Published April 27, 2018
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Tension-free H0 from evanescent dark energy
Description
A tension free estimate of H0~74 km/s/Mpc is derived from cosmological data H(z) based on a stress-energy tensor of the cosmological vacuum induced by thermodynamic properties of the cosmological horizon, that defines the phase space of FRW-cosmologies analogous to black hole spacetimes. Included is a discussion on self-similar galaxy dynamics and apparent dark matter therein in light of recent data from Lellie et al. (2016), Genzel et al. (2017) and galaxy models in LambdaCDM in MUGS2.
Notes
Preferred citation: Evidence for Galaxy Dynamics Tracing Background Cosmology Below the de Sitter Scale of Acceleration, 2017, van Putten, M.H.P.M. van Putten, ApJ, 848, 28, DOI 10.3847/1538-4357/aa88cc
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References
- van Putten, M.H.P.M., 2018, arXiv:1804.06212; 2018, ApJ 848 28