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The galaxy power spectrum take on spatial curvature and cosmic concordance
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“The same disagreement is evident in the independent analysis shown in Figure 1 of Ref. [89], as well as in Figure 1 of Ref. [90], which reports a similar tension with the full-shape (FS) galaxy power spectrum measurements from the BOSS DR12 CMASS sample.”
From Challenges of the Standard Cosmological Model (2022) · cites this paper as [90]
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Cites
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NINE-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE ( WMAP ) OBSERVATIONS: COSMOLOGICAL PARAMETER RESULTS
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“Our MCMC chains are generated through a suitably modified version of the cosmological sampler CosmoMC [263], to which we have included the FS likelihood.”
MethodInfluentialAlam, S., Ata, M., Bailey, S., Beutler, F., Bizyaev, D., Blazek, J. A., Bolton, A. S., Brownstein, J. R., Burden, A., Chuang, C.-H., et al. (2017) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stx721 · Cited by 3,056
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Dark Energy Survey Year 3 results: Cosmological constraints from galaxy clustering and weak lensing
Abbott, T. M. C., Aguena, M., Alarcon, A., Allam, S., Alves, O., Amon, A., Andrade-Oliveira, F., Annis, J., Avila, S., Bacon, D., et al. (2022) · Physical Review D · doi:10.1103/physrevd.105.023520 · Cited by 1,124
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Metadata
- Authors
- Vagnozzi, S., Di Valentino, E., Gariazzo, S., Melchiorri, A., Mena, O., & Silk, J.
- Affiliations
- University of Cambridge (GB)
- Consejo Superior de Investigaciones Científicas (ES)
- Sapienza University of Rome (IT)
- Centre National de la Recherche Scientifique (FR)
- Corresponding author
- Vagnozzi, Sunny
- Venue
- Physics of the Dark Universe
- Publisher
- Elsevier BV
- Published
- 2021-09
- Volume
- 33
- Pages
- 100851
- ISSN
- 2212-6864 (ISSN-L)
- OpenAlex
- W3175779977
- Cited by
- 138
- References
- 278
- Citations by year
- 2026: 10 · 2025: 24 · 2024: 30 · 2023: 28 · 2022: 31 · 2021: 15
- FWCI
- 13.97
- Type
- journal article
- Language
- en
- Open access
- green
- arxiv.org
- Licence
- Locations
- Physics of the Dark Universe (publishedVersion)
- arXiv (Cornell University) (submittedVersion)
- HAL (submittedVersion)
- Iris (University of Trento) (submittedVersion, cc-by-nc-nd)
- Institutional Research Information System University of Turin (University of Turin) (submittedVersion)
- arXiv (Cornell University)
- Funders
- Instituto Nazionale di Fisica Nucleare (H2020-MSCA-ITN-2019//860881-HIDDeN)
- University of Cambridge Homerton College
- Agencia Estatal de Investigación (FPA2017-85216-P, FPA2017-85985-P)
- Durham University Institute of Advanced Study
- Generalitat Valenciana (FPA2017-90566-REDC, PROMETEO/2019/083)
- Ministerio de Economía y Competitividad
- Foundation Blanceflor Boncompagni Ludovisi, née Bildt
- Kavli Foundation
- Isaac Newton Trust
- European Research Council (681431, IJC2018-036458-I)
- European Regional Development Fund
- H2020 Marie Skłodowska-Curie Actions (754496)
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Cosmology and Gravitation Theories
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Galaxies: Formation, Evolution, Phenomena
- Physical Sciences › Physics and Astronomy › Nuclear and High Energy Physics › Dark Matter and Cosmic Phenomena
- Keywords
- spatial curvature, baryon acoustic oscillations, BOSS, cosmological parameter constraints
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