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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Redshift, luminosity distanceCosmological redshift (last term tracker soluti<strong>on</strong>)z + 1 = a a 0= ā0¯γā¯γ 0= (2 + f v)f v1/33f v01/3 ¯H0 t=2 4/3 t 1/3 (t + b)f v01/3 ¯H0 t(2t + 3b) 4/3 ,where b = 2(1 − f v0 )(2 + f v0 )/[9f v0 ¯H0 ]Dressed luminosity distance rel<str<strong>on</strong>g>at</str<strong>on</strong>g>i<strong>on</strong> d L= (1 + z)Dwhere the effective comoving distance to a redshift z isD = a 0r w , withr w = ¯γ (1 − f v ) 1/3 ∫ t0tdt ′¯γ(t ′ )(1 − f v (t ′ )) 1/3 ā(t ′ ) .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.68/143