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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Phot<strong>on</strong> to bary<strong>on</strong> r<str<strong>on</strong>g>at</str<strong>on</strong>g>ioNumber density <str<strong>on</strong>g>of</str<strong>on</strong>g> bary<strong>on</strong>s <str<strong>on</strong>g>at</str<strong>on</strong>g> the volume average iswhere ¯γ ′ 0 ≡ 1¯H0 d¯γdtf B≡ ¯Ω B0/¯Ω M0.¯n B= 3 ¯H 2 0 ¯Ω B08πG m p= 11.2f B ¯Ω M0h 2(¯γ 0− ¯γ ′ 0 )2 m −3 ,∣t0, m p is the prot<strong>on</strong> mass,Hence the average phot<strong>on</strong> to bary<strong>on</strong> r<str<strong>on</strong>g>at</str<strong>on</strong>g>io isη Bγ= ¯n B¯n γ= 2.736 × 10−8 f B ¯ΩM0¯γ 3 0 h2(¯γ 0− ¯γ ′ 0 )2 ,as compared to η FLRW = 2.736 × 10 −8 f BΩ Mh 2 .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.85/143