Published January 10, 2018 | Version v1
Presentation Open

Evidence for galaxy dynamics tracing cosmological evolution

  • 1. Sejong University

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.

Notes

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

Files

talkV1.pdf

Files (1.3 MB)

Name Size Download all
md5:a0545f358b4d79330e4323314d6800dd
1.3 MB Preview Download