Divergence of perturbation theory in large scale structures

DOI10.1088/1475-7516/2018/05/039OpenAlexW3099888303WikidataQ129843755 ScholiaQ129843755MaRDI QIDQ5023762

Drian van der Woude, Enrico Pajer

Publication date: 24 January 2022

Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1710.01736

zbMATH Keywords

power spectrumcosmological perturbation theorycosmological parameters from LSScosmic flows

Mathematics Subject Classification ID

Relativity and gravitational theory (83-XX)

Related Items (5)

Evolution of dark matter velocity dispersion ⋮ Asymptotic expansions for Large Scale Structure ⋮ Non-perturbative probability distribution function for cosmological counts in cells ⋮ Structure formation beyond shell-crossing: nonperturbative expansions and late-time attractors ⋮ The effective field theory and perturbative analysis for log-density fields

Cites Work

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• Dynamics of gravitational clustering
• Impact of shell crossing and scope of perturbative approaches, in real and redshift space
• Combining perturbation theories with halo models
• Physical Foundations of Cosmology
• Using the Zeldovich dynamics to test expansion schemes
• Divergence of Perturbation Theory in Quantum Electrodynamics

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