Cosmological Constraints from Moments of the Thermal Sunyaev-Zel'dovich Effect

In this paper, we explain how moments of the thermal Sunyaev-Zel'dovich (tSZ) effect can constrain both cosmological parameters and the astrophysics of the intracluster medium (ICM). As the tSZ signal is strongly non-Gaussian, higher moments of tSZ maps contain useful information. We first calc...

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Main Authors: Hill, J. Colin, Sherwin, Blake D.
Format: Text
Language:unknown
Published: arXiv 2012
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Online Access:https://dx.doi.org/10.48550/arxiv.1205.5794
https://arxiv.org/abs/1205.5794
id ftdatacite:10.48550/arxiv.1205.5794
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spelling ftdatacite:10.48550/arxiv.1205.5794 2023-05-15T18:23:00+02:00 Cosmological Constraints from Moments of the Thermal Sunyaev-Zel'dovich Effect Hill, J. Colin Sherwin, Blake D. 2012 https://dx.doi.org/10.48550/arxiv.1205.5794 https://arxiv.org/abs/1205.5794 unknown arXiv https://dx.doi.org/10.1103/physrevd.87.023527 arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ Cosmology and Nongalactic Astrophysics astro-ph.CO FOS Physical sciences article-journal Article ScholarlyArticle Text 2012 ftdatacite https://doi.org/10.48550/arxiv.1205.5794 https://doi.org/10.1103/physrevd.87.023527 2022-04-01T14:02:56Z In this paper, we explain how moments of the thermal Sunyaev-Zel'dovich (tSZ) effect can constrain both cosmological parameters and the astrophysics of the intracluster medium (ICM). As the tSZ signal is strongly non-Gaussian, higher moments of tSZ maps contain useful information. We first calculate the dependence of the tSZ moments on cosmological parameters, finding that higher moments scale more steeply with sigma_8 and are sourced by more massive galaxy clusters. Taking advantage of the different dependence of the variance and skewness on cosmological and astrophysical parameters, we construct a statistic, ||/^1.4, which cancels much of the dependence on cosmology (i.e., sigma_8) yet remains sensitive to the astrophysics of intracluster gas (in particular, to the gas fraction in low-mass clusters). Constraining the ICM astrophysics using this statistic could break the well-known degeneracy between cosmology and gas physics in tSZ measurements, allowing for tight constraints on cosmological parameters. Although detailed simulations will be needed to fully characterize the accuracy of this technique, we provide a first application to data from the Atacama Cosmology Telescope and the South Pole Telescope. We estimate that a Planck-like full-sky tSZ map could achieve a <1% constraint on sigma_8 and a 1-sigma error on the sum of the neutrino masses that is comparable to the existing lower bound from oscillation measurements. : 11 pages, 12 figures, to be submitted to Phys. Rev. D; v2: 14 pages, 16 figures, matches PRD accepted version (changes from v1 include additional calculations with primordial non-Gaussianity and a new appendix discussing the tSZ kurtosis) Text South pole DataCite Metadata Store (German National Library of Science and Technology) South Pole
institution Open Polar
collection DataCite Metadata Store (German National Library of Science and Technology)
op_collection_id ftdatacite
language unknown
topic Cosmology and Nongalactic Astrophysics astro-ph.CO
FOS Physical sciences
spellingShingle Cosmology and Nongalactic Astrophysics astro-ph.CO
FOS Physical sciences
Hill, J. Colin
Sherwin, Blake D.
Cosmological Constraints from Moments of the Thermal Sunyaev-Zel'dovich Effect
topic_facet Cosmology and Nongalactic Astrophysics astro-ph.CO
FOS Physical sciences
description In this paper, we explain how moments of the thermal Sunyaev-Zel'dovich (tSZ) effect can constrain both cosmological parameters and the astrophysics of the intracluster medium (ICM). As the tSZ signal is strongly non-Gaussian, higher moments of tSZ maps contain useful information. We first calculate the dependence of the tSZ moments on cosmological parameters, finding that higher moments scale more steeply with sigma_8 and are sourced by more massive galaxy clusters. Taking advantage of the different dependence of the variance and skewness on cosmological and astrophysical parameters, we construct a statistic, ||/^1.4, which cancels much of the dependence on cosmology (i.e., sigma_8) yet remains sensitive to the astrophysics of intracluster gas (in particular, to the gas fraction in low-mass clusters). Constraining the ICM astrophysics using this statistic could break the well-known degeneracy between cosmology and gas physics in tSZ measurements, allowing for tight constraints on cosmological parameters. Although detailed simulations will be needed to fully characterize the accuracy of this technique, we provide a first application to data from the Atacama Cosmology Telescope and the South Pole Telescope. We estimate that a Planck-like full-sky tSZ map could achieve a <1% constraint on sigma_8 and a 1-sigma error on the sum of the neutrino masses that is comparable to the existing lower bound from oscillation measurements. : 11 pages, 12 figures, to be submitted to Phys. Rev. D; v2: 14 pages, 16 figures, matches PRD accepted version (changes from v1 include additional calculations with primordial non-Gaussianity and a new appendix discussing the tSZ kurtosis)
format Text
author Hill, J. Colin
Sherwin, Blake D.
author_facet Hill, J. Colin
Sherwin, Blake D.
author_sort Hill, J. Colin
title Cosmological Constraints from Moments of the Thermal Sunyaev-Zel'dovich Effect
title_short Cosmological Constraints from Moments of the Thermal Sunyaev-Zel'dovich Effect
title_full Cosmological Constraints from Moments of the Thermal Sunyaev-Zel'dovich Effect
title_fullStr Cosmological Constraints from Moments of the Thermal Sunyaev-Zel'dovich Effect
title_full_unstemmed Cosmological Constraints from Moments of the Thermal Sunyaev-Zel'dovich Effect
title_sort cosmological constraints from moments of the thermal sunyaev-zel'dovich effect
publisher arXiv
publishDate 2012
url https://dx.doi.org/10.48550/arxiv.1205.5794
https://arxiv.org/abs/1205.5794
geographic South Pole
geographic_facet South Pole
genre South pole
genre_facet South pole
op_relation https://dx.doi.org/10.1103/physrevd.87.023527
op_rights arXiv.org perpetual, non-exclusive license
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
op_doi https://doi.org/10.48550/arxiv.1205.5794
https://doi.org/10.1103/physrevd.87.023527
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