Scalar-Induced Gravitational Waves in a $\Lambda$CDM Cosmology

Abstract

We reconsider the gravitational wave spectrum induced by scalar perturbations in spatially flat Friedmann-Lemaître-Robertson-Walker spacetimes, focusing on the matter- and $\Lambda$-dominated epochs. During matter domination, sub-horizon modes are not free and a commonly applied approximation for the derivative of the tensor perturbation is flawed. We show analytically that this leads to a significant overestimation of the energy density spectrum. In addition, we demonstrate that gauge-dependent non-oscillating tensor perturbations appear in the presence of a cosmological constant. Complementing the analytical calculations, we compute the according present-day spectrum numerically for a Planck-like $\Lambda$CDM cosmology, finding that non-oscillating growing modes appear during the transition between matter and $\Lambda$ domination in conformal Newtonian gauge.

12 pages, 4 figures; v3: minor improvements, conclusions unchanged; accepted by PRD on 17 Feb 2023

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Cited by in corpus (3)

• Scalar induced gravitational waves in chiral scalar-tensor theory of gravity
• Scalar-induced gravitational waves in spatially covariant gravity
• Observable Gravitational Wave Strain at Second Order