%0 Journal Article
%T Measurements of the Cosmological Parameters Ω<sub>m</sub> and <i>H</i><sub>0</sub>
%A B. Hoeneisen
%J International Journal of Astronomy and Astrophysics
%P 386-405
%@ 2161-4725
%D 2018
%I Scientific Research Publishing
%R 10.4236/ijaa.2018.84027
%X From Baryon Acoustic Oscillation measurements with Sloan Digital Sky Survey SDSS DR14 galaxies, and the acoustic horizon angle <img src=\"Edit_10e9b032-edee-4b2a-9de4-7946d86af7cb.bmp\" alt=\"\" />measured by the Planck Collaboration, we obtain <span style=\"white-space:nowrap;\">次<sub><em>m</em></sub>=0.2724㊣0.0047</span>, and <span style=\"white-space:nowrap;\"><em>h</em>+0.020<span style=\"white-space:nowrap;\">&amp;sdot;</span>﹉<em>m</em><sub><em>v</em></sub>=0.7038㊣0.0060</span>, assuming flat space and a cosmological constant. We combine this result with the 2018 Planck ※TT, TE, EE + lowE + lensing§ analysis, and update a study of <span style=\"white-space:nowrap;\">﹉<em>m</em><sub><em>v</em></sub></span> with new direct measurements of <span style=\"white-space:nowrap;\">考<sub>8</sub></span>, and obtain <span style=\"white-space:nowrap;\">﹉<em>m</em><sub><em>v</em></sub>=0.27㊣0.08</span> eV assuming three nearly degenerate neutrino eigenstates. Measurements are consistent with <span style=\"white-space:nowrap;\">次<sub>k</sub>=0</span>, and <span style=\"white-space:nowrap;\">次<sub>de</sub>(<em>a</em>)=次<sub>托</sub></span> constant.
%K Cosmological Parameters
%K Baryon Acoustic Oscillations
%K Galaxy Distributions
%K Cosmic Microwave Background
%U http://www.scirp.org/journal/PaperInformation.aspx?PaperID=89588