高次のLagrange的摂動論による宇宙の大規模構造形成

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タイトル別名
  • コウジ ノ Lagrangeテキセツドウロン ニ ヨル ウチュウ ノ ダイキボ コウゾウ ケイセイ
  • Higher-order Lagrangian perturbation for structure formation in the Universe

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The structure formation in the Universe has been known as one of the most important problem in modern cosmology. The formation causes its self-gravitating instability and cosmic expansion. Therefore when we analyze the structure obtained by the observations, we would know the evolution of the Universe. We have derived fifth-order perturbative equations in Lagrangian perturbation theory for a cosmological dust fluid. These equations are derived under the supposition of Newtonian cosmology in the Friedmann-Lemaitre-Robertson-Walker Universe model. The application of the fifth-order perturbation leads to a precise prediction of the large-scale structure.

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