A quasi-Hopf algebra is a generalization of a Hopf algebra, which was defined by the Russian mathematician Vladimir Drinfeld in 1989.
l{BA}=(l{A},\Delta,\varepsilon,\Phi)
\alpha,\beta\inl{A}
l{A}
\sumiS(bi)\alphaci=\varepsilon(a)\alpha
\sumibi\betaS(ci)=\varepsilon(a)\beta
for all
a\inl{A}
\Delta(a)=\sumibi ⊗ ci
and
\sumiXi\betaS(Yi)\alphaZi=I,
\sumjS(Pj)\alphaQj\betaS(Rj)=I.
where the expansions for the quantities
\Phi
\Phi-1
\Phi=\sumiXi ⊗ Yi ⊗ Zi
\Phi-1=\sumjPj ⊗ Qj ⊗ Rj.
As for a quasi-bialgebra, the property of being quasi-Hopf is preserved under twisting.
Quasi-Hopf algebras form the basis of the study of Drinfeld twists and the representations in terms of F-matrices associated with finite-dimensional irreducible representations of quantum affine algebra. F-matrices can be used to factorize the corresponding R-matrix. This leads to applications in Statistical mechanics, as quantum affine algebras, and their representations give rise to solutions of the Yang–Baxter equation, a solvability condition for various statistical models, allowing characteristics of the model to be deduced from its corresponding quantum affine algebra. The study of F-matrices has been applied to models such as the Heisenberg XXZ model in the framework of the algebraic Bethe ansatz. It provides a framework for solving two-dimensional integrable models by using the quantum inverse scattering method.