High School Comoving distance in cosmology

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In cosmology, the proper time between two points, such as galaxies, is often taken as zero (dΓ=0) to simplify calculations of proper distance. This approach leads to the expression for comoving distance, which is essential for understanding cosmological redshift. The derivation involves relating the comoving distance traveled by signals to the scale factor history. By comparing the time difference at emission with the time difference at reception, one can analyze the effects of cosmic expansion. This method is crucial for accurately modeling distances in an expanding universe.
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For calculating the proper distance in cosmology why is the proper time between two points (galaxy) dΓ is taken 0??
e.g dΓ2=dt2-a(t)2dr2
Taking dΓ=0 and ∫dr=∫dt/a(t)
 
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Apashanka said:
For calculating the proper distance in cosmology why is the proper time between two points (galaxy) dΓ is taken 0??
e.g dΓ2=dt2-a(t)2dr2
Taking dΓ=0 and ∫dr=∫dt/a(t)
It is not. What you have there is an expression for the comoving distance.

In the particular case you are referring to, it is part of a derivation of cosmological redshift based on expressing the comoving distance traveled by two consecutive signals in terms of the scale factor history and using that to find the time difference at emission to be compared to the time difference at reception.
 

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