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Cited by 138Cosmology and Gravitation TheoriesGalaxies: Formation, Evolution, PhenomenaDark Matter and Cosmic Phenomena

The DOI matches its Crossref record; 278 of the 278 references it cites were found in a registry or an index.

The galaxy power spectrum take on spatial curvature and cosmic concordance

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Vagnozzi, Sunny, Di Valentino, Eleonora, Gariazzo, Stefano, Melchiorri, Alessandro, Mena, Olga, Silk, Joseph·2021·Physics of the Dark Universe
DOI 10.1016/j.dark.2021.100851
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Research works printed but not linked: 11

  1. Starobinsky, 1987, A new type of isotropic cosmological models without singularity, Adv. Ser. Astrophys. Cosmol., 3, 130
  2. Sato, 1987, Cosmological baryon number domain structure and the first order phase transition of a vacuum, Adv. Ser. Astrophys. Cosmol., 3, 134
  3. Linde, 1987, A new inflationary universe scenario: A possible solution of the horizon, flatness, homogeneity, isotropy and primordial monopole problems, Adv. Ser. Astrophys. Cosmol., 3, 149
  4. Mao, 2008, How accurately can 21 cm tomography constrain cosmology?, Phys. Rev., D78
  5. Di Valentino, 2017, Can interacting dark energy solve the H0 tension?, Phys. Rev. D, 96
  6. Vagnozzi, 2018, Constraints on the sum of the neutrino masses in dynamical dark energy models with w(z)≥−1 are tighter than those obtained in ΛCDM, Phys. Rev., D98
  7. Yang, 2019, Dawn of the dark: unified dark sectors and the EDGES Cosmic Dawn 21-cm signal, J. Cosmol. Astropart. Phys., 1911, 044
  8. Anchordoqui, 2020, H0 Tension and the String Swampland, Phys. Rev., D101
  9. D’Agostino, 2020, Measurements of H0 in modified gravity theories: The role of lensed quasars in the late-time universe, Phys. Rev., D101
  10. Reid, 2010, Cosmological constraints from the clustering of the sloan digital sky survey DR7 luminous red galaxies, Mon. Not. R. Astron. Soc., 404, 60
  11. Garcia-Quintero, 2019, Cosmological discordances. III. More on measure properties, large-scale-structure constraints, the Hubble constant and Planck data, Phys. Rev., D100

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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
ORCID
Venue
Physics of the Dark Universe
Publisher
Elsevier BV
Published
2021-09
Volume
33
Pages
100851
ISSN
2212-6864 (ISSN-L)
DOI
10.1016/j.dark.2021.100851
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
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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