January 30, 2024 Dataset Open Access

Eingorn, Maxim; Yilmaz, Ezgi; Yukselci, A. Emrah; Zhuk, Oleksandr

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{
  "@type": "Dataset", 
  "identifier": "https://doi.org/10.14278/rodare.2712", 
  "keywords": [
    "inhomogeneous Universe", 
    "large-scale structure", 
    "cosmic screening", 
    "cosmological perturbations", 
    "N-body simulations", 
    "power spectrum"
  ], 
  "name": "Data publication: A quantitative analysis of the effect of box size in N-body simulations of the matter power spectrum", 
  "creator": [
    {
      "affiliation": "North Carolina Central University", 
      "@type": "Person", 
      "name": "Eingorn, Maxim"
    }, 
    {
      "@type": "Person", 
      "name": "Yilmaz, Ezgi", 
      "@id": "https://orcid.org/0000-0002-9453-5991"
    }, 
    {
      "affiliation": "Istanbul Technical University", 
      "@type": "Person", 
      "name": "Yukselci, A. Emrah"
    }, 
    {
      "@type": "Person", 
      "name": "Zhuk, Oleksandr"
    }
  ], 
  "url": "https://rodare.hzdr.de/record/2712", 
  "license": "https://creativecommons.org/licenses/by/4.0/legalcode", 
  "distribution": [
    {
      "fileFormat": "xlsx", 
      "contentUrl": "https://rodare.hzdr.de/api/files/974b2616-1fe1-4d61-b927-9797be6a2e2f/Power spectra data.xlsx", 
      "@type": "DataDownload"
    }
  ], 
  "datePublished": "2024-01-30", 
  "contributor": [], 
  "sameAs": [
    "https://www.hzdr.de/publications/Publ-38704"
  ], 
  "description": "<p>The dataset consists of the matter power spectra at four redshifts (z=80,50,15,0) generated by simulating Lambda-Cold Dark Matter cosmology within the cosmic screening approach as described in the associated paper. Outputs of six distinct runs are available for boxes with L= 280, 560, 1680, 4480, 5120, 5632 Mpc/h comoving sizes, each with 2 Mpc/h resolution.</p>", 
  "@context": "https://schema.org/", 
  "@id": "https://doi.org/10.14278/rodare.2712"
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