Dataset Open Access

Data publication: Mass density vs. energy density at cosmological scales

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


DataCite XML Export

<?xml version='1.0' encoding='utf-8'?>
<resource xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns="http://datacite.org/schema/kernel-4" xsi:schemaLocation="http://datacite.org/schema/kernel-4 http://schema.datacite.org/meta/kernel-4.1/metadata.xsd">
  <identifier identifierType="DOI">10.14278/rodare.2469</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: Mass density vs. energy density at cosmological scales</title>
  </titles>
  <publisher>Rodare</publisher>
  <publicationYear>2023</publicationYear>
  <subjects>
    <subject>N-body simulations</subject>
    <subject>large-scale structure</subject>
    <subject>inhomogeneous Universe</subject>
    <subject>cosmological perturbations</subject>
    <subject>power spectrum</subject>
    <subject>cosmic screening</subject>
  </subjects>
  <dates>
    <date dateType="Issued">2023-09-05</date>
  </dates>
  <resourceType resourceTypeGeneral="Dataset"/>
  <alternateIdentifiers>
    <alternateIdentifier alternateIdentifierType="url">https://rodare.hzdr.de/record/2469</alternateIdentifier>
  </alternateIdentifiers>
  <relatedIdentifiers>
    <relatedIdentifier relatedIdentifierType="URL" relationType="IsIdenticalTo">https://www.hzdr.de/publications/Publ-37511</relatedIdentifier>
    <relatedIdentifier relatedIdentifierType="URL" relationType="IsReferencedBy">https://www.hzdr.de/publications/Publ-37510</relatedIdentifier>
    <relatedIdentifier relatedIdentifierType="DOI" relationType="IsVersionOf">10.14278/rodare.2468</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 matter power spectra at four redshifts (z=80,50,15,0) generated by simulating Lambda-Cold Dark Matter cosmology with respect to two distinct weak-field expansion schemes (one relevant to the energy density and the other relevant to the mass density of matter) as described in the associated paper. Additionally, it contains the power spectrum of the gravitational potential at the same redshift values, based on the expansion scheme of the screening approach only.&lt;/p&gt;</description>
  </descriptions>
</resource>
128
10
views
downloads
All versions This version
Views 128128
Downloads 1010
Data volume 34.3 MB34.3 MB
Unique views 109109
Unique downloads 99

Share

Cite as