October 1, 2025 Dataset Open Access

Akarsu, Özgür; Di Valentino, Eleonora; Vyskocil, Jiri; Yılmaz, Ezgi; Yükselci, A. Emrah; Zhuk, Oleksandr

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{
  "@type": "Dataset", 
  "datePublished": "2025-10-01", 
  "sameAs": [
    "https://www.hzdr.de/publications/Publ-41918"
  ], 
  "description": "<p>Matter power spectra presented in the associated&nbsp;paper are obtained from the datasets separately generated from N-body simulations with the relativistic code&nbsp;<em>gevolution </em>[1], and from calculations with the linear Boltzmann code CLASS [2], for matching cosmological best-fit parameters and background&nbsp;cosmologies.&nbsp;Regarding the latter element, we study two cases that are the concordance Lambda-Cold Dark Matter (&Lambda;CDM) model and a late-time modification with a sign-switching vacuum sector&nbsp;(&Lambda;sCDM), and for each model there are two best-fit parameter sets, derived from a&nbsp;<em>Planck</em>-only and a combined &quot;full&quot; dataset.&nbsp;</p>\n\n<p>P(k) (power spectra) outputs from gevolution are computed at the four redshifts z=15, 2, 1, 0 for the density contrasts of total matter (CDM, baryons, and massive neutrinos) as well as CDM-baryons (cb)-only. A detailed explanation of how the matter sector is handled in simulations is&nbsp;available in the main paper. All runs are carried out in boxes of L=2080 Mpc/h with 0.5 h/Mpc resolution.</p>\n\n<p>Power spectra based on CLASS outputs are obtained from the transfer functions of CDM and baryons, and the respective background densities at z=15, 2, 1, 0. CLASS dataset for the latter is shown only up to z=100.</p>\n\n<p>1. J. Adamek, D. Daverio, R. Durrer, and M. Kunz, gevolution: a cosmological N-body code based on General Relativity, JCAP 07, 053. arXiv:1604.06065 [astro-ph.CO].</p>\n\n<p>2. D. Blas, J. Lesgourgues, and T. Tram, The Cosmic Linear Anisotropy Solving System (CLASS) II: Approximation schemes, JCAP 07, 034. arXiv:1104.2933 [astro-ph.CO].</p>", 
  "license": "https://creativecommons.org/licenses/by/4.0/legalcode", 
  "keywords": [
    "cosmological N-body simulations", 
    "sign switching cosmological constant", 
    "matter power spectrum"
  ], 
  "distribution": [
    {
      "contentUrl": "https://rodare.hzdr.de/api/files/7de6aa89-9712-4a80-89f0-49d8316706f4/Pk outputs.xlsx", 
      "fileFormat": "xlsx", 
      "@type": "DataDownload"
    }
  ], 
  "identifier": "https://doi.org/10.14278/rodare.4020", 
  "@context": "https://schema.org/", 
  "inLanguage": {
    "alternateName": "eng", 
    "name": "English", 
    "@type": "Language"
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  "creator": [
    {
      "affiliation": "Istanbul Technical University", 
      "name": "Akarsu, \u00d6zg\u00fcr", 
      "@type": "Person"
    }, 
    {
      "affiliation": "School of Mathematical and Physical Sciences, University of Sheffield", 
      "name": "Di Valentino, Eleonora", 
      "@type": "Person"
    }, 
    {
      "@id": "https://orcid.org/0000-0001-8822-0929", 
      "affiliation": "HZDR - CASUS", 
      "name": "Vyskocil, Jiri", 
      "@type": "Person"
    }, 
    {
      "affiliation": "Deutsches Zentrum f\u00fcr Astrophysik", 
      "name": "Y\u0131lmaz, Ezgi", 
      "@type": "Person"
    }, 
    {
      "affiliation": "Istanbul Technical University", 
      "name": "Y\u00fckselci, A. Emrah", 
      "@type": "Person"
    }, 
    {
      "affiliation": "HZDR - CASUS", 
      "name": "Zhuk, Oleksandr", 
      "@type": "Person"
    }
  ], 
  "@id": "https://doi.org/10.14278/rodare.4020", 
  "name": "Data: Nonlinear Matter Power Spectrum from relativistic N-body Simulations: \u039bsCDM versus \u039bCDM", 
  "url": "https://rodare.hzdr.de/record/4020"
}