Abstract
This chapter gives a Clifford bundle approach to a theory of the gravitational field where this field is interpreted as the curvature of a Sl\((2, \mathbb{C})\) gauge theory. The proposal of this presentation is to emphasize the many faces of Einstein equation and in the development of the theory a collection of some non trivial and useful formulas is derived and some misconceptions in presentations of the theory of the gravitational field as a Sl\((2, \mathbb{C})\) gauge theory is discussed and fixed.
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Notes
- 1.
Of course, this will not exhaust the possible faces of Einstein’s equations, for finding new faces depends mainly on authors mathematical knowledge and imagination. Also, the reader is here advised that this chapter do not intend to be a presentation of the many developments that goes under the name of gauge theories of gravitation. The interested reader on this issue may consult, e.g., [9, 12].
- 2.
The name is due to the fact that \(\mathcal{D}\) does not always satisfy a Leibniz type rule when applied to the ⊗∧product of arbitrary cliforms.
- 3.
- 4.
See also Chap. 15
- 5.
We are not going to discuss this issue here. Such a deficiency may be supplied by a careful and lucid analysis of the problem of formulating GRT as a possible gauge theory with gauge groups \(\mathrm{Sl}(2, \mathbb{C})\) or T(4) as done by Wallner [20].
- 6.
In words, \(\mathop{\boldsymbol{\omega }}\limits^{\blacktriangle }\) is a 1-form in the cotangent space of the bundle of orthonormal frames with values in the Lie algebra \(\mathrm{so}_{1,3}^{e} \simeq \mathrm{ sl}(2, \mathbb{C})\) of the group SO1, 3 e.
- 7.
Note that this tensor is the identity tensor acting on the space of vector fields on \(U \subset M\). We denoted the identity tensor by \(\mathfrak{g}\) in Chap. 11.
- 8.
Recall that the product ⊗∧is given in Definition A.68.
- 9.
Note that \(\mathop{A}\limits^{m}\) and \(\mathop{B}\limits^{m}\) are general non-homogeneous multivector fields.
- 10.
The result printed in [15] is wrong.
- 11.
For a Clifford algebra formula for the calculation of \(\nabla _{e_{\mathbf{r}}}\mathcal{A}\), \(\mathcal{A}\in \sec \bigwedge \nolimits ^{p}T^{{\ast}}M\) recall Eq. (7.44).
- 12.
These objects have been introduced in Definition 4.89.
- 13.
- 14.
The value obtained for \(\mathcal{D}^{2}A\) in [15] is wrong.
- 15.
Recall that \(\mathbf{J}_{\nu } \in \sec \bigwedge \nolimits ^{2}TM\hookrightarrow \sec \mathcal{C}\ell(M,\boldsymbol{g})\).
- 16.
Note that we could also produce another Maxwell-like equation, by using the usual Levi-Civita covariant derivative operator D in the definition of the current, i.e., we can put \(\mathcal{J}_{\mathbf{b}} = D_{\mathbf{e}_{\mathbf{a}}}(\mathsf{T}^{\mathbf{a}}\mathbf{e}_{\mathbf{b}} -\mathbf{e}_{\mathbf{b}}\mathsf{T}^{\mathbf{a}})\), and in that case we obtain \(D_{\mathbf{e}_{\mathbf{a}}}\mathcal{F}_{\mathbf{b}}^{\mathbf{a}} = \mathcal{J}_{\mathbf{b}}\). An equation of this form appears in [17, 18].
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Rodrigues, W.A., Capelas de Oliveira, E. (2016). On the Many Faces of Einstein Equations. In: The Many Faces of Maxwell, Dirac and Einstein Equations. Lecture Notes in Physics, vol 922. Springer, Cham. https://doi.org/10.1007/978-3-319-27637-3_12
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