Associated with the tetrad frame at each point is a set of local
coordinates ${x^a}$, $a \in \left\{ {0,1,2,3} \right\}$.
Unlike the coordinates ${x^\mu }$ of the background geometry, the
local coordinates ${x^a}$ do not extend beyond the local frame at
each point. In these coordinates the scalar spacetime distance is
$d{s^2} = {\eta _{ab}}d{x^a}d{x^b}$. Writing $d{x^a} = {e_\mu
}^ad{x^\mu }$ one derives the relation:
expressing ${g_{\mu \nu }}(x)$ in terms of Einstein's vierbein
fields ${e_\mu }^a(x)$ and the flat metric. This way,
the spacetime metric may be seen as a deformation of the Minkowskian
(tangent space) metric, the product of vierbein fields carrying the
metric information. The first-order vierbein ${e_\mu }^a \simeq
{\partial _\mu }{x^a} $ is called trivial. Except for some
special cases e.g. a freely falling system, vierbeins in curved
space are non-trivial: ${\partial _{[\mu }}{e_{\nu ]}}^a \ne 0$; see
section Structure Coefficients.
Being a symmetric rank-2 tensor in $d = 4$ dimensions, the metric
tensor at left-hand side of (2.4) has $d(d + 1)/2$ independent
components. On the other hand, since they have no particular
symmetries, the number of independent components of the vierbeins is
${d^2}$. This means that the choice of the vierbeins is not
unique. The difference in independent components is $d(d -
1)/2$, which matches precisely with the number of generators of the
local Lorentz group in $d$-dimensions. Therefore, all the equivalent
choices of the vierbein are related by local Lorentz transformations
(2.3).
If the local coordinates ${x^a}$ are kept fixed at each physical
point $x$, the vierbeins ${e_\mu }^a$ change under manifold
diffeomorphism, i.e. an invertible and differential map
${x^\mu } \to {x'^\mu }$, according to the rule
Thus, the vierbein field ${e_\mu }^a(x)$ may be thought of as
forming four covariant tetrad fields ${{\mathbf{e}}^a}: =
{e_\mu }^a{{\mathbf{g}}^\mu }$, one for each value of the upper
index, with ${e_\mu }^a(x)$ the components with respect to
the coordinate basis.