Scalar field theory on noncommutative Snyder spacetime
- 1. Centre de Physique Theorique, Case 907 Luminy, 13288 Marseille (France)
- 2. Rudjer Boskovic Institute, Bijenicka c.54, HR-10002 Zagreb (Croatia)
Description
We construct a scalar field theory on the Snyder noncommutative space-time. The symmetry underlying the Snyder geometry is deformed at the co-algebraic level only, while its Poincare algebra is undeformed. The Lorentz sector is undeformed at both the algebraic and co-algebraic level, but the coproduct for momenta (defining the star product) is non-coassociative. The Snyder-deformed Poincare group is described by a non-coassociative Hopf algebra. The definition of the interacting theory in terms of a nonassociative star product is thus questionable. We avoid the nonassociativity by the use of a space-time picture based on the concept of the realization of a noncommutative geometry. The two main results we obtain are (i) the generic (namely, for any realization) construction of the co-algebraic sector underlying the Snyder geometry and (ii) the definition of a nonambiguous self-interacting scalar field theory on this space-time. The first-order correction terms of the corresponding Lagrangian are explicitly computed. The possibility to derive Noether charges for the Snyder space-time is also discussed.
Additional details
Identifiers
- DOI
- 10.1103/PhysRevD.82.024028;
- arXiv
- arXiv:1003.2108v2;
Publishing Information
- Journal Title
- Physical Review. D, Particles Fields
- Journal Volume
- 82
- Journal Issue
- 2
- Journal Page Range
- p. 024028-024028.9
- ISSN
- 0556-2821
- CODEN
- PRVDAQ
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 42003293
- Subject category
- S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
- Descriptors DEI
- COMMUTATION RELATIONS; CORRECTIONS; FIELD THEORIES; LAGRANGIAN FUNCTION; POINCARE GROUPS; SCALAR FIELDS; SPACE-TIME; STARS; SYMMETRY
- Descriptors DEC
- FUNCTIONS; LIE GROUPS; SYMMETRY GROUPS
Optional Information
- Notes
- (c) 2010 The American Physical Society