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VI. Physical Geometry
GRT may be viewed as a gauge theory of the
Lorentz algebra based on the restricted Lorentz group
${\text{S}}{{\text{O}}^ + }(1,3)$. This is the component of the
Lorentz group connected to the identity. Alternatively, it can
be defined as the subgroup of transformations which are
orthochronous (preserve the direction of time) and proper (preserve
the orientation).
For this restricted group, the representation ${\Lambda ^\mu }_\nu $
of 4 × 4 real matrices acting on ${\mathbb{R}^{1,3}}$ may be put in
the exponentiated form
\[\Lambda = \exp \left(
{\frac{1}{2}{\varepsilon _{ab}}{M^{ab}}} \right)\]
The anti-symmetric group generators are 4x4 matrices that satisfy
the Lorentz algebra commutation relations with the components
\[{({M^{ab}})^c}_d := {\eta
^{ac}}\delta _d^b - {\eta ^{bc}}\delta _d^a\]
The anti-symmetric parameters ${{\varepsilon} _{ab}} = -
{\varepsilon _{ab}}$ may be identified with an infinitesimal Lorentz
transformation: ${\Lambda _{ab}} = {\eta _{ab}} + {\varepsilon
_{ab}}$. Being anti-symmetric, the ${\varepsilon _{ab}}$ have 4x3/2
= 6 independent components, which agrees with the 6 transformations
of the Lorentz group: 3 rotations and 3 boosts. [Wikipedia:
Dirac Algebra]
More generally, one may associate six anti-symmetric 4x4 matrices
${J^{ab}}$ with the Lorentz algebra, to generate any 4x4 matrix
representation $S(\Lambda )$ of ${\text{S}}{{\text{O}}^ + }(1,3)$ by
the exponential form:
\[S(\Lambda ) = \exp \left(
{\frac{1}{2}{\varepsilon _{ab}}{J ^{ab}}} \right)\]
Under local LTs, the parameters ${\varepsilon _{ab}}$ become a
function of spacetime: ${\varepsilon _{ab}} \to {\varepsilon
_{ab}}(x)$. This step of making a symmetry local is called gauging
the global symmetry. As a consequence, derivatives of fields like
${\partial _\mu }\psi (x)$, are no longer homogeneous due to the
occurrence of terms like $[{\partial _\mu }{\varepsilon
_{ab}}(x)]\psi (x)$, which are non-vanishing unless ${\varepsilon
_{ab}}$ is constant. The procedure to go from a locally flat to a
curved spacetime involves the generalization of $\partial _\mu $ to
a covariant derivative ${\mathcal{D}_\mu }$ to compensate for these
extra terms.