Systematics of adiabatic modes: flat universes

DOI10.1088/1475-7516/2018/03/013OpenAlexW3102773554WikidataQ130184725 ScholiaQ130184725MaRDI QIDQ5022239

Enrico Pajer, Sadra Jazayeri

Publication date: 18 January 2022

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

Full work available at URL: https://arxiv.org/abs/1710.02177

zbMATH Keywords

inflationnon-Gaussianitycosmological perturbation theoryphysics of the early universe

Mathematics Subject Classification ID

Relativity and gravitational theory (83-XX)

Related Items (16)

From amplitudes to contact cosmological correlators ⋮ The spatial gauge-dependence of single-field inflationary bispectra ⋮ Spatial curvature at the sound horizon ⋮ On the symmetries of cosmological perturbations ⋮ Strolling along gravitational vacua ⋮ Soft theorems for boosts and other time symmetries ⋮ Inflationary cross-correlations of a non-minimal spectator and their soft limits ⋮ Infrared (in)sensitivity of relativistic effects in cosmological observable statistics ⋮ Synchronizing the consistency relation ⋮ Asymptotic symmetries and memories of gauge theories in FLRW spacetimes ⋮ Inflationary soft theorems revisited: a generalized consistency relation ⋮ Revisiting non-Gaussianity from non-attractor inflation models ⋮ Vanishing of local non-Gaussianity in canonical single field inflation ⋮ The effective theory of shift-symmetric cosmologies ⋮ Building a boostless bootstrap for the bispectrum ⋮ Anisotropic separate universe and Weinberg's adiabatic mode

Cites Work

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• Inflationary consistency conditions from a wavefunctional perspective
• Symmetries and loops in inflation
• Ward identities for scale and special conformal transformations in inflation
• Symmetries and consistency relations in the large scale structure of the universe
• Constraints from conformal symmetry on the three point scalar correlator in inflation
• Lectures on the Infrared Structure of Gravity and Gauge Theory
• Matter bounce cosmology with a generalized single field: non-Gaussianity and an extended no-go theorem
• A general proof of the conservation of the curvature perturbation

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