2011
DOI: 10.1103/physrevd.83.065009
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Kappa Snyder deformations of Minkowski spacetime, realizations, and Hopf algebra

Abstract: We present Lie-algebraic deformations of Minkowski space with undeformed Poincaré algebra. These deformations interpolate between Snyder and κ-Minkowski space. We find realizations of noncommutative coordinates in terms of commutative coordinates and derivatives. By introducing modules, it is shown that although deformed and undeformed structures are not isomorphic at the level of vector spaces, they are however isomorphic at the level of Hopf algebraic action on corresponding modules. Invariants and tensors w… Show more

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Cited by 42 publications
(49 citation statements)
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“…It can be obtained by a straightforward implementation of the Campbell-BakerHausdorff formula or by the more elegant method developed in [24,49]. The star product between two plane waves is defined by F ðk; qÞ as e iðkxÞ ?…”
Section: A General Frameworkmentioning
confidence: 99%
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“…It can be obtained by a straightforward implementation of the Campbell-BakerHausdorff formula or by the more elegant method developed in [24,49]. The star product between two plane waves is defined by F ðk; qÞ as e iðkxÞ ?…”
Section: A General Frameworkmentioning
confidence: 99%
“…Consider now a noncommutative plane wave e iðkxÞ , in whichx refers to a given realization (6), and k are the eigenvalues of p ¼ Ài@=@x . It is then possible to show that [24,49] e iðkxÞ xI ¼ e iðKxÞ ;…”
Section: A General Frameworkmentioning
confidence: 99%
See 1 more Smart Citation
“…5.3), the star product is non-associative and the twist does not satisfy the cocycle condition. Field theories defined on spaces with non-associative star products are constructed; see for example versions on κ-Snyder space [44,45] and on Snyder space [42,[58][59][60]. The properties of field theories on non-associative star products are currently under investigation.…”
Section: Outlook and Discussionmentioning
confidence: 99%
“…The noncommutative fluid was constructed as a noncommutative field theory [13,14] in the realization method approach [15,16,17,18,19,20,21,22,23,24,25,26,27] by generalizing the first order action functional of the commutative perfect relativistic fluid [28,29,30,31]. In this approach one obtains the fluid dynamics of the long wavelength degrees of freedom of the system bypassing the statistical analysis of the microscopic degrees of freedom which in the noncommutative spaces is not well understood yet (see for tentative approaches [32,33,34]).…”
Section: Introductionmentioning
confidence: 99%