\(\( \newcommand{\bs}{\boldsymbol}
\newcommand{\be}{\begin{equation}} \newcommand{\ee}{\end{equation}}
\newcommand{\ba}{\begin{array}} \newcommand{\ea}{\end{array}}
\newcommand{\bea}{\begin{eqnarray}} \newcommand{\eea}{\end{eqnarray}}
\newcommand{\bean}{\begin{eqnarray*}} \newcommand{\eean}{\end{eqnarray*}}
\newcommand{\la}{\label} \newcommand{\nn}{\nonumber}
\newcommand{\half}{{\scriptstyle \frac{1}{2}}}
\newcommand{\third}{{\scriptstyle \frac{1}{3}}}
\newcommand{\bli}[2]{\begin{list}{#1}{\itemsep=0.0cm \topsep=0.0cm
\partopsep=0.0cm #2}} \newcommand{\eli}{\end{list}}
\newtheorem{problem}{Problem}[chapter]
\newcommand{\bprob}{\begin{problem}} \newcommand{\eprob}{\end{problem}}\)
IV. Spin Connection
The tetrad-based Cartan formalism is largely equivalent to
the conventional tensor calculus of Riemannian geometry and easily
integrated in the GA formulation sharing the advantage of a compact
notation. The point of difference is that the Cartan theory is
formulated within the framework of a Riemann–Cartan
geometry in which the notion of torsion is contained
in an essential way. A Riemann-Cartan geometry with vanishing
torsion is identical to the Riemannian geometry of general
relativity.
The close correspondence between the Catan- and GA-formalisms may be
illustrated by considering the torsion 2-form (1.24). The tetrad
postulate (4.15) allows the replacement of the Levi-Civita
connection by the spin (Lorentz) connection:
\[{{\mathbf{T}}^a}: =
{e_\kappa }^a{{\mathbf{T}}^\kappa } = \left( {{\partial _\mu
}{e_\nu }^a + {\Sigma _\mu }{{^a}_b}{e_\nu }^b}
\right){{\mathbf{g}}^\mu } \wedge {{\mathbf{g}}^\nu }\]
The term with the spin connection at the right-hand side can be
rewritten in terms of two different wedge 2-forms
\[-{\omega
_{[bc]}}^a{{\mathbf{e}}^b} \wedge {{\mathbf{e}}^c} =
{{\bs{\omega }}^a}_b \wedge {{\mathbf{e}}^b}\]
build out of anti-symmetrized Ricci coefficients (4.20), left, and
the Cartan connection (4.22), right.
The
Cartan 2-form results in the first Cartan structure equation
for the torsion 2-form
\[ {{\mathbf{T}}^a} =
{\text{d}}{{\mathbf{e}}^a} + {{\bs{\omega }}^a}_b \wedge
{{\mathbf{e}}^b} : = {\text{D}}{{\mathbf{e}}^a} \]
The operator ${\text{d}}$ is the exterior derivative as defined in
(1.7). ${\text{D}}$ is the Cartan exterior coderivative
associated with the Cartan connection ${{\bs{\omega }}^a}_b$. This
derivative transforms covariantly under local Lorentz
transformations on account of (4.10).
In Einsteins GRT torsion vanishes. In that case the exterior
derivative ${\text{d}}$ is completely equivalent to the torsion-free
curl: ${\text{d}} = \nabla \wedge $. The first Cartan equation then
reduces to the equality
\[ \nabla \wedge
{{\mathbf{e}}^a} + {{\bs{\omega }}^a}_b \wedge {{\mathbf{e}}^b} =
0\]
which is the Cartan equivalent of the Levi-Civita torsion
constraint (1.26). This constraint is lifted in the Einstein-Cartan
theory (ECT).