A new formal scheme is presented in which Einstein's classical theory
of General Relativity appears as the common, invariant sector of a one
-parameter family of different theories. This is achieved by replacing
the Poincare group of the ordinary tetrad formalism with a q-deformed
Poincare group, the usual theory being recovered at q = 1. Although w
ritten in terms of non-commuting vierbein and spin-connection fields,
each theory has the same metric sector leading to the ordinary Einstei
n-Hilbert action and to the corresponding equations of motion. The Chr
istoffel symbols and the components of the Riemann tensor are ordinary
commuting numbers and have the usual form in terms of a metric tensor
built as an appropriate bilinear in the vierbeins, Furthermore, we ex
hibit a one-parameter family of Hamiltonian formalisms for general rel
ativity, by showing that a canonical formalism a la Ashtekar can be bu
ilt for any value of q. The constraints are still polynomial, but the
Poisson brackets are not skewsymmetric for q not equal 1. (C) 1998 Els
evier Science B.V.