Cosmological constraints from the EFT power spectrum and tree-level bispectrum of 21cm intensity maps

Fuente: arXiv
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Autori principali: Randrianjanahary, Liantsoa F., Karagiannis, Dionysios, Maartens, Roy
Natura: Preprint
Pubblicazione: 2023
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author Randrianjanahary, Liantsoa F.
Karagiannis, Dionysios
Maartens, Roy
author_facet Randrianjanahary, Liantsoa F.
Karagiannis, Dionysios
Maartens, Roy
contents We explore the information content of 21cm intensity maps in redshift space using the 1-loop Effective Field Theory power spectrum model and the bispectrum at tree level. The 21cm signal contains signatures of dark matter, dark energy and the growth of large-scale structure in the Universe. These signatures are typically analyzed via the 2-point correlation function or power spectrum. However, adding the information from the 3-point correlation function or bispectrum will be crucial to exploiting next-generation intensity mapping experiments. The bispectrum could offer a unique opportunity to break key parameter degeneracies that hinder the measurement of cosmological parameters and improve on the precision. We use a Fisher forecast analysis to estimate the constraining power of the HIRAX survey on cosmological parameters, dark energy and modified gravity.
format Preprint
id arxiv_https___arxiv_org_abs_2312_02511
institution arXiv
publishDate 2023
record_format arxiv
spellingShingle Cosmological constraints from the EFT power spectrum and tree-level bispectrum of 21cm intensity maps
Randrianjanahary, Liantsoa F.
Karagiannis, Dionysios
Maartens, Roy
Cosmology and Nongalactic Astrophysics
General Relativity and Quantum Cosmology
We explore the information content of 21cm intensity maps in redshift space using the 1-loop Effective Field Theory power spectrum model and the bispectrum at tree level. The 21cm signal contains signatures of dark matter, dark energy and the growth of large-scale structure in the Universe. These signatures are typically analyzed via the 2-point correlation function or power spectrum. However, adding the information from the 3-point correlation function or bispectrum will be crucial to exploiting next-generation intensity mapping experiments. The bispectrum could offer a unique opportunity to break key parameter degeneracies that hinder the measurement of cosmological parameters and improve on the precision. We use a Fisher forecast analysis to estimate the constraining power of the HIRAX survey on cosmological parameters, dark energy and modified gravity.
title Cosmological constraints from the EFT power spectrum and tree-level bispectrum of 21cm intensity maps
topic Cosmology and Nongalactic Astrophysics
General Relativity and Quantum Cosmology
url https://arxiv.org/abs/2312.02511