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The separate-universe approach provides an effective description of cosmological perturbations at large scales, where the universe can be described by an ensemble of independent, locally homogeneous and isotropic patches.
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F. Finelli and R. Brandenberger, On the generation of a scale invariant spectrum of adiabatic fluctuations in cosmological models with a contracting phase , Phys. Rev. D 65
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I. Khalatnikov, A.Y. Kamenshchik and A.A. Starobinsky, Comment about quasiisotropic solution of Einstein equations near cosmological singularity , Class.Quant.Grav. 19
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D.H. Lyth and D. Wands, Conserved cosmological perturbations , Phys. Rev. D 68
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G.I. Rigopoulos and E.P.S. Shellard, Separate universe approach and the evolution of nonlinear superhorizon cosmological perturbations , Phys. Rev. D 68
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D.H. Lyth and D. Wands, Conserved cosmological perturbations , Phys.Rev. D68
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G.I. Rigopoulos and E.P.S. Shellard, The separate universe approach and the evolution of nonlinear superhorizon cosmological perturbations , Phys. Rev. D68
2003
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D.H. Lyth and Y. Rodriguez, The Inflationary prediction for primordial non-Gaussianity , Phys. Rev. Lett. 95
2005
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2015
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V. Vennin and A.A. Starobinsky, Correlation Functions in Stochastic Inflation , Eur. Phys. J. C75
2015
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2015
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2016
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R. Brandenberger and P. Peter, Bouncing Cosmologies: Progress and Problems , Found. Phys. 47
2017
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2017
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2017
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2018
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2018
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H. Firouzjahi, A. Nassiri-Rad and M. Noorbala, Stochastic Ultra Slow Roll Inflation , JCAP 01
2019
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2019
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