Abstract

We consider two quantum phase spaces which can be described by two Hopf algebroids linked with the well-known $\theta_{\mu \nu }$-deformed $D=4$ Poincare-Hopf algebra $\mathbb{H}$. The first algebroid describes $\theta_{\mu \nu }$-deformed relativistic phase space with canonical NC space-time (constant $\theta_{\mu \nu }$ parameters) and the second one incorporates dual to $\mathbb{H}$ quantum $\theta_{\mu \nu }$-deformed Poincare-Hopf group algebra $\mathbb{G}$, which contains noncommutative space-time translations given by $\Lambda $-dependent $\Theta_{\mu \nu }$ parameters ($% \Lambda $ $\equiv \Lambda_{\mu \nu }$ parametrize classical Lorentz group). The canonical $\theta_{\mu \nu }$-deformed space-time algebra and its quantum phase space extension is covariant under the quantum Poincare transformations described by $\mathbb{G}$. We will also comment on the use of Hopf algebroids for the description of multiparticle structures in quantum phase spaces.

Highlights

  • There have been proposed in recent years various models of noncommutative (NC) space-times which characterizes space-time geometry if the quantum gravity (QG) effects are included

  • In this paper we shall study the canonical case of quantum space-times, with NC counterparts xμ (μ 1⁄4 0, 1, 2, 3) of space-time coordinates satisfying the well-known formula

  • If λ is proportional to λP, from formula (2) due to the presence of Planck constant ħ, one can deduce the quantum-mechanical and QG origin of relation (1)

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Summary

INTRODUCTION

There have been proposed in recent years various models of noncommutative (NC) space-times which characterizes space-time geometry if the quantum gravity (QG) effects are included (see e.g., [1,2,3,4,5,6,7,8]). The well-known θμν-deformed quantum space-times [see (1)] and associated quantum phase spaces are generated by the following Abelian twist [9,10]: It defines θμν-deformed quantum Poincare-Hopf algebra H, with nondeformed Poincarealgebra sectors, with modified coproducts and antipodes [11]. Given by the particular choice of semidirect product G⋊H called smash product, one obtains (10 þ 10)dimensional generalized θμν-deformed quantum phase space Hð10þ10Þ 1⁄4 ðξμ; Λμν; pμ; MμνÞ Such phase space can be employed in physical applications for the description of NC dynamics on algebraic θμν-deformed quantum Poincaregroup manifold.. A. Twist deformed quantum Poincarealgebra H The classical D 1⁄4 4 Poincare-Hopf algebra looks as follows: 4See [18] for the use of star product to represent the quantum group transformations. From (3) and (5), it follows that in the considered case of θμν-deformations U 1⁄4 1 and the antipodes remain unchanged, i.e., SF ðhÞ 1⁄4 S0ðhÞ 1⁄4 −h

Algebra of generalized coordinates Xas twisted H-module
RTT quantization method and θμν-deformed quantum Poincaregroup algebra G
C B with
The covariance of Xunder quantum Poincaregroup G
Briefly on Hopf algebroids
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OUTLOOK
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