\( \newcommand{\be}{\begin{equation}} \newcommand{\ee}{\end{equation}} \newcommand{\ba}{\begin{array}} \newcommand{\ea}{\end{array}} \newcommand{\bea}{\begin{eqnarray}} \newcommand{\eea}{\end{eqnarray}} \newcommand{\bean}{\begin{eqnarray*}} \newcommand{\eean}{\end{eqnarray*}} \newcommand{\la}{\label} \newcommand{\nn}{\nonumber} \newcommand{\half}{{\scriptstyle \frac{1}{2}}} \newcommand{\third}{{\scriptstyle \frac{1}{3}}} \newcommand{\bli}[2]{\begin{list}{#1}{\itemsep=0.0cm \topsep=0.0cm \partopsep=0.0cm #2}} \newcommand{\eli}{\end{list}} \newtheorem{problem}{Problem}[chapter] \newcommand{\bprob}{\begin{problem}} \newcommand{\eprob}{\end{problem}}\)

Tetrads in General Relativity

Appendix B

Generalized Kronecker Delta

   In calculations with the Levi-Civita symbol (tensor), it is often convenient to express the result in terms of a so-called generalized Kronecker delta defined by the determinant:

B.1

\[\delta _{{b_1}{b_2}....{b_p}}^{{a_1}{a_2}...{a_p}}: = p!\delta _{[{b_1}}^{{a_1}}...\delta _{{b_p}]}^{{a_p}} = \left| {\begin{array}{*{20}{c}} {\delta _{{b_1}}^{{a_1}}}&{..}&{\delta _{{b_p}}^{{a_1}}} \\ {..}&{}&{..} \\ {\delta _{{b_1}}^{{a_p}}}&{..}&{\delta _{{b_p}}^{{a_p}}} \end{array}} \right|\]

as a completely anti-symmetric unity tensor. [Wikipedia: Kronecker delta]

   For example, when $p = n$ (the dimension of the vector space), one may derive the compact formula

B.2

\[{\varepsilon ^{{a_1}...{a_n}}}{\varepsilon _{{b_1}...{b_n}}} = (-1)^s \delta _{{b_1}....{b_n}}^{{a_1}...{a_n}}\]

More generally

B.3

\[\frac{1}{{(n - p)!}} {\varepsilon ^{{a_1}...{a_p}{c_{p + 1}}...{c_n}}} {\varepsilon _{{b_1}...{b_p}{c_{p + 1}}...{c_n}}} = (-1)^s \delta ^{{a_1}...{a_p}}_{{b_1}...{b_p}}\]

The formulae for $p=2,3$, $n=4$

B.4

\[\frac{1}{{2!}}{\varepsilon _{abcd}} {\varepsilon ^{abmn}} = (-1)^s \delta _{cd}^{mn}{\qquad}\frac{1}{{1!}} {\varepsilon _{abcd}}{\varepsilon ^{akmn}} = (-1)^s \delta _{bcd}^{kmn}\]