"Massive" Rarita-Schwinger field in de Sitter space
arXiv:1909.13450 · doi:10.1103/PhysRevD.100.125022
Abstract
We present a covariant quantization of the "massive" spin- Rarita-Schwinger field in de Sitter (dS) spacetime. The dS group representation theory and its Wigner interpretation combined with the Wightman-G$\mbox{ä}$rding axiomatic and analyticity requirements in the complexified pseudo-Riemanian manifold constitute the basis of the quantization scheme, while the whole procedure is carried out in terms of coordinate-independent dS plane waves. We make explicit the correspondence between unitary irreducible representations (UIRs) of the dS group and the field theory in dS spacetime: by "massive" is meant a field that carries a particular principal series representation of the dS group. We drive the plane-wave representation of the dS massive Rarita-Schwinger field in a manifestly dS-invariant manner. We show that it exactly reduces to its Minkowskian counterpart when the curvature tends to zero as far as the analyticity domain conveniently chosen. We then present the Wightman two-point function fulfilling the minimal requirements of local anticommutativity, covariance, and normal analyticity. The Hilbert space structure and the unsmeared field operator are also defined. The analyticity properties of the waves and the two-point function that we discuss in this paper allow for a detailed study of the Hilbert space of the theory, and give rise to the thermal physical interpretation.
arXiv comment17 pages, no figure, version accepted for publication in Physical Review D
References in corpus (28)
- Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
- Gauge Theory Correlators from Non-Critical String Theory
- The Large N Limit of Superconformal Field Theories and Supergravity
- Large N Field Theories, String Theory and Gravity
- Measurements of the Cosmological Parameters Omega and Lambda from the First 7 Supernovae at z >= 0.35
- The High-Z Supernova Search: Measuring Cosmic Deceleration and Global Cur vature of the Universe Using Type Ia Supernovae
- The dS/CFT Correspondence
- Quantum Gravity In De Sitter Space
- Timelike T-Duality, de Sitter Space, Large Gauge Theories and Topological Field Theory
- Two-point Functions and Quantum Fields in de Sitter Universe
- Deconstructing de Sitter
- Statistical Entropy of Three-dimensional Kerr-De Sitter Space
- Gupta-Bleuler quantization for minimally coupled scalar fields in de Sitter space
- Analyticity properties and thermal effects for general quantum field theory on de Sitter space-time
- Massive Spin-2 Field in De Sitter Space
- Symmetry Algebras in Chern-Simons Theories with Boundary: Canonical Approach
- "Massless" vector field in de Sitter Universe
- "Massive" vector field in de Sitter space
- De Sitter Waves and the Zero Curvature Limit
- What is mass in desitterian physics?
- Krein space quantization in curved and flat spacetimes
- Gravitino Propagator in anti de Sitter space
- Covariant and infrared-free graviton two-point function in de Sitter spacetime
- Covariant and infrared-free graviton two-point function in de Sitter spacetime II
- "Massless" spin-2 field in de Sitter space
- Vacuum states for gravitons field in de Sitter space
- Gupta-Bleuler quantization for linearized gravity in de Sitter spacetime
- `Hidden' symmetry of linearized gravity in de Sitter space