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Evidence for galaxy dynamics tracing cosmological evolution

van Putten, Maurice

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  <identifier identifierType="DOI">10.5281/zenodo.1144113</identifier>
      <creatorName>van Putten, Maurice</creatorName>
      <familyName>van Putten</familyName>
      <affiliation>Sejong University</affiliation>
    <title>Evidence for galaxy dynamics tracing cosmological evolution</title>
    <date dateType="Issued">2018-01-10</date>
  <resourceType resourceTypeGeneral="Text">Presentation</resourceType>
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    <relatedIdentifier relatedIdentifierType="DOI" relationType="IsVersionOf">10.5281/zenodo.1144112</relatedIdentifier>
    <rights rightsURI="">Creative Commons Attribution 4.0 International</rights>
    <rights rightsURI="info:eu-repo/semantics/openAccess">Open Access</rights>
    <description descriptionType="Abstract">&lt;p&gt;We identify C0 galaxy dynamics in data of Lellie et al. (2016) and Genzel et al. (2017) normalized to the de Sitter scale of acceleration adS=cH covering redshifts up to abou two. It shows dynamics tracing cosmological evolution governed by Lambda = omega_0^2 derived from the eigenfrequency omega_0 = sqrt(1-q)H of the cosmological horizon with Hubble parameter H and deceleration parameter q, derived from the Gauss-Bonnet theorem. An exact solution H(z) is presented, representing evanescent dark energy and dark matter from entanglement across the cosmological horizon.&lt;/p&gt;</description>
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