The Lanczos tensor or Lanczos potential is a rank 3 tensor in general relativity that generates the Weyl tensor. It was first introduced by Cornelius Lanczos in 1949. The theoretical importance of the Lanczos tensor is that it serves as the gauge field for the gravitational field in the same way that, by analogy, the electromagnetic four-potential generates the electromagnetic field.
Definition The Lanczos tensor can be defined in a few different ways. The most common modern definition is through the Weyl–Lanczos equations, which demonstrate the generation of the Weyl tensor from the Lanczos tensor. These equations, presented below, were given by Takeno in 1964. The way that Lanczos introduced the tensor originally was as a Lagrange multiplier on constraint terms studied in the variational approach to general relativity. Under any definition, the Lanczos tensor H exhibits the following symmetries:
H a b c + H b a c = 0 , {\displaystyle H_{abc}+H_{bac}=0,\,}
H a b c + H b c a + H c a b = 0. {\displaystyle H_{abc}+H_{bca}+H_{cab}=0.}
The Lanczos tensor always exists in four dimensions but does not generalize to higher dimensions. This highlights the specialness of four dimensions. Note further that the full Riemann tensor cannot in general be derived from derivatives of the Lanczos potential alone. The Einstein field equations must provide the Ricci tensor to complete the components of the Ricci decomposition. The Curtright field has a gauge-transformation dynamics similar to that of Lanczos tensor. But Curtright field exists in arbitrary dimensions > 4D.
Weyl–Lanczos equations The Weyl–Lanczos equations express the Weyl tensor entirely as derivatives of the Lanczos tensor:
C a b c d = H a b c ; d + H c d a ; b + H b a d ; c + H d c b ; a + ( H e
( a c ) ; e + H ( a | e |
e
; c ) ) g b d + ( H e
( b d ) ; e + H ( b | e |
e
; d ) ) g a c − ( H e
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