van Putten, Maurice
2018-01-10
<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>
Preferred citation: Self-similar galaxy dynamics below the de Sitter scale of acceleration, 2018,
van Putten, M.H.P.M., MNRAS, 481, L26, https://doi.org/10.1093/mnrasl/sly149
https://doi.org/10.5281/zenodo.1144113
oai:zenodo.org:1144113
Zenodo
https://doi.org/10.5281/zenodo.1144112
info:eu-repo/semantics/openAccess
Creative Commons Attribution 4.0 International
https://creativecommons.org/licenses/by/4.0/legalcode
AAS231, American Astronomical Society meeting 231, Washington DC, 8-12 January 2018
Evidence for galaxy dynamics tracing cosmological evolution
info:eu-repo/semantics/lecture