Equation to give the lookback time as a function of redshift

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The discussion focuses on deriving the lookback time as a function of redshift from a given equation in cosmology. The original equation presented has a typographical error, and the correct form approximates redshift as a function of time. The key to inverting the equation lies in recognizing it as a second-order approximation, where the small term is expressed as a Taylor series around z=0. Participants clarify that the inversion can be achieved by approximating the relationship accurately to second order in z. The conversation concludes with acknowledgment of the collaborative effort in resolving the confusion.
happyparticle
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Homework Statement
Inverting ##z = H_0(t_0 - t_e) + (1 + \frac{q_0}{2}H_0^2(t_0 - t_e)^2)## to give the lookback time as a function of redshift ##t_0 - t_e = H_0^{-1}[z - (1 + \frac{q_0}{2})z^2]##
Relevant Equations
##H_0## is the Hubble's constant
##q_0## is the deceleration parameter
##z## is the redshift
Hi,
I'm currently reading the introduction to cosmology second edition by Barbara Ryden and at the page 105, the author says we get ##t_0 - t_e = H_0^{-1}[z - (1 + \frac{q_0}{2})z^2]## by inverting ##z = H_0(t_0 - t_e) + (1 + \frac{q_0}{2}H_0^2(t_0 - t_e)^2)##.

However, I can't figure out how she got this result.
Any help will be appreciate.

Thank you
 
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happyparticle said:
Homework Statement: Inverting ##z = H_0(t_0 - t_e) + (1 + \frac{q_0}{2}H_0^2(t_0 - t_e)^2)## to give the lookback time as a function of redshift ##t_0 - t_e = H_0^{-1}[z - (1 + \frac{q_0}{2})z^2]##
Relevant Equations: ##H_0## is the Hubble's constant
##q_0## is the deceleration parameter
##z## is the redshift

Hi,
I'm currently reading the introduction to cosmology second edition by Barbara Ryden and at the page 105, the author says we get ##t_0 - t_e = H_0^{-1}[z - (1 + \frac{q_0}{2})z^2]## by inverting ##z = H_0(t_0 - t_e) + (1 + \frac{q_0}{2}H_0^2(t_0 - t_e)^2)##.

However, I can't figure out how she got this result.
Any help will be appreciate.

Thank you
I believe you have some typographical errors. The formula for ##z## should read $$z \approx H_0(t_0-t_e) + \left(\frac{1+q_0}{2} \right)H_0^2(t_0-t_e)^2.$$
This is an approximate expression that assumes ##H_0(t_0-t_e)## is small. So, the equation expresses ##z## to second order in ##H_0(t_0-t_e)##.

For convenience, let ##x = H_0(t_0-t_e)## and ##b = \large \frac{1+q_0}{2}##. So, we may write the relation as $$z \approx x+ bx^2$$ where ##x## is a small first-order term. When inverting this, you only need to get an approximate expression for ##x## in terms of ##z## that is accurate to second order in ##z##.

Can you see a way to do that?
 
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Likes MatinSAR, happyparticle and Delta2
I can't see it. I tried a taylor's series but I don't get the same result.

I made a mistake. I think it works with a Taylor's series around z=0.

Thank you! I would not have seen it without your help.
 
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