October 1, 2025 Dataset Open Access

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

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{
  "title": "Data: Nonlinear Matter Power Spectrum from relativistic N-body Simulations: \u039bsCDM versus \u039bCDM", 
  "DOI": "10.14278/rodare.4499", 
  "id": "4499", 
  "language": "eng", 
  "author": [
    {
      "family": "Akarsu, \u00d6zg\u00fcr"
    }, 
    {
      "family": "Di Valentino, Eleonora"
    }, 
    {
      "family": "Vyskocil, Jiri"
    }, 
    {
      "family": "Y\u0131lmaz, Ezgi"
    }, 
    {
      "family": "Y\u00fckselci, A. Emrah"
    }, 
    {
      "family": "Zhuk, Oleksandr"
    }
  ], 
  "publisher": "Rodare", 
  "issued": {
    "date-parts": [
      [
        2025, 
        10, 
        1
      ]
    ]
  }, 
  "abstract": "<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>CDM-baryon P(k) outputs with nonlinear corrections from CLASS implementation of HMcode [3] at z=2,1, and 0 are also included in the published data, and have been used in the plots presented in the Appendix of the related manuscript.&nbsp;</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>\n\n<p>3. A. J. Mead, C. Heymans, L. Lombriser, J. A. Peacock, O. I. Steele, and H. A. Winther, Accurate halo-model matter power spectra with dark energy, massive neutrinos and modified gravitational forces, Mon. Not. Roy. Astron. Soc. 459, 1468 (2016). arXiv:1602.02154 [astro-ph.CO].</p>", 
  "type": "dataset"
}