How Well Do We Know the Scalar-Induced Gravitational Waves?

Fuente: arXiv
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Autores principales: Iovino, A. J., Matarrese, S., Perna, G., Ricciardone, A., Riotto, A.
Formato: Preprint
Publicado: 2024
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author Iovino, A. J.
Matarrese, S.
Perna, G.
Ricciardone, A.
Riotto, A.
author_facet Iovino, A. J.
Matarrese, S.
Perna, G.
Ricciardone, A.
Riotto, A.
contents Gravitational waves sourced by amplified scalar perturbations are a common prediction across a wide range of cosmological models. These scalar curvature fluctuations are inherently nonlinear and typically non-Gaussian. We argue that the effects of non-Gaussianity may not always be adequately captured by an expansion around a Gaussian field, expressed through nonlinear parameters such as $f_{\rm{NL}}$. As a consequence, the resulting amplitude of the stochastic gravitational wave background may differ significantly from predictions based on the standard quadratic source model routinely used in the literature.
format Preprint
id arxiv_https___arxiv_org_abs_2412_06764
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle How Well Do We Know the Scalar-Induced Gravitational Waves?
Iovino, A. J.
Matarrese, S.
Perna, G.
Ricciardone, A.
Riotto, A.
Cosmology and Nongalactic Astrophysics
General Relativity and Quantum Cosmology
High Energy Physics - Phenomenology
Gravitational waves sourced by amplified scalar perturbations are a common prediction across a wide range of cosmological models. These scalar curvature fluctuations are inherently nonlinear and typically non-Gaussian. We argue that the effects of non-Gaussianity may not always be adequately captured by an expansion around a Gaussian field, expressed through nonlinear parameters such as $f_{\rm{NL}}$. As a consequence, the resulting amplitude of the stochastic gravitational wave background may differ significantly from predictions based on the standard quadratic source model routinely used in the literature.
title How Well Do We Know the Scalar-Induced Gravitational Waves?
topic Cosmology and Nongalactic Astrophysics
General Relativity and Quantum Cosmology
High Energy Physics - Phenomenology
url https://arxiv.org/abs/2412.06764