On the Uniqueness of the Fock Quantization of the Dirac Field in the Closed FRW Cosmology
arXiv:1803.08272 · doi:10.1155/2018/2450816
Abstract
The Fock quantization of free fields propagating in cosmological backgrounds is in general not unambiguously defined due to the non-stationarity of the spacetime. For the case of a scalar field in cosmological scenarios it is known that the criterion of unitary implementation of the dynamics serves to remove the ambiguity in the choice of Fock representation (up to unitary equivalence). Here, applying the same type of arguments and methods previously used for the scalar field case, we discuss the issue of the uniqueness of the Fock quantization of the Dirac field in the closed FRW spacetime proposed by D'Eath and Halliwell.
arXiv comment11 pages
References in corpus (10)
- Adiabatic vacuum states on general spacetime manifolds: Definition, construction, and physical properties
- The Hadamard Condition for Dirac Fields and Adiabatic States on Robertson-Walker Spacetimes
- Quantum Gowdy model: A uniqueness result
- Criteria for the determination of time dependent scalings in the Fock quantization of scalar fields with a time dependent mass in ultrastatic spacetimes
- Nuclearity, Local Quasiequivalence and Split Property for Dirac Quantum Fields in Curved Spacetime
- Fock quantization of a scalar field with time dependent mass on the three-sphere: unitarity and uniqueness
- Quantum unitary evolution of linearly polarized S^1\times S^2 and S^3 Gowdy models coupled to massless scalar fields
- Dirac fields in flat FLRW cosmology: Uniqueness of the Fock quantization
- Fermions in Hybrid Loop Quantum Cosmology
- Unique Fock quantization of a massive fermion field in a cosmological scenario