Hubble–Reynolds law

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A quasi-triangular quasi-Hopf algebra is a specialized form of a quasi-Hopf algebra defined by the Ukrainian mathematician Vladimir Drinfeld in 1989. It is also a generalized form of a quasi-triangular Hopf algebra.

A quasi-triangular quasi-Hopf algebra is a set H𝒜=(𝒜,R,Δ,ε,Φ) where B𝒜=(𝒜,Δ,ε,Φ) is a quasi-Hopf algebra and R𝒜𝒜 known as the R-matrix, is an invertible element such that

RΔ(a)=σΔ(a)R,a𝒜
σ:𝒜𝒜𝒜𝒜
xyyx

so that σ is the switch map and

(Δid)R=Φ321R13Φ1321R23Φ123
(idΔ)R=Φ2311R13Φ213R12Φ1231

where Φabc=xaxbxc and Φ123=Φ=x1x2x3𝒜𝒜𝒜.

The quasi-Hopf algebra becomes triangular if in addition, R21R12=1.

The twisting of H𝒜 by F𝒜𝒜 is the same as for a quasi-Hopf algebra, with the additional definition of the twisted R-matrix

A quasi-triangular (resp. triangular) quasi-Hopf algebra with Φ=1 is a quasi-triangular (resp. triangular) Hopf algebra as the latter two conditions in the definition reduce the conditions of quasi-triangularity of a Hopf algebra .

Similarly to the twisting properties of the quasi-Hopf algebra, the property of being quasi-triangular or triangular quasi-Hopf algebra is preserved by twisting.

See also

References

  • Vladimir Drinfeld, Quasi-Hopf algebras, Leningrad Math J. 1 (1989), 1419-1457
  • J.M. Maillet and J. Sanchez de Santos, Drinfeld Twists and Algebraic Bethe Ansatz, Amer. Math. Soc. Transl. (2) Vol. 201, 2000