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More out of less: an excess integrated Sachs–Wolfe signal from supervoids mapped out by the Dark Energy Survey

More out of less: an excess integrated Sachs–Wolfe signal from supervoids mapped out by the Dark Energy Survey
More out of less: an excess integrated Sachs–Wolfe signal from supervoids mapped out by the Dark Energy Survey
The largest structures in the cosmic web probe the dynamical nature of dark energy through their integrated Sachs–Wolfe imprints. In the strength of the signal, typical cosmic voids have shown good consistency with expectation AISW = ΔTdataTtheory = 1, given the substantial cosmic variance. Discordantly, large-scale hills in the gravitational potential, or supervoids, have shown excess signals. In this study, we mapped out 87 new supervoids in the total 5000 deg2 footprint of the Dark Energy Survey at 0.2 < z < 0.9 to probe these anomalous claims. We found an excess imprinted profile with AISW ≈ 4.1 ± 2.0 amplitude. The combination with independent BOSS data reveals an ISW imprint of supervoids at the 3.3σ significance level with an enhanced AISW ≈ 5.2 ± 1.6 amplitude. The tension with ΛCDM predictions is equivalent to 2.6σ and remains unexplained.
1365-2966
5267-5277
Smith, Mathew
8bdc74e1-a37b-434d-ae75-82763109bf7a
DES Collaboration
Smith, Mathew
8bdc74e1-a37b-434d-ae75-82763109bf7a

Smith, Mathew , DES Collaboration (2019) More out of less: an excess integrated Sachs–Wolfe signal from supervoids mapped out by the Dark Energy Survey. Monthly Notices of the Royal Astronomical Society, 484 (4), 5267-5277. (doi:10.1093/mnras/stz341).

Record type: Article

Abstract

The largest structures in the cosmic web probe the dynamical nature of dark energy through their integrated Sachs–Wolfe imprints. In the strength of the signal, typical cosmic voids have shown good consistency with expectation AISW = ΔTdataTtheory = 1, given the substantial cosmic variance. Discordantly, large-scale hills in the gravitational potential, or supervoids, have shown excess signals. In this study, we mapped out 87 new supervoids in the total 5000 deg2 footprint of the Dark Energy Survey at 0.2 < z < 0.9 to probe these anomalous claims. We found an excess imprinted profile with AISW ≈ 4.1 ± 2.0 amplitude. The combination with independent BOSS data reveals an ISW imprint of supervoids at the 3.3σ significance level with an enhanced AISW ≈ 5.2 ± 1.6 amplitude. The tension with ΛCDM predictions is equivalent to 2.6σ and remains unexplained.

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More information

Accepted/In Press date: 22 January 2019
e-pub ahead of print date: 6 February 2019
Published date: April 2019

Identifiers

Local EPrints ID: 430781
URI: http://eprints.soton.ac.uk/id/eprint/430781
ISSN: 1365-2966
PURE UUID: 7a13848d-ff43-4e8a-845a-190f65bb69d0
ORCID for Mathew Smith: ORCID iD orcid.org/0000-0002-3321-1432

Catalogue record

Date deposited: 10 May 2019 16:30
Last modified: 16 Mar 2024 04:19

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Contributors

Author: Mathew Smith ORCID iD
Corporate Author: DES Collaboration

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