Presentation Open Access
van Putten, Maurice
<?xml version='1.0' encoding='utf-8'?> <oai_dc:dc xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/ http://www.openarchives.org/OAI/2.0/oai_dc.xsd"> <dc:creator>van Putten, Maurice</dc:creator> <dc:date>2018-01-10</dc:date> <dc:description>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.</dc:description> <dc:identifier>https://zenodo.org/record/1144113</dc:identifier> <dc:identifier>10.5281/zenodo.1144113</dc:identifier> <dc:identifier>oai:zenodo.org:1144113</dc:identifier> <dc:relation>doi:10.5281/zenodo.1144112</dc:relation> <dc:rights>info:eu-repo/semantics/openAccess</dc:rights> <dc:rights>https://creativecommons.org/licenses/by/4.0/legalcode</dc:rights> <dc:title>Evidence for galaxy dynamics tracing cosmological evolution</dc:title> <dc:type>info:eu-repo/semantics/lecture</dc:type> <dc:type>presentation</dc:type> </oai_dc:dc>
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