Evanescent dark energy and dark matter

The cosmological distributions of dark energy and dark matter are identified with evanescent waves crossing the cosmological horizon. A detailed confrontation with cosmological data on the Hubble parameter gives $H_0=74.29\pm2.6$, consistent with Anderson & Riess (2017) and Guidorzi et al.(2017) from GW170817. This result derives from $\Lambda = \omega_0^2$ derived from the eigenfrequency $\omega_0 = \sqrt{1-q}H$, where $q$ is the deceleration parameter, based on the Gauss-Bonnet theorem. A further detailed consideration of galaxy dynamics against data from Lellie et al.(2016) and Genzel et al.(2017) points to a dark matter mass of less than $10^{-30}$eV. (Based on van Putten, 2017, ApJ, 848, 28; ApJ 837, 22.)