Fermionic alpha-vacua
arXiv:hep-th/0410229 · doi:10.1103/PhysRevD.71.024002
Abstract
A spin one-half particle propagating in a de Sitter background has a one parameter family of states which transform covariantly under the isometry group of the background. These states are the fermionic analogues of the alpha-vacua for a scalar field. We shall show how using a point-source propagator for a fermion in an alpha-state produces divergent perturbative corrections. These corrections cannot be used to cancel similar divergences arising from scalar fields in bosonic alpha-vacua since they have an incompatible dependence on the external momenta. The theory can be regularized by modifying the propagator to include an antipodal source.
13 pages, 3 eps figures, uses RevTeX
Cited by in corpus (14)
- Fermion production during and after axion inflation
- Renormalization of initial conditions and the trans-Planckian problem of inflation
- Time-dependent spacetimes in AdS/CFT: Bubble and black hole
- Trans-Planckian signals from the breaking of local Lorentz invariance
- Emergent -like fermionic vacuum structure and entanglement in the hyperbolic de Sitter spacetime
- Some measures for fermionic entanglement in the cosmological de Sitter spacetime
- Alpha-Vacua, Black Holes, and AdS/CFT
- Probing Planckian physics in de Sitter space with quantum correlations
- Uniqueness Criteria for the Fock Quantization of Dirac Fields and Applications in Hybrid Loop Quantum Cosmology
- Accelerated paths and Unruh effect II: finite time detector response in (Anti) de Sitter spacetime and Huygen's Principle
- Unique fermionic vacuum in de Sitter spacetime from hybrid quantum cosmology
- Fluctuations in the stress energy tensor of spinor fields evolving in general FRW spacetimes
- Spinor Green's functions via spherical means on products of space forms
- Probing Alpha-Vacua of Black Holes in LHC