hedgehug
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Redefining the scale factor from its current value of 1 to 1 at the time of the CMB emission, and from 1/(1100+1) at the time of the CMB emission to 1100+1 at the present time, shouldn't change the result of the integral for calculating the radius of the observable universe, right?
What exactly would the current integral ##\int_{0}^{t_0}cdt/a(t)## look like after this change? Integration limits must remain the same: 0 and ##t_0=13.8## billion years, and the integral must obviously remain consistent with the FLRW metric for null geodesic.
What exactly would the current integral ##\int_{0}^{t_0}cdt/a(t)## look like after this change? Integration limits must remain the same: 0 and ##t_0=13.8## billion years, and the integral must obviously remain consistent with the FLRW metric for null geodesic.