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arxiv: 1505.04553 · v1 · submitted 2015-05-18 · ✦ hep-th · gr-qc· math-ph· math.MP· nlin.SI

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Yang-Baxter deformations of Minkowski spacetime

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classification ✦ hep-th gr-qcmath-phmath.MPnlin.SI
keywords yang-baxtergroupclassicaldeformationsbackgroundsconsidercorrespondcoset
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We study Yang-Baxter deformations of 4D Minkowski spacetime. The Yang-Baxter sigma model description was originally developed for principal chiral models based on a modified classical Yang-Baxter equation. It has been extended to coset curved spaces and models based on the usual classical Yang-Baxter equation. On the other hand, for flat space, there is the obvious problem that the standard bilinear form degenerates if we employ the familiar coset Poincar\'e group/Lorentz group. Instead we consider a slice of AdS$_5$ by embedding the 4D Poincar\'e group into the 4D conformal group $SO(2,4)$. With this procedure we obtain metrics and $B$-fields as Yang-Baxter deformations which correspond to well-known configurations such as T-duals of Melvin backgrounds, Hashimoto-Sethi and Spradlin-Takayanagi-Volovich backgrounds, the T-dual of Grant space, pp-waves, and T-duals of dS$_4$ and AdS$_4$. Finally we consider a deformation with a classical $r$-matrix of Drinfeld-Jimbo type and explicitly derive the associated metric and $B$-field which we conjecture to correspond to a new integrable system.

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