounding universe. From this point on, most of the universe is composed of plasma.
Timeline of the Big Bang - Formation of stars
See also: Star formation
Timeline of the Big Bang - Formation of galaxies
See also: Galaxy formation
Timeline of the Big Bang - Formation of groups clusters and superclusters
See also: Large-scale structure of the cosmos
Timeline of the Big Bang - Formation of the solar system
See also: Solar system
Timeline of the Big Bang - Today
Since the expansion of the universe appears to be accelerating, superclusters are likely the largest structures that will ever form in the universe. The present accelerated expansion prevents any more inflationary structures entering the horizon and prevents new gravitationally bound structures from forming.
Other related archives21 centimeter radiation, Baryogenesis, Big Bang, Big bang nucleosynthesis, Big crunch, Big rip, Cosmic inflation, Cosmic microwave background, Earth, Electroweak force, Galaxy formation, Grand unified theory, Hartle-Hawking initial state, Hawking radiation, Heat death, Higgs boson, Higgs mechanism, Large-scale structure of the cosmos, Loop quantum gravity, Quantum gravity, Quark-gluon plasma, Reionization, Sakharov conditions, Solar system, Standard Model, Star formation, String theory, Structure formation, Supersymmetry breaking, TeV, Ultimate fate of the universe, Vacuum metastability disaster, active galaxies, antibaryons, baryons, closed, clusters of galaxies, cosmic microwave background, cosmic neutrino background, cyclic model, dark energy, ekpyrotic universe, electromagnetism, electroweak force, false vacuum, flattened, gauge group, gauge interactions, general relativity, gravitational singularity, gravity, hadrons, line of neutral hydrogen, loop quantum gravity, magnetic monopoles, neutrinos, neutrons, oscillatory universe, particle accelerators, perturbation theory, phantom energy, plasma, population III stars, protons, quark-gluon plasma, quasars, scientific theory, stars, string landscape, string theory, strong nuclear force, superclusters, supersymmetry, symmetry is broken, tunnel, vacuum expectation value, weak nuclear force
 Adapted from the Wikipedia article "Structure formation", under the G.N U Free Docmentation License. Please also see http://en.wikipedia.org/wiki |
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