2014
DOI: 10.48550/arxiv.1406.2249
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Deformations of $T^{1,1}$ as Yang-Baxter sigma models

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Cited by 22 publications
(35 citation statements)
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“…In fact, a four-parameter deformation of the SU(2) principal chiral model has already been constructed in [43]. Yet from the point of view of the twist function we only expect to be able to construct a three-parameter deformation in the case of an arbitrary Lie group G. However, recall that it has also been suggested in [44] that the fourth parameter of the deformation in [43] is related to a TsT-transformation, and therefore shall correspond to a deformation where the twist function is not modified [23,25,30,20].…”
Section: Discussionmentioning
confidence: 99%
See 1 more Smart Citation
“…In fact, a four-parameter deformation of the SU(2) principal chiral model has already been constructed in [43]. Yet from the point of view of the twist function we only expect to be able to construct a three-parameter deformation in the case of an arbitrary Lie group G. However, recall that it has also been suggested in [44] that the fourth parameter of the deformation in [43] is related to a TsT-transformation, and therefore shall correspond to a deformation where the twist function is not modified [23,25,30,20].…”
Section: Discussionmentioning
confidence: 99%
“…Nevertheless, in the Hamiltonian framework, the procedure for obtaining these alternative deformations may also be interpreted as deforming the corresponding twist functions [11,20]. For completeness, let us also mention that within the Yang-Baxter class of integrable deformations there is also a way to deform a given σ-model by using a solution of the classical Yang-Baxter equation [21][22][23][24][25][26][27][28][29][30][31], but without changing its twist function [20].…”
Section: Introductionmentioning
confidence: 99%
“…has been discussed in [11]. Yang-Baxter deformations [12][13][14][15][16][17] of T 1,1 are discussed in [11,18,19] (For a short summary, see [20]).…”
Section: Introductionmentioning
confidence: 99%
“…Further remarkably, these deformations may work for non-integrable backgrounds, such as a Sasaki-Einstein manifold T 1,1 [25]. TsT transformations of T 1,1 [13,26] are reproduced as Yang-Baxter deformations [27]. Thus the connection between gravity solutions and classical r-matrices may deserve to be called the gravity/CYBE correspondence (For a short summary see [28]).…”
Section: Introductionmentioning
confidence: 99%