Evidence for galaxy dynamics tracing cosmological evolution

Other literature type, Lecture English OPEN
van Putten, Maurice (2018)
  • Related identifiers: doi: 10.5281/zenodo.1144112, doi: 10.5281/zenodo.1144113
  • Subject: Molecular Biology | Computational Biology | galaxy dynamics | Hubble parameter H | Infectious Diseases | deceleration parameter q | Ecology | Genetics | Evolutionary Biology | Pharmacology | Physical Sciences not elsewhere classified | Chemical Sciences not elsewhere classified | Developmental Biology | Mathematical Sciences not elsewhere classified | Medicine | Gauss-Bonnet theorem | evolution | C 0 galaxy dynamics | omega | horizon | Hematology | Sitter scale | Biochemistry | Cancer
    arxiv: General Relativity and Quantum Cosmology | Astrophysics::Cosmology and Extragalactic Astrophysics

<p>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.</p>
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