UCL Discovery Stage
UCL home » Library Services » Electronic resources » UCL Discovery Stage

Planck intermediate results XLVII. Planck constraints on reionization history

Adam, R; Aghanim, N; Ashdown, M; Aumont, J; Baccigalupi, C; Ballardini, M; Banday, AJ; ... Zonca, A; + view all (2016) Planck intermediate results XLVII. Planck constraints on reionization history. Astronomy & Astrophysics , 596 , Article A108. 10.1051/0004-6361/201628897. Green open access

[thumbnail of McEwen_aa28897-16.pdf]
Preview
Text
McEwen_aa28897-16.pdf

Download (1MB) | Preview

Abstract

We investigate constraints on cosmic reionization extracted from the Planck cosmic microwave background (CMB) data. We combine the Planck CMB anisotropy data in temperature with the low-multipole polarization data to fit ΛCDM models with various parameterizations of the reionization history. We obtain a Thomson optical depth τ = 0.058 ± 0.012 for the commonly adopted instantaneous reionization model. This confirms, with data solely from CMB anisotropies, the low value suggested by combining Planck 2015 results with other data sets, and also reduces the uncertainties. We reconstruct the history of the ionization fraction using either a symmetric or an asymmetric model for the transition between the neutral and ionized phases. To determine better constraints on the duration of the reionization process, we also make use of measurements of the amplitude of the kinetic Sunyaev-Zeldovich (kSZ) effect using additional information from the high-resolution Atacama Cosmology Telescope and South Pole Telescope experiments. The average redshift at which reionization occurs is found to lie between z = 7.8 and 8.8, depending on the model of reionization adopted. Using kSZ constraints and a redshift-symmetric reionization model, we find an upper limit to the width of the reionization period of Δz < 2.8. In all cases, we find that the Universe is ionized at less than the 10% level at redshifts above z ≃ 10. This suggests that an early onset of reionization is strongly disfavoured by the Planck data. We show that this result also reduces the tension between CMB-based analyses and constraints from other astrophysical sources.

Type: Article
Title: Planck intermediate results XLVII. Planck constraints on reionization history
Open access status: An open access version is available from UCL Discovery
DOI: 10.1051/0004-6361/201628897
Publisher version: http://doi.org/10.1051/0004-6361/201628897
Language: English
Additional information: © ESO 2016
Keywords: Science & Technology, Physical Sciences, Astronomy & Astrophysics, cosmic background radiation, dark ages, reionization, first stars, polarization, MICROWAVE BACKGROUND ANISOTROPIES, PROBE WMAP OBSERVATIONS, STAR-FORMING GALAXIES, ANGULAR POWER SPECTRUM, HIGH-REDSHIFT GALAXIES, SOUTH-POLE TELESCOPE, DEEP FIELD CAMPAIGN, LY-ALPHA-EMITTERS, SIMILAR-TO 6, COSMIC REIONIZATION
UCL classification: UCL
UCL > Provost and Vice Provost Offices > UCL BEAMS
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Space and Climate Physics
URI: https://discovery-pp.ucl.ac.uk/id/eprint/1524172
Downloads since deposit
4,028Downloads
Download activity - last month
Download activity - last 12 months
Downloads by country - last 12 months

Archive Staff Only

View Item View Item