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Autores principales: Salcedo, Andrés N., Rozo, Eduardo, Wu, Hao-Yi, Cao, Shulei, Paillas, Enrique, Zhang, Hanyu, Rykoff, Eli S.
Formato: Preprint
Publicado: 2025
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Acceso en línea:https://arxiv.org/abs/2512.06701
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author Salcedo, Andrés N.
Rozo, Eduardo
Wu, Hao-Yi
Cao, Shulei
Paillas, Enrique
Zhang, Hanyu
Rykoff, Eli S.
author_facet Salcedo, Andrés N.
Rozo, Eduardo
Wu, Hao-Yi
Cao, Shulei
Paillas, Enrique
Zhang, Hanyu
Rykoff, Eli S.
contents We show that, in flat $Λ$CDM, low-redshift structure probes -- cluster abundances, 3$\times$2-point analyses, and full-shape clustering -- are mutually consistent, jointly delivering precise constraints on $σ_8$ and $Ω_{\rm m}$ that agree with geometrical datasets (CMB+BAO+SN). In $w_0w_a$CDM, adding clusters to the geometry dataset reduces the evidence for evolving dark energy while relaxing the $H_0$ tension, suggesting a $Λ$CDM evolution of the late-time Universe and a sound horizon that differs from its standard value.
format Preprint
id arxiv_https___arxiv_org_abs_2512_06701
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle What Galaxy Clusters Have to Say About Dynamical Dark Energy and $H_0$
Salcedo, Andrés N.
Rozo, Eduardo
Wu, Hao-Yi
Cao, Shulei
Paillas, Enrique
Zhang, Hanyu
Rykoff, Eli S.
Cosmology and Nongalactic Astrophysics
We show that, in flat $Λ$CDM, low-redshift structure probes -- cluster abundances, 3$\times$2-point analyses, and full-shape clustering -- are mutually consistent, jointly delivering precise constraints on $σ_8$ and $Ω_{\rm m}$ that agree with geometrical datasets (CMB+BAO+SN). In $w_0w_a$CDM, adding clusters to the geometry dataset reduces the evidence for evolving dark energy while relaxing the $H_0$ tension, suggesting a $Λ$CDM evolution of the late-time Universe and a sound horizon that differs from its standard value.
title What Galaxy Clusters Have to Say About Dynamical Dark Energy and $H_0$
topic Cosmology and Nongalactic Astrophysics
url https://arxiv.org/abs/2512.06701