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We introduce the concept of multi-point propagators between linear cosmic fields and their nonlinear counterparts in the context of cosmological perturbation theory.
The large-scale structure of the universe
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Reconstructing the primordial spectrum of fluctuations of the universe from the observed nonlinear clustering of galaxies
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Diagrammatic Methods in Statistics and Biasing in the Large-Scale Structure of the Universe
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Nonlinear Evolution of the Bispectrum of Cosmological Perturbations
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Resumming Cosmological Perturbations via the Lagrangian Picture: One-loop Results in Real Space and in Redshift Space
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Scale Transformations, Tree-level Perturbation Theory, and the Cosmological Matter Bispectrum
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Renormalized cosmological perturbation theory
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