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Article
Report number arXiv:1906.08697 ; CERN-TH-2019-091 ; INR-TH-2019-012 ; TTK-19-22
Title Time-sliced perturbation theory with primordial non-Gaussianity and effects of large bulk flows on inflationary oscillating features
Author(s) Vasudevan, Anagha (Bohr Inst.) ; Ivanov, Mikhail M. (New York U., CCPP ; Moscow, INR) ; Sibiryakov, Sergey (Moscow, INR ; EPFL, Lausanne, LPPC ; CERN) ; Lesgourgues, Julien (RWTH Aachen U.)
Publication 2019-09-19
Imprint 2019-06-20
Number of pages 40
Note 39 pages, 7 figures, minor revision, published version
In: JCAP 1909 (2019) 037
DOI 10.1088/1475-7516/2019/09/037 (publication)
Subject category hep-th ; Particle Physics - Theory ; hep-ph ; Particle Physics - Phenomenology ; astro-ph.CO ; Astrophysics and Astronomy
Abstract We extend the formalism of time-sliced perturbation theory (TSPT) for cosmological large-scale structure to include non-Gaussian initial conditions. We show that in such a case the TSPT interaction vertices acquire new contributions whose time-dependence factorizes for the Einstein-de Sitter cosmology. The new formulation is free from spurious infrared (IR) enhancements and reveals a clear IR structure of non-Gaussian vertices. We use the new technique to study the evolution of oscillating features in primordial statistics and show that they are damped due to non-linear effects of large bulk flows. We derive the damping factors for the oscillating primordial power spectrum and bispectrum by means of a systematic IR resummation of relevant Feynman diagrams.
Copyright/License preprint: (License: arXiv nonexclusive-distrib 1.0)



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