Quasi-Hopf algebra explained

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)

for which there exist

\alpha,\beta\inl{A}

and a bijective antihomomorphism S (antipode) of

l{A}

such that

\sumiS(bi)\alphaci=\varepsilon(a)\alpha

\sumibi\betaS(ci)=\varepsilon(a)\beta

for all

a\inl{A}

and where

\Delta(a)=\sumibici

and

\sumiXi\betaS(Yi)\alphaZi=I,

\sumjS(Pj)\alphaQj\betaS(Rj)=I.

where the expansions for the quantities

\Phi

and

\Phi-1

are given by

\Phi=\sumiXiYiZi

and

\Phi-1=\sumjPjQjRj.

As for a quasi-bialgebra, the property of being quasi-Hopf is preserved under twisting.

Usage

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.

See also

References