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We make progress towards an analytical understanding of the regime of validity of perturbation theory for large scale structures and the nature of some non-perturbative corrections.
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Y. Ohta, I. Kayo, and A. Taruya, “Cosmological density distribution function from the ellipsoidal collapse model in real space,” Astrophys. J
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2013
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D. Blas, M. Garny, and T. Konstandin, “Cosmological perturbation theory at three-loop order,” JCAP
2014
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2014
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2015
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2016
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2016
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