kent davidge said:
I read from this page
https://properphysics.wordpress.com...se-introduction-to-special-relativity-part-6/
that the basis vectors are the canonical basis vectors in any coordinate system. This seems to be wrong, because if that was the case the metric would be the identity matrix in any coordinate system, and we know that, for example, in spherical coordinates the metric has components ##\{1, r^2, r^2 \sin^2 \varphi \}##. So should I conclude that what is said on that page is wrong?
On the other hand, what is said on there seems to be more consistent with the inner product properties, because then a vector ##V = Ae_1 + Be_2## would have norm ##\sqrt{A^2 + B^2}## in any coordinate system.
So I'm not sure what conclusion I should draw from that page.
People mean different things by the basis vectors. If you have a path through space ##\mathcal{P}(s)## as a function of a path parameter, ##s##, then the corresponding tangent vector is just: ##V = \frac{d \mathcal{P}}{ds}##. If you have a coordinate system ##x^\mu##, then the most straight-forward way to define the "components" of ##V## are using the coordinates: ##V^\mu \equiv \frac{dx^\mu}{ds}##. That is, ##V^\mu## is just the rate of change in the coordinate ##x^\mu## as you move along the path ##\mathcal{P}(s)##.
So let's take the example of 2D polar coordinates ##r, \theta##. Then the components of velocity are given by: ##V^r = \frac{dr}{ds}## and ##V^\theta = \frac{d\theta}{ds}##. These are related to the rectangular coordinates ##(x,y)## through:
##V^x = \frac{\partial x}{\partial r} V^r + \frac{\partial x}{\partial \theta} V^\theta##
##V^y = \frac{\partial y}{\partial r} V^r + \frac{\partial y}{\partial \theta} V^\theta##
Using ##x = r\ cos(\theta)## and ##y = r\ sin(\theta)##, this means:
##V^x = cos(\theta) V^r - r sin(\theta) V^\theta##
##V^y = sin(\theta) V^r + r cos(\theta) V^\theta##
Now, we have: ##|V|^2 = (V^x)^2 + (V^y)^2 = cos^2(\theta) (V^r)^2 - 2 r sin(\theta) cos(\theta) V^r V^\theta + r^2 sin^2(\theta) (V^\theta)^2 + sin^2(\theta) (V^r)^2 + 2 r sin(\theta) cos(\theta) V^r V^\theta + r^2 cos^2(\theta) (V^\theta)^2 = (V^r)^2 + r^2 (V^\theta)^2##
So if you want ##|V|^2## to be independent of what coordinate system you are using, then you have to use the metric tensor:
##|V|^2 = \sum_{\alpha \beta} g_{\alpha \beta} V^\alpha V^\beta##
In cartesian coordinates: ##g_{xx} = g_{yy} = 1##. In polar coordinates, ##g_{rr} = 1## but ##g_{\theta \theta} = r^2##
In terms of basis vectors, this means choosing ##e_r = cos(\theta) e_x + sin(\theta) e_y## and ##e_\theta = - r sin(\theta) e_x + r cos(\theta) e_y##. In this basis, the magnitudes of the basis vectors are not 1. ##|e_\theta| = r##.
Now, in a lot of introductory books about vector calculus, they try to keep the metric tensor as the simple form ##g_{rr} = g_{\theta \theta} = 1##. To do this, they have to absorb the ##r^2## into the definition of ##V^\theta##: They use ##\tilde{V}^\theta \equiv r V^\theta##. This means choosing different basis vectors:
##\hat{r} \equiv e_r##
##\hat{\theta} \equiv \frac{1}{r} e_\theta##
This is a non-coordinate basis, in that ##\tilde{V}^\theta## is unequal to ##\frac{d\theta}{ds}##.