[cosmology] Find the comobile distance of a galaxy given redshift and H0.

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.
 
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Since you know z, and since z is easily expressible in terms of the scale factor a, maybe you should use \dot{a} = da/dt to eliminate dt in
jacdiam89 said:
X=\int^{t 0}_{t em}\frac{cdt}{a\dot{a}}
 
First of all, thank you,

i did the substitution, now the integral is in da. I have problems using a_{0}. If i use the scale factor without it, the conclusions should be the same...i think! I mean, if
z_{mis}=\frac{1}{a_{em}}-1
then
a_{em} is \frac{a}{a_{0}}

...is it true?

I guess it is wrong, i think i didn't understand why the scale factor must be normalized..
 
I have had a closer look at this, and I think I have worked it out.
jacdiam89 said:
I should use the equation:

X=\int^{t 0}_{t em}\frac{cdt}{a\dot{a}}

Did you mean
\chi = \int^{a_0}_{a_{em}}\frac{cda}{a\dot{a}} ?
jacdiam89 said:
X= comobile distance

..but i don't know how to put the scale factor into it.

I don't think so. I think that \chi is the comoving coordinate and that the the comoving distance (what you are looking for) is a_0 \chi
jacdiam89 said:
First of all, thank you,

i did the substitution, now the integral is in da. I have problems using a_{0}. If i use the scale factor without it, the conclusions should be the same...i think! I mean, if
z_{mis}=\frac{1}{a_{em}}-1
then
a_{em} is \frac{a}{a_{0}}

...is it true?

I guess it is wrong

I think
z = \frac{a_0}{a_{em}} - 1
that is, you don't need to worry about the normalization.

I wrote the above in a hurry (my wife is pulling me out the door for a social engagement), so it might have some mistakes.
 
To solve this, I first used the units to work out that a= m* a/m, i.e. t=z/λ. This would allow you to determine the time duration within an interval section by section and then add this to the previous ones to obtain the age of the respective layer. However, this would require a constant thickness per year for each interval. However, since this is most likely not the case, my next consideration was that the age must be the integral of a 1/λ(z) function, which I cannot model.
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