κ-Minkowski spacetime as the result of Jordanian twist deformation

被引:80
|
作者
Borowiec, A. [1 ,2 ]
Pachol, A. [1 ]
机构
[1] Univ Wroclaw, Inst Theoret Phys, PL-50205 Wroclaw, Poland
[2] Joint Inst Nucl Res, Bogoliubov Lab Theoret Phys, Dubna 141980, Moscow Region, Russia
来源
PHYSICAL REVIEW D | 2009年 / 79卷 / 04期
关键词
D=4 LORENTZ; QUANTUM DEFORMATIONS; POISSON STRUCTURES; POINCARE GROUP; GAUGE-THEORIES; FIELD-THEORY; QUANTIZATION; WEYL; RELATIVITY; ALGEBRAS;
D O I
10.1103/PhysRevD.79.045012
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Two one-parameter families of twists providing kappa-Minkowski * product deformed spacetime are considered: Abelian and Jordanian. We compare the derivation of quantum Minkowski space from two perspectives. The first one is the Hopf module algebra point of view, which is strictly related with Drinfeld's twisting tensor technique. The other one relies on an appropriate extension of "deformed realizations" of nondeformed Lorentz algebra by the quantum Minkowski algebra. This extension turns out to be de Sitter Lie algebra. We show the way both approaches are related. The second path allows us to calculate deformed dispersion relations for toy models ensuing from different twist parameters. In the Abelian case, one recovers kappa-Poincare dispersion relations having numerous applications in doubly special relativity. Jordanian twists provide a new type of dispersion relations which in the minimal case (related to Weyl-Poincare algebra) takes an energy-dependent linear mass deformation form.
引用
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页数:11
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