August 2, 2016 Software Open Access

Seery, David

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  <identifier identifierType="DOI">10.5281/zenodo.59403</identifier>
  <creators>
    <creator>
      <creatorName>Seery, David</creatorName>
      <givenName>David</givenName>
      <familyName>Seery</familyName>
      <affiliation>University of Sussex</affiliation>
    </creator>
  </creators>
  <titles>
    <title>CppTransport 2016.2</title>
  </titles>
  <publisher>Zenodo</publisher>
  <publicationYear>2016</publicationYear>
  <subjects>
    <subject>inflation</subject>
    <subject>early universe cosmology</subject>
    <subject>automated tools</subject>
  </subjects>
  <dates>
    <date dateType="Issued">2016-08-02</date>
  </dates>
  <resourceType resourceTypeGeneral="Software"/>
  <alternateIdentifiers>
    <alternateIdentifier alternateIdentifierType="url">https://zenodo.org/record/59403</alternateIdentifier>
  </alternateIdentifiers>
  <relatedIdentifiers>
    <relatedIdentifier relatedIdentifierType="DOI" relationType="IsSupplementedBy">10.5281/zenodo.59406</relatedIdentifier>
    <relatedIdentifier relatedIdentifierType="DOI" relationType="IsNewVersionOf">10.5281/zenodo.58710</relatedIdentifier>
    <relatedIdentifier relatedIdentifierType="DOI" relationType="IsVersionOf">10.5281/zenodo.639556</relatedIdentifier>
    <relatedIdentifier relatedIdentifierType="URL" relationType="IsPartOf">https://zenodo.org/communities/ecfunded</relatedIdentifier>
  </relatedIdentifiers>
  <rightsList>
    <rights rightsURI="http://www.opensource.org/licenses/GPL-2.0">GNU General Public License v2.0 only</rights>
    <rights rightsURI="info:eu-repo/semantics/openAccess">Open Access</rights>
  </rightsList>
  <descriptions>
    <description descriptionType="Abstract">&lt;p&gt;2016.2 release of the&amp;nbsp;&lt;strong&gt;CppTransport&lt;/strong&gt;&amp;nbsp;platform&amp;nbsp;for computation of correlation functions generated during an inflationary epoch in the early universe.&lt;/p&gt;

&lt;p&gt;This is a bug-fix release that addresses&amp;nbsp;a specific performance issue when integrating correlation functions with k_t exponentially different to k*. This would cause a significant slowdown and could require unnecessarily tight numerical tolerances.&lt;/p&gt;</description>
  </descriptions>
  <fundingReferences>
    <fundingReference>
      <funderName>European Commission</funderName>
      <funderIdentifier funderIdentifierType="Crossref Funder ID">10.13039/501100000780</funderIdentifier>
      <awardNumber awardURI="info:eu-repo/grantAgreement/EC/FP7/308082/">308082</awardNumber>
      <awardTitle>Precision tests of the inflationary scenario</awardTitle>
    </fundingReference>
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