The size of local bispectrum and trispectrum in a non-minimal inflation

DOI10.1016/J.NUCLPHYSB.2018.06.018zbMath1395.83135arXiv1611.10025OpenAlexW2734655831WikidataQ125907797 ScholiaQ125907797MaRDI QIDQ1672300

Kosar Asadi, Kourosh Nozari

Publication date: 7 September 2018

Published in: Nuclear Physics. B (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1611.10025

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Model quantum field theories (81T10) Gravitational interaction in quantum theory (81V17) Methods of quantum field theory in general relativity and gravitational theory (83C47)

Related Items (1)

The minimally coupled and canonical scalar field inflationary cosmology with negative quadratic and modified Higgs-like potentials: a symmetry based approach

Cites Work

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• Asymptotic Statistics
• Evolution of second-order cosmological perturbations
• The Primordial Density Perturbation
• Inflationary universe: A possible solution to the horizon and flatness problems
• Gravitational waves from inflation on the brane

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