jacdiam89
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Homework Statement
Calculate the comobile distance of a galaxy with z=7.3, H_{0}=72 km/s/Mpc, universe with \Omega_{0}=\Omega_{0,m}=1
Calculate the scale factor when the galaxy emitted the light we receive today.
Homework Equations
Friedmann equation
(\frac{\dot{a}}{a})^{2}=(H_{0})^{2}[ \Omega_{0,r}(\frac{a}{a_{0}})^{-4}+\Omega_{0,m}(\frac{a}{a_{0}})^{-3}+(1-\Omega_{0})(\frac{a}{a_{0}})^{2}+\Omega_{\Lambda}]
The Attempt at a Solution
With this model of universe Friedmann equation becomes:
(\frac{\dot{a}}{a})^{2}=(H_{0})^{2}[\Omega_{0,m}(\frac{a}{a_{0}})^{-3}]
so
(\frac{\dot{a}}{a})=(H_{0})(\frac{a}{a_{0}})^{-3/2}
I should use the equation:
X=\int^{t 0}_{t em}\frac{cdt}{a\dot{a}}
X= comobile distance
..but i don't know how to put the scale factor into it.