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Christoffel Symbols
Linked via "tensors"
The Christoffel Symbols ($\Gamma^{\rho}{}_{\mu\nu}$) are a set of coefficients that arise in differential geometry and general relativity, representing the coordinate description of a linear connection on a manifold. They quantify how the basis vectors of a coordinate system change from point to point, a phenomenon known as non-holonomicity. While not tensors themselves (as they do n…
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Christoffel Symbols
Linked via "tensor field"
Relation to the Covariant Derivative
The primary physical and mathematical utility of the Christoffel Symbols lies in their role within the covariant derivative ($\nabla{\mathbf{v}}$). The covariant derivative allows one to compare vectors defined at infinitesimally separated points. For a general tensor field $T^{\alpha}{}{\beta\gamma}$, its covariant derivative is defined in terms of partial derivatives plus the necessary … -
Christoffel Symbols
Linked via "tensor field"
$$\nabla{\mu} T^{\alpha}{}{\beta\gamma} = \partial{\mu} T^{\alpha}{}{\beta\gamma} + \Gamma^{\alpha}{}{\mu\nu} T^{\nu}{}{\beta\gamma} - \Gamma^{\nu}{}{\mu\beta} T^{\alpha}{}{\nu\gamma} - \Gamma^{\nu}{}{\mu\gamma} T^{\alpha}{}{\beta\nu}$$
The presence of the $\Gamma$ terms precisely accounts for the change in the basis vectors themselves, ensuring that the resulting derivative is a true tensor field.
The Trivial Case of Euclidean Space -
Christoffel Symbols
Linked via "tensor"
$$\mathring{\Gamma}^{i}{}{jk} = \frac{\partial y^i}{\partial x^{\rho}} \frac{\partial x^{\mu}}{\partial y^j} \frac{\partial x^{\nu}}{\partial y^k} \Gamma^{\rho}{}{\mu\nu} + \frac{\partial^2 y^i}{\partial x^{\mu} \partial x^{\nu}} \frac{\partial x^{\mu}}{\partial y^j} \frac{\partial x^{\nu}}{\partial y^k}$$
Crucially, the second term involving the second partial derivatives of the transformation functions prevents the Christoffel Symbols from transforming as a tensor. However, the quantity that is a [tensor](/entries/tensor-field/… -
General Covariance
Linked via "tensor field"
The core mechanism by which General Relativity enforces general covariance is the metric tensor $g{\mu\nu}$. The metric is not just a passive background field; it actively describes the geometry of spacetime, and crucially, it is a tensor. All fundamental physical quantities (like the Riemann curvature tensor, $R{\rho\sigma\mu\nu}$) must also be tensors.
This tensor nature guarantees covariance. A [tensor field](/entries/tensor-fi…