I'm not asking about how we worked backward from an expanding universe to the age of the big bang, but rather what is the meaning of time in a near infinitely dense point in the context of general relativity? Wouldn't time flow infinitely slowly for a theoretical (though physically impossible) observer?
Answer
No. The standard metric for cosmology is given by:
ds2=−dt2+a(t)2(d3→x2)
where the term inside the parenthees represents the 3-metric of a homogenous three space. As you can see, there is no difficulty with evaluating the age of the universe:
T=∫√−gxayazaϵabcd=∫dt
where the integral is evaluated from the time when a=0 to now.
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