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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Dressed “comoving distance” D(z)2H 0D(i)(ii)(iii)3.53H 0D(i)(ii)(iii)1.5112.521.50.501 2 3 4 5 6z0z110.50200 400 600 800 1000zBest-fit TS model (black line) compared to 3 sp<str<strong>on</strong>g>at</str<strong>on</strong>g>ially fl<str<strong>on</strong>g>at</str<strong>on</strong>g>ΛCDM models: (i) best–fit to WMAP5 <strong>on</strong>ly (Ω Λ = 0.75);(ii) joint WMAP5 + BAO + SneIa fit (Ω Λ = 0.72);(iii) best fl<str<strong>on</strong>g>at</str<strong>on</strong>g> fit to (Riess07) SneIa <strong>on</strong>ly (Ω Λ = 0.66).15th <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.93/143
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