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Enhancing gravitational wave anisotropies with peaked scalar sources

Ema Dimastrogiovanni, Matteo Fasiello, Ameek Malhotra, Gianmassimo Tasinato Orcid Logo

Journal of Cosmology and Astroparticle Physics, Volume: 2023, Issue: 01, Start page: 018

Swansea University Author: Gianmassimo Tasinato Orcid Logo

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Abstract

Gravitational wave (GW) backgrounds of cosmological origin are expected to be nearly isotropic, with small anisotropies resembling those of the cosmic microwave background. We analyse the case of a scalar-induced GW background and clarify in the process the relation between two different approaches...

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Published in: Journal of Cosmology and Astroparticle Physics
ISSN: 1475-7516
Published: IOP Publishing 2023
Online Access: Check full text

URI: https://cronfa.swan.ac.uk/Record/cronfa62473
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Abstract: Gravitational wave (GW) backgrounds of cosmological origin are expected to be nearly isotropic, with small anisotropies resembling those of the cosmic microwave background. We analyse the case of a scalar-induced GW background and clarify in the process the relation between two different approaches to calculating GW anisotropies. We focus on GW scenarios sourced by a significantly peaked scalar spectrum, which are frequently considered in the context of primordial black holes production. We show that the resulting GW anisotropies are characterised by a distinct frequency dependence. We explore the observational consequences concentrating on a GW background enhanced in the frequency band of space-based GW detectors. We study the detectability of the signal through both cross-correlations among different space-based GW detectors, and among GW and CMB experiments.
College: Faculty of Science and Engineering
Funders: M.F. would like to acknowledge support from the “Atracción de Talento” grant 2019- T1/TIC15784, his work is partially supported by the Spanish Research Agency (Agencia Estatal de Investigación) through the Grant IFT Centro de Excelencia Severo Ochoa No CEX2020- 001007-S, funded by MCIN/AEI/10.13039/501100011033. GT is partially funded by the STFC grant ST/T000813/1
Issue: 01
Start Page: 018