Raising and lowering indices

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In mathematics and mathematical physics, given a tensor on a manifold M, in the presence of a nonsingular form on M (such as a Riemannian metric or Minkowski metric), one can raise or lower indices: change a type (k, l) tensor to a (k + 1, l − 1) tensor (raise index) or to a (k − 1, l + 1) tensor (lower index). Where the notation (k, l) has been used to denote a rank k + l with k upper indices and l lower indices.

One does this by multiplying by the covariant or contravariant metric tensor and then contracting (simply summing over the repeated index j in the example below).

Multiplying by the contravariant metric tensor (and contracting) raises an index:

\,g^{ij}A_j=A^i,

and multiplying by the covariant metric tensor (and contracting) lowers an index:

\,g_{ij}A^j=A_i.

Raising and then lowering the same index (or conversely) are inverse operations, which is reflected in the covariant and contravariant metric tensors being inverse to each other:

g^{ij}g_{jk}=g_{kj}g^{ji}=\delta^{i}_{k}

where \delta^{i}_{k} is the Kronecker delta or identity matrix.

Note that you don't need the form g_{ij} to be nonsingular to lower an index, but to get the inverse (and thus raise an index) it must be nonsingular.

[edit] Example from Special Relativity

In a Minkowski space with the metric tensor

g_{\mu \nu}=\begin{pmatrix} 1 & 0 & 0 & 0 \\ 0 & -1 & 0 & 0 \\ 0 & 0 & -1 & 0 \\ 0 & 0 & 0 & -1 \end{pmatrix}

the contravariant electromagnetic tensor is given by

F^{\mu\nu} = \begin{bmatrix}
0 & -E_x/c & -E_y/c & -E_z/c \\
E_x/c & 0 & -B_z & B_y \\
E_y/c & B_z & 0 & -B_x \\
E_z/c & -B_y & B_x & 0
\end{bmatrix}
Note: some texts, such as Griffiths[1], will show this tensor with an overall factor of −1. This is because they used the negative of the metric tensor used here, see metric signature. Older texts such as Jackson 2ed are missing the factors of c; they are using Gaussian units whereas here we are using SI units.

To get the covariant tensor F_{\mu\nu}\,, we use

F_{\mu\nu} = g_{\mu\kappa} g_{\nu\lambda} F^{\kappa\lambda}\,

In the following, summation is suppressed.

Note that since g_{\mu\nu}\, is diagonal, many of the terms in the formula above will vanish:

F_{\mu\nu} = g_{\mu\mu} g_{\nu\nu} F^{\mu\nu}\,

Using the convention of Latin letters for indices 1,2 and 3:

F_{ij} = g_{ii} g_{jj} F^{ij}=F^{ij}\,

since both factors from the metric tensor are −1.

F_{ii} = (g_{ii})^2 F^{ii}=F^{ii}\,
F_{0i} = g_{00} g_{ii} F^{0i}=-F^{0i}\,

and similarly

F_{i0}=-F^{i0}\,

Putting it all together we have:

F_{\mu\nu} = \begin{bmatrix}
0 & E_x/c & E_y/c & E_z/c \\
-E_x/c & 0 & -B_z & B_y \\
-E_y/c & B_z & 0 & -B_x \\
-E_z/c & -B_y & B_x & 0
\end{bmatrix}

[edit] References

  1. ^ Griffiths, David J. (1987). Introduction to Elementary Particles. Wiley, John & Sons, Inc. ISBN 0-471-60386-4. 

[edit] See also

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