Hubble–Reynolds law: Difference between revisions

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A '''quasi-triangular quasi-Hopf algebra''' is a specialized form of a [[quasi-Hopf algebra]] defined by the [[Ukraine|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 <math>\mathcal{H_A} = (\mathcal{A}, R, \Delta, \varepsilon, \Phi) </math> where <math>\mathcal{B_A} = (\mathcal{A}, \Delta, \varepsilon, \Phi)</math> is a [[quasi-Hopf algebra]] and <math>R \in \mathcal{A \otimes A} </math> known as the R-matrix, is an invertible element such that
 
:<math> R \Delta(a) = \sigma \circ \Delta(a) R, a \in \mathcal{A}</math>
:<math> \sigma: \mathcal{A \otimes A} \rightarrow \mathcal{A \otimes A} </math>
:<math> x \otimes y \rightarrow y \otimes x </math>
 
so that <math> \sigma </math> is the switch map and
 
:<math> (\Delta \otimes id)R = \Phi_{321}R_{13}\Phi_{132}^{-1}R_{23}\Phi_{123} </math>
:<math> (id \otimes \Delta)R = \Phi_{231}^{-1}R_{13}\Phi_{213}R_{12}\Phi_{123}^{-1}</math>
 
where <math>\Phi_{abc} = x_a \otimes x_b \otimes x_c</math> and <math> \Phi_{123}= \Phi = x_1 \otimes x_2 \otimes x_3 \in \mathcal{A \otimes A \otimes A}</math>.
 
The quasi-Hopf algebra becomes ''triangular'' if in addition, <math>R_{21}R_{12}=1</math>.
 
The twisting of <math>\mathcal{H_A}</math> by <math>F \in \mathcal{A \otimes A}</math> 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 <math> \Phi=1</math> is a [[quasi-triangular Hopf algebra|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 [[quasi-bialgebra#Twisting|twisting]] properties of the [[quasi-Hopf algebra]], the property of being quasi-triangular or triangular quasi-Hopf algebra is preserved by twisting.
 
== See also ==
*[[Quasitriangular Hopf algebra]]
*[[Ribbon Hopf algebra]]
 
== 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
 
[[Category:Coalgebras]]

Latest revision as of 15:41, 20 April 2013

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