What is the maximum distance and the maximum time a photon has traveled which is observed by us today at the particle horizon in the LCDM cosmological model applying general relativity?
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$\begingroup$ What do you mean by "applying GR" ? $\endgroup$ – Reign Oct 31 at 4:42
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$\begingroup$ i.e., not using Special Relativity for calculations - which anyway should be evident for evaluations of cosmological models. $\endgroup$ – Rene Kail Oct 31 at 7:03
For Particle Horizon distance you can use the
$$r = c\int_{t_e}^{t_o}\frac{dt}{a(t)}$$ But you can write this equation in terms of z and (making limits from $\infty$ to $0$) to make calculations easier.
To calculate the conformal time part you have to divide above equation by c.
$$\eta = \int_{t_e}^{t_o}\frac{dt}{a(t)}$$
Edit: So we know that $$1 + z = a(t)^{-1}$$
hence
$$\frac{dz}{dt} = \frac{dz} {da} \frac{da} {dt}$$ $$\frac{dz}{dt} = -\frac{1}{a^2} \dot{a}$$ $$dz = -\frac{H}{a}dt = -H(1+z)dt$$ $$dt = -\frac{dz}{H(1+z)}$$
Since at $t_e$ corrsponds to $z = \infty$ and $t_0 = 0$ we have
$$r = c\int_{t_e}^{t_o}\frac{dt}{a(t)} = -c\int_{\infty}^{0}\frac{dz}{H}$$
Also we know that $$H = H_0\sqrt{\Omega_r(1+z)^4 + \Omega_m(1+z)^3 + \Omega_{\Lambda}}$$
Finally
$$ r_{horizon} = -\frac{c}{H_0}\int_{\infty}^{0}\frac{dz}{\sqrt{\Omega_r(1+z)^4 + \Omega_m(1+z)^3 + \Omega_{\Lambda}}}$$
and
$$ \eta = -\frac{1}{H_0}\int_{\infty}^{0}\frac{dz}{\sqrt{\Omega_r(1+z)^4 + \Omega_m(1+z)^3 + \Omega_{\Lambda}}}$$
For $\Omega_r = 9 \times 10^{-5}$, $\Omega_m = 0.31$ and $\Omega_{\Lambda}= 0.69$
we get
$$-\int_{\infty}^{0}\frac{dz}{\sqrt{\Omega_r(1+z)^4 + \Omega_m(1+z)^3 + \Omega_{\Lambda}}} = 3.200$$
So
$$r_{horizon} = 3.2 \times c/H_0 = 3.2 \times 4408.712 Mpc = 14107.88 Mpc = 46.013 Gly$$
$$ \eta = 3.2 \times 1/H_0 = 3.2 \times 14.38Gyr = 46.016 Gyr$$
So light has traveled 46.013 Gly since the Big Bang and the corresponding conformal time would be 46.013 Gyr. This time is not the age of the universe.