Slides of 5 lectures at XV Brazilian School on Cosmology and ...
Slides of 5 lectures at XV Brazilian School on Cosmology and ...
Slides of 5 lectures at XV Brazilian School on Cosmology and ...
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Best fit parametersHubble c<strong>on</strong>stant H 0+ ∆H 0= 61.7 +1.2−1.1 km/s/Mpcpresent void volume fracti<strong>on</strong> f v0 = 0.76 +0.12−0.09bare density parameter ¯Ω M0= 0.125 +0.060−0.069dressed density parameter Ω M0= 0.33 +0.11−0.16n<strong>on</strong>–bary<strong>on</strong>ic dark m<str<strong>on</strong>g>at</str<strong>on</strong>g>ter / bary<strong>on</strong>ic m<str<strong>on</strong>g>at</str<strong>on</strong>g>ter mass r<str<strong>on</strong>g>at</str<strong>on</strong>g>io(¯Ω M0− ¯Ω B0)/¯Ω B0= 3.1 +2.5−2.4bare Hubble c<strong>on</strong>stant ¯H 0 = 48.2 +2.0−2.4 km/s/Mpcmean lapse functi<strong>on</strong> ¯γ 0= 1.381 +0.061−0.046deceler<str<strong>on</strong>g>at</str<strong>on</strong>g>i<strong>on</strong> parameter q 0= −0.0428 +0.0120−0.0002wall age universe τ 0= 14.7 +0.7−0.5 Gyr15th <str<strong>on</strong>g>Brazilian</str<strong>on</strong>g> <str<strong>on</strong>g>School</str<strong>on</strong>g> <strong>on</strong> <strong>Cosmology</strong> <strong>and</strong> Gravit<str<strong>on</strong>g>at</str<strong>on</strong>g>i<strong>on</strong>, August 2012 – p.80/143
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