The kinetic Sunyaev-Zel'dovich signal from inhomogeneous reionization: a parameter space study
[ABRIDGED] Inhomogeneous reionization acts as a source of arcminute-scale anisotropies in the cosmic microwave background (CMB), the most important of which is the kinetic Sunyaev-Zel'dovich (kSZ) effect. Observational efforts with the Atacama Cosmology Telescope (ACT) and the South Pole Telesc...
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ftdatacite:10.48550/arxiv.1112.1820 2023-05-15T18:23:11+02:00 The kinetic Sunyaev-Zel'dovich signal from inhomogeneous reionization: a parameter space study Mesinger, Andrei McQuinn, Matthew Spergel, David 2011 https://dx.doi.org/10.48550/arxiv.1112.1820 https://arxiv.org/abs/1112.1820 unknown arXiv https://dx.doi.org/10.1111/j.1365-2966.2012.20713.x 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 2011 ftdatacite https://doi.org/10.48550/arxiv.1112.1820 https://doi.org/10.1111/j.1365-2966.2012.20713.x 2022-04-01T14:05:42Z [ABRIDGED] Inhomogeneous reionization acts as a source of arcminute-scale anisotropies in the cosmic microwave background (CMB), the most important of which is the kinetic Sunyaev-Zel'dovich (kSZ) effect. Observational efforts with the Atacama Cosmology Telescope (ACT) and the South Pole Telescope (SPT) are poised to detect this signal for the first time. Indeed, recent SPT measurements place a bound on the dimensionless kSZ power spectrum around a multipole of l=3000 of P_tot < 2.8 (6) micro K^2 at 95% C.L., by ignoring (allowing) correlations between the thermal Sunyaev-Zel'dovich (tSZ) effect and the cosmic infrared background (CIB). To interpret these and upcoming observations, we compute the kSZ signal from a suite of ~ 100 reionization models using the publicly available code 21cmFAST. Our physically motivated reionization models are parameterized by the ionizing efficiency of high-redshift galaxies, the minimum virial temperature of halos capable of hosting stars, and the ionizing photon mean free path. We predict the contribution of patchy reionization to be P_patchy = 1.5-3.5 micro K^2. Therefore, even when conservatively adopting a low estimate of the post-reionization signal, P_OV ~ 2 micro K^2, none of our models are consistent with the aggressive 2sigma SPT bound that does not include correlations. This implies that either: (i) the early stages of reionization occurred in a much more homogeneous manner than suggested by the stellar-driven scenarios we explore, such as would be the case if, e.g., very high energy X-rays or exotic particles contributed significantly; and/or (ii) that there is a significant correlation between the CIB and the tSZ. On the other hand, the conservative SPT bound is compatible with all of our models, and is on the boarder of constraining reionization. : 15 pages, 12 figures, MNRAS in-press Text South pole DataCite Metadata Store (German National Library of Science and Technology) South Pole |
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Cosmology and Nongalactic Astrophysics astro-ph.CO FOS Physical sciences |
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Cosmology and Nongalactic Astrophysics astro-ph.CO FOS Physical sciences Mesinger, Andrei McQuinn, Matthew Spergel, David The kinetic Sunyaev-Zel'dovich signal from inhomogeneous reionization: a parameter space study |
topic_facet |
Cosmology and Nongalactic Astrophysics astro-ph.CO FOS Physical sciences |
description |
[ABRIDGED] Inhomogeneous reionization acts as a source of arcminute-scale anisotropies in the cosmic microwave background (CMB), the most important of which is the kinetic Sunyaev-Zel'dovich (kSZ) effect. Observational efforts with the Atacama Cosmology Telescope (ACT) and the South Pole Telescope (SPT) are poised to detect this signal for the first time. Indeed, recent SPT measurements place a bound on the dimensionless kSZ power spectrum around a multipole of l=3000 of P_tot < 2.8 (6) micro K^2 at 95% C.L., by ignoring (allowing) correlations between the thermal Sunyaev-Zel'dovich (tSZ) effect and the cosmic infrared background (CIB). To interpret these and upcoming observations, we compute the kSZ signal from a suite of ~ 100 reionization models using the publicly available code 21cmFAST. Our physically motivated reionization models are parameterized by the ionizing efficiency of high-redshift galaxies, the minimum virial temperature of halos capable of hosting stars, and the ionizing photon mean free path. We predict the contribution of patchy reionization to be P_patchy = 1.5-3.5 micro K^2. Therefore, even when conservatively adopting a low estimate of the post-reionization signal, P_OV ~ 2 micro K^2, none of our models are consistent with the aggressive 2sigma SPT bound that does not include correlations. This implies that either: (i) the early stages of reionization occurred in a much more homogeneous manner than suggested by the stellar-driven scenarios we explore, such as would be the case if, e.g., very high energy X-rays or exotic particles contributed significantly; and/or (ii) that there is a significant correlation between the CIB and the tSZ. On the other hand, the conservative SPT bound is compatible with all of our models, and is on the boarder of constraining reionization. : 15 pages, 12 figures, MNRAS in-press |
format |
Text |
author |
Mesinger, Andrei McQuinn, Matthew Spergel, David |
author_facet |
Mesinger, Andrei McQuinn, Matthew Spergel, David |
author_sort |
Mesinger, Andrei |
title |
The kinetic Sunyaev-Zel'dovich signal from inhomogeneous reionization: a parameter space study |
title_short |
The kinetic Sunyaev-Zel'dovich signal from inhomogeneous reionization: a parameter space study |
title_full |
The kinetic Sunyaev-Zel'dovich signal from inhomogeneous reionization: a parameter space study |
title_fullStr |
The kinetic Sunyaev-Zel'dovich signal from inhomogeneous reionization: a parameter space study |
title_full_unstemmed |
The kinetic Sunyaev-Zel'dovich signal from inhomogeneous reionization: a parameter space study |
title_sort |
kinetic sunyaev-zel'dovich signal from inhomogeneous reionization: a parameter space study |
publisher |
arXiv |
publishDate |
2011 |
url |
https://dx.doi.org/10.48550/arxiv.1112.1820 https://arxiv.org/abs/1112.1820 |
geographic |
South Pole |
geographic_facet |
South Pole |
genre |
South pole |
genre_facet |
South pole |
op_relation |
https://dx.doi.org/10.1111/j.1365-2966.2012.20713.x |
op_rights |
arXiv.org perpetual, non-exclusive license http://arxiv.org/licenses/nonexclusive-distrib/1.0/ |
op_doi |
https://doi.org/10.48550/arxiv.1112.1820 https://doi.org/10.1111/j.1365-2966.2012.20713.x |
_version_ |
1766202718046650368 |