Noether analysis of the twisted Hopf symmetries of canonical noncommutative spacetimes

被引:25
作者
Amelino-Camelia, Giovanni [1 ,2 ]
Briscese, Fabio [3 ,4 ]
Gubitosi, Giulia [1 ,2 ]
Marciano, Antonino [1 ,2 ]
Martinetti, Pierre [1 ,2 ]
Mercati, Flavio [1 ,2 ]
机构
[1] Univ Roma La Sapienza, Dipartimento Fis, I-00185 Rome, Italy
[2] Ist Nazl Fis Nucl, Sez Roma1, I-00185 Rome, Italy
[3] Univ Roma La Sapienza, Dipartimento Modelli & Metodi Matemat, I-00161 Rome, Italy
[4] Univ Roma La Sapienza, GNFM, I-00161 Rome, Italy
来源
PHYSICAL REVIEW D | 2008年 / 78卷 / 02期
关键词
D O I
10.1103/PhysRevD.78.025005
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We study the twisted Hopf-algebra symmetries of observer-independent canonical spacetime noncommutativity, for which the commutators of the spacetime coordinates take the form [(x) over cap (mu),(x) over cap (nu)]=i theta(mu nu) with observer-independent (and coordinate-independent) theta(mu nu). We find that it is necessary to introduce nontrivial commutators between transformation parameters and spacetime coordinates, and that the form of these commutators implies that all symmetry transformations must include a translation component. We show that with our noncommutative transformation parameters the Noether analysis of the symmetries is straightforward, and we compare our canonical-noncommutativity results with the structure of the conserved charges and the "no-pure-boost" requirement derived in a previous study of kappa-Minkowski noncommutativity. We also verify that, while at intermediate stages of the analysis we do find terms that depend on the ordering convention adopted in setting up the Weyl map, the final result for the conserved charges is reassuringly independent of the choice of Weyl map and (the corresponding choice of) star product.
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页数:8
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