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Data publication: A quantitative analysis of the effect of box size in N-body simulations of the matter power spectrum

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


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  <identifier identifierType="DOI">10.14278/rodare.2712</identifier>
  <creators>
    <creator>
      <creatorName>Eingorn, Maxim</creatorName>
      <givenName>Maxim</givenName>
      <familyName>Eingorn</familyName>
      <affiliation>North Carolina Central University</affiliation>
    </creator>
    <creator>
      <creatorName>Yilmaz, Ezgi</creatorName>
      <givenName>Ezgi</givenName>
      <familyName>Yilmaz</familyName>
      <nameIdentifier nameIdentifierScheme="ORCID" schemeURI="http://orcid.org/">0000-0002-9453-5991</nameIdentifier>
    </creator>
    <creator>
      <creatorName>Yukselci, A. Emrah</creatorName>
      <givenName>A. Emrah</givenName>
      <familyName>Yukselci</familyName>
      <affiliation>Istanbul Technical University</affiliation>
    </creator>
    <creator>
      <creatorName>Zhuk, Oleksandr</creatorName>
      <givenName>Oleksandr</givenName>
      <familyName>Zhuk</familyName>
    </creator>
  </creators>
  <titles>
    <title>Data publication: A quantitative analysis of the effect of box size in N-body simulations of the matter power spectrum</title>
  </titles>
  <publisher>Rodare</publisher>
  <publicationYear>2024</publicationYear>
  <subjects>
    <subject>inhomogeneous Universe</subject>
    <subject>large-scale structure</subject>
    <subject>cosmic screening</subject>
    <subject>cosmological perturbations</subject>
    <subject>N-body simulations</subject>
    <subject>power spectrum</subject>
  </subjects>
  <dates>
    <date dateType="Issued">2024-01-30</date>
  </dates>
  <resourceType resourceTypeGeneral="Dataset"/>
  <alternateIdentifiers>
    <alternateIdentifier alternateIdentifierType="url">https://rodare.hzdr.de/record/2712</alternateIdentifier>
  </alternateIdentifiers>
  <relatedIdentifiers>
    <relatedIdentifier relatedIdentifierType="URL" relationType="IsIdenticalTo">https://www.hzdr.de/publications/Publ-38704</relatedIdentifier>
    <relatedIdentifier relatedIdentifierType="URL" relationType="IsReferencedBy">https://www.hzdr.de/publications/Publ-38697</relatedIdentifier>
    <relatedIdentifier relatedIdentifierType="DOI" relationType="IsVersionOf">10.14278/rodare.2711</relatedIdentifier>
    <relatedIdentifier relatedIdentifierType="URL" relationType="IsPartOf">https://rodare.hzdr.de/communities/rodare</relatedIdentifier>
  </relatedIdentifiers>
  <rightsList>
    <rights rightsURI="https://creativecommons.org/licenses/by/4.0/legalcode">Creative Commons Attribution 4.0 International</rights>
    <rights rightsURI="info:eu-repo/semantics/openAccess">Open Access</rights>
  </rightsList>
  <descriptions>
    <description descriptionType="Abstract">&lt;p&gt;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.&lt;/p&gt;</description>
  </descriptions>
</resource>
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