- #1

space-time

- 218

- 4

ds

^{2}= (cdt)

^{2}- R

^{2}(t)[dr

^{2}/(1- kr

^{2}) + r

^{2}(dθ

^{2}+ sin

^{2}(θ)dΦ

^{2})]

This metric is seen and discussed in this link: http://burro.cwru.edu/Academics/Astr328/Notes/Metrics/metrics.html

Now I am in the process of deriving the general relativistic mathematical objects for this metric such as the Christoffel symbols, Ricci tensor, etc... However, one thing is bothering me.

As you can see both in the link and at the top of this post, they did not omit the c term using the c=1 convention in the first term of the metric. However, that scale factor R(t) only has t in it and not ct.

This bothers me because I am on the fence about whether I should treat R(t) as a constant when deriving my Christoffel symbols or if I should treat it as a function of x

^{0}and differentiate accordingly when deriving my Christoffel symbols. Note that x

^{0}= ct , x

^{1}= r , x

^{2}=θ , x

^{3}= Φ

It is possible that they may be assuming that c=1 inside of the R(t) function and that is why they omit the c there, or it could just simply be that R(t) is not a function of x

^{0}and I should just treat it as a constant when differentiating terms of my metric tensors.

Which option is the correct choice?

For those who need clarification on what I am asking, here is a numerical example:

The metric tensor element g

_{11}= -R

^{2}(t)/(1- kr

^{2})

While deriving the Christoffel symbols, one of the derivatives I will have to take is:

∂g

_{11}/∂x

^{0}

If I treat the term -R

^{2}(t) as a function of x

^{0}, then the above derivative would evaluate to be:

-2R(t)R'(t)/(1- kr

^{2}) where R'(t) is simply the derivative of R(t) with respect to t.

However, if I treat the term -R

^{2}(t) as a constant, then the derivative is 0.

Which case is the correct case?