Time-sliced perturbation theory with primordial non-Gaussianity and effects of large bulk flows on inflationary oscillating features

DOI10.1088/1475-7516/2019/09/037OpenAlexW2952109313MaRDI QIDQ5861844

Anagha Vasudevan, Julien Lesgourgues, Sergey Sibiryakov, Mikhail M. Ivanov

Publication date: 2 March 2022

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

Full work available at URL: https://arxiv.org/abs/1906.08697

zbMATH Keywords

inflationpower spectrumcosmic webbaryon acoustic oscillations

Mathematics Subject Classification ID

Relativity and gravitational theory (83-XX)

Related Items (3)

Non-Gaussian CMB and LSS statistics beyond polyspectra ⋮ Consistent modeling of velocity statistics and redshift-space distortions in one-loop perturbation theory ⋮ Planck residuals anomaly as a fingerprint of alternative scenarios to inflation

Uses Software

• CLASS

Cites Work

• The cosmological bootstrap: inflationary correlators from symmetries and singularities
• Large-scale structure of the universe and cosmological perturbation theory
• Non-Gaussianity as a particle detector
• Large-scale galaxy bias
• The effective field theory of cosmological large scale structures
• Symmetries and consistency relations in the large scale structure of the universe
• How Gaussian can our Universe be?

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