Cold dark energy constraints from the abundance of galaxy clusters

Heneka, Caroline; Rapetti, David; Cataneo, Matteo; Mantz, Adam B.; Allen, Steven W.; von der Linden, Anja

doi:10.1093/mnras/stx2549

Title: Cold dark energy constraints from the abundance of galaxy clusters

Journal Article · Thu Oct 05 00:00:00 EDT 2017 · Monthly Notices of the Royal Astronomical Society

DOI:https://doi.org/10.1093/mnras/stx2549· OSTI ID:1425665

Heneka, Caroline ^[1]; Rapetti, David ^[2]; Cataneo, Matteo ^[3]; Mantz, Adam B. ^[4]; Allen, Steven W. ^[5]; von der Linden, Anja ^[6]

Univ. of Copenhagen (Denmark). The Niels Bohr Inst., Dark Cosmology Center; Univ. of California, Irvine, CA (United States). Dept. of Physics and Astronomy; Ruprecht-Karls-Univ. Heidelberg, Heidelberg (Germany)
Univ. of Copenhagen (Denmark). The Niels Bohr Inst., Dark Cosmology Center; Ludwig Maximilian Univ., Munich (Germany). Faculty of Physics; Excellence Cluster Universe, Garching (Germany); Univ. of Colorado, Boulder, CO (United States). Center for Astrophysics and Space Astronomy, Dept. of Astrophysical and Planetary Science; NASA Ames Research Center (ARC), Moffett Field, Mountain View, CA (United States)
Univ. of Copenhagen (Denmark). The Niels Bohr Inst., Dark Cosmology Center; Univ. of Edinburgh, Scotland (United Kingdom). Inst. for Astronomy
Stanford Univ., CA (United States). Kavli Inst. for Particle Astrophysics and Cosmology; Stanford Univ., CA (United States). Dept. of Physics
Stanford Univ., CA (United States). Kavli Inst. for Particle Astrophysics and Cosmology; Stanford Univ., CA (United States). Dept. of Physics; SLAC National Accelerator Lab., Menlo Park, CA (United States)
Univ. of Copenhagen (Denmark). The Niels Bohr Inst., Dark Cosmology Center; Stanford Univ., CA (United States). Kavli Inst. for Particle Astrophysics and Cosmology; Stanford Univ., CA (United States). Dept. of Physics; Stony Brook Univ., NY (United States). Dept. of Physics and Astronomy

We constrain cold dark energy of negligible sound speed using galaxy cluster abundance observations. In contrast to standard quasi-homogeneous dark energy, negligible sound speed implies clustering of the dark energy fluid at all scales, allowing us to measure the effects of dark energy perturbations at cluster scales. We compare those models and set the stage for using non-linear information from semi-analytical modelling in cluster growth data analyses. For this, we recalibrate the halo mass function with non-linear characteristic quantities, the spherical collapse threshold and virial overdensity, that account for model and redshift-dependent behaviours, as well as an additional mass contribution for cold dark energy. Here in this paper, we present the first constraints from this cold dark matter plus cold dark energy mass function using our cluster abundance likelihood, which self-consistently accounts for selection effects, covariances and systematic uncertainties. We combine cluster growth data with cosmic microwave background, supernovae Ia and baryon acoustic oscillation data, and find a shift between cold versus quasi-homogeneous dark energy of up to 1σ. We make a Fisher matrix forecast of constraints attainable with cluster growth data from the ongoing Dark Energy Survey (DES). For DES, we predict ~ 50 percent tighter constraints on (Ωm, w) for cold dark energy versus wCDM models, with the same free parameters. Overall, we show that cluster abundance analyses are sensitive to cold dark energy, an alternative, viable model that should be routinely investigated alongside the standard dark energy scenario.

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Research Organization:: SLAC National Accelerator Laboratory (SLAC), Menlo Park, CA (United States)

Sponsoring Organization:: USDOE; European Research Council (ERC); National Aeronautics and Space Administration (NASA)

Grant/Contract Number:: AC02-76SF00515; NNX15AE12G; 647112

OSTI ID:: 1425665

Journal Information:: Monthly Notices of the Royal Astronomical Society, Vol. 473, Issue 3; ISSN 0035-8711

Publisher:: Royal Astronomical SocietyCopyright Statement

Country of Publication:: United States

Language:: English

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Cited by: 12 works

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Effective gravitational couplings for cosmological perturbations in the most general scalar–tensor theories with second-order field equations De Felice, Antonio; Kobayashi, Tsutomu; Tsujikawa, Shinji Physics Letters B, Vol. 706, Issue 2-3 https://doi.org/10.1016/j.physletb.2011.11.028	journal	December 2011
Spherical collapse in Galileon gravity: fifth force solutions, halo mass function and halo bias Barreira, Alexandre; Li, Baojiu; Baugh, Carlton M. Journal of Cosmology and Astroparticle Physics, Vol. 2013, Issue 11 https://doi.org/10.1088/1475-7516/2013/11/056	journal	November 2013
The signature of dark energy perturbations in galaxy cluster surveys Abramo, L. R.; Batista, R. C.; Rosenfeld, R. Journal of Cosmology and Astroparticle Physics, Vol. 2009, Issue 07 https://doi.org/10.1088/1475-7516/2009/07/040	journal	July 2009

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Variable sound speed in interacting dark energy models Linton, Mark S.; Pourtsidou, Alkistis; Crittenden, Robert Journal of Cosmology and Astroparticle Physics, Vol. 2018, Issue 04 https://doi.org/10.1088/1475-7516/2018/04/043	journal	April 2018
General modified gravity with 21cm intensity mapping: simulations and forecast Heneka, C.; Amendola, L. Journal of Cosmology and Astroparticle Physics, Vol. 2018, Issue 10 https://doi.org/10.1088/1475-7516/2018/10/004	journal	October 2018
New generic evolution for $k$ -essence dark energy with $w \approx - 1$ Kehayias, John; Scherrer, Robert J. Physical Review D, Vol. 100, Issue 2 https://doi.org/10.1103/physrevd.100.023525	journal	July 2019
Skewness of matter distribution in clustering dark energy cosmologies Velten, Hermano; Fazolo, Raquel Emy Physical Review D, Vol. 101, Issue 2 https://doi.org/10.1103/physrevd.101.023518	journal	January 2020
Variable sound speed in interacting dark energy models Linton, Mark S.; Pourtsidou, Alkistis; Crittenden, Robert arXiv https://doi.org/10.48550/arxiv.1711.05196	text	January 2017
The progeny of a Cosmic Titan: a massive multi-component proto-supercluster in formation at z=2.45 in VUDS Cucciati, O.; Lemaux, B. C.; Zamorani, G. arXiv https://doi.org/10.48550/arxiv.1806.06073	text	January 2018
Skewness of matter distribution in clustering dark energy cosmologies Velten, Hermano; Fazolo, Raquel Emy arXiv https://doi.org/10.48550/arxiv.1912.00094	text	January 2019

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