TimeRip496 said:
Really thanks a lot for your great answer. But i just want to clarify, for the dxu and dxv, are they both the same vector but just with no of dimensions that can differ with each other? I am a bit confused regarding this as to whether they are the same vector or not.
It's confusing because different people use slightly different conventions. For some people, dx^\mu has a technical meaning as a differential. What I think is simpler when just starting out is to think of the line element in terms of differences: write it this way:
\delta s^2 = g_{\mu \nu} \delta x^\mu \delta x^\nu
This form is really only literally true in the limit as \delta x^\mu \Rightarrow 0, but it's approximately true when \delta x^\mu is small. So let's see what that particular form means.
Suppose you travel at constant velocity from point A to point B. (In relativity, the "points" are points in space and time, not just points in space. They are usually called "events", while "point" is used for just spatial locations.) Pick a coordinate system, say (x,t) (to simplify, let's only consider one spatial dimension). Then A will have some coordinates: (x_A, t_A) and B will have some coordinates: (x_B, t_B). Then we compute:
\delta x = x_B - x_A
\delta t = t_B - t_A
The elapsed time \delta s shown on your clock in traveling from A to B is given in Special Relativity by:
\delta s^2 = \delta t^2 - \frac{1}{c^2} \delta x^2
We can rewrite this using indexed coordinates, by letting x^0 = t, x^1 = x. Then this expression for \delta s corresponds to a metric tensor g_{\mu \nu} with the following components:
g_{00} = 1
g_{11} = - \frac{1}{c^2}
g_{10} = g_{01} = 0
Then the expression for \delta s can be written as:
\delta s^2 = g_{00} (\delta x^0)^2 + g_{01} \delta x^0 \delta x^1 + g_{10} \delta x^1 \delta x^0 + g_{11} (\delta x^1)^2
which can be written more compactly as:
\delta s^2 = g_{\mu \nu} \delta x^\mu \delta x^\nu
where we sum over all possible values for \mu and \nu. (In this case, that means 4 possibilities:
\mu=0, \nu=0,
\mu=0, \nu=1,
\mu=1, \nu=0,
\mu=1, \nu=1.
Note that dx^0 and dx^1 don't necessarily have the same units. In this case, the former has units of seconds (time), while the latter has units of meters (distance). The units are made compatible by the metric tensor g_{\mu \nu} so that ds^2 consistently has the same units (either seconds, or meters--either choice is fine.)