Cosmological perturbation theory

id: cosmological-perturbation-theory-282-10237427
title: Cosmological perturbation theory
text: In physical cosmology, cosmological perturbation theory is the theory by which the evolution of structure is understood in the Big Bang model. Cosmological perturbation theory may be broken into two categories: Newtonian or general relativistic. Each case uses its governing equations to compute gravitational and pressure forces which cause small perturbations to grow and eventually seed the formation of stars, quasars, galaxies and clusters. Both cases apply only to situations where the universe
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category slug: encyclopedia
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original url: https://en.wikipedia.org/wiki/Cosmological_perturbation_theory
date created:
date modified: 2023-10-28T13:23:48Z
main entity: {"identifier":"Q17005905","url":"https://www.wikidata.org/entity/Q17005905"}
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integrity: 13

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