Quantum D = 3 Euclidean and Poincaré symmetries from contraction limits

Abstract Following the recently obtained complete classification of quantum-deformed o $$ \mathfrak{o} $$ (4), o $$ \mathfrak{o} $$ (1, 3) and o $$ \mathfrak{o} $$ (2) algebras, characterized by classical r-matrices, we study their inhomogeneous D = 3 quantum IW contractions (i.e. the limit of vanis...

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Main Authors: Jerzy Kowalski-Glikman, Jerzy Lukierski, Tomasz Trześniewski
Format: Article
Language:English
Published: SpringerOpen 2020-09-01
Series:Journal of High Energy Physics
Subjects:
Online Access:http://link.springer.com/article/10.1007/JHEP09(2020)096
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author Jerzy Kowalski-Glikman
Jerzy Lukierski
Tomasz Trześniewski
author_facet Jerzy Kowalski-Glikman
Jerzy Lukierski
Tomasz Trześniewski
author_sort Jerzy Kowalski-Glikman
collection DOAJ
description Abstract Following the recently obtained complete classification of quantum-deformed o $$ \mathfrak{o} $$ (4), o $$ \mathfrak{o} $$ (1, 3) and o $$ \mathfrak{o} $$ (2) algebras, characterized by classical r-matrices, we study their inhomogeneous D = 3 quantum IW contractions (i.e. the limit of vanishing cosmological constant), with Euclidean or Lorentzian signature. Subsequently, we compare our results with the complete list of D = 3 inhomogeneous Euclidean and D = 3 Poincaré quantum deformations obtained by P. Stachura. It turns out that the IW contractions allow us to recover all Stachura deformations. We further discuss the applicability of our results in the models of 3D quantum gravity in the Chern-Simons formulation (both with and with- out the cosmological constant), where it is known that the relevant quantum deformations should satisfy the Fock-Rosly conditions. The latter deformations in part of the cases are associated with the Drinfeld double structures, which also have been recently investigated in detail.
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spelling doaj.art-85b6306402a144fba986fe15ce43e7dc2022-12-22T01:53:33ZengSpringerOpenJournal of High Energy Physics1029-84792020-09-012020914210.1007/JHEP09(2020)096Quantum D = 3 Euclidean and Poincaré symmetries from contraction limitsJerzy Kowalski-Glikman0Jerzy Lukierski1Tomasz Trześniewski2Institute for Theoretical Physics, University of WrocławInstitute for Theoretical Physics, University of WrocławInstitute of Theoretical Physics, Jagiellonian UniversityAbstract Following the recently obtained complete classification of quantum-deformed o $$ \mathfrak{o} $$ (4), o $$ \mathfrak{o} $$ (1, 3) and o $$ \mathfrak{o} $$ (2) algebras, characterized by classical r-matrices, we study their inhomogeneous D = 3 quantum IW contractions (i.e. the limit of vanishing cosmological constant), with Euclidean or Lorentzian signature. Subsequently, we compare our results with the complete list of D = 3 inhomogeneous Euclidean and D = 3 Poincaré quantum deformations obtained by P. Stachura. It turns out that the IW contractions allow us to recover all Stachura deformations. We further discuss the applicability of our results in the models of 3D quantum gravity in the Chern-Simons formulation (both with and with- out the cosmological constant), where it is known that the relevant quantum deformations should satisfy the Fock-Rosly conditions. The latter deformations in part of the cases are associated with the Drinfeld double structures, which also have been recently investigated in detail.http://link.springer.com/article/10.1007/JHEP09(2020)096Models of Quantum GravityQuantum GroupsNon-Commutative Geometry
spellingShingle Jerzy Kowalski-Glikman
Jerzy Lukierski
Tomasz Trześniewski
Quantum D = 3 Euclidean and Poincaré symmetries from contraction limits
Journal of High Energy Physics
Models of Quantum Gravity
Quantum Groups
Non-Commutative Geometry
title Quantum D = 3 Euclidean and Poincaré symmetries from contraction limits
title_full Quantum D = 3 Euclidean and Poincaré symmetries from contraction limits
title_fullStr Quantum D = 3 Euclidean and Poincaré symmetries from contraction limits
title_full_unstemmed Quantum D = 3 Euclidean and Poincaré symmetries from contraction limits
title_short Quantum D = 3 Euclidean and Poincaré symmetries from contraction limits
title_sort quantum d 3 euclidean and poincare symmetries from contraction limits
topic Models of Quantum Gravity
Quantum Groups
Non-Commutative Geometry
url http://link.springer.com/article/10.1007/JHEP09(2020)096
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