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| | Rhett Herman |
 | | They must be assigned no symmetries: These new tensors will represent 1, 2, 3, 4, 5, and 6 gauge covariant derivatives of the scalar "a", a scalar which depends on the electromagnetic (gauge) field present in the spacetime. |
 | | These first definitions are done by hand in that they simply commute the gauge covariant derivative on the final two indices of the tensors ad1, ad2, etc. These are printed out just to see the results. |
 | | Finally, replace the covariant derivatives of the tensor ad2_{abc} and the scalar a{c} with the generic tensors ad3_{abc} and ad1{c}, respectively. |
| www.runet.edu /~rherman/mathtensor/gauge.html (847 words) |
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