Unitary evolution and uniqueness of the Fock representation of Dirac fields in cosmological spacetimes

Jerónimo Cortez, Beatriz Elizaga Navascués, Mercedes Martín-Benito, Guillermo A. Mena Marugán, and José M. Velhinho
Phys. Rev. D 92, 105013 – Published 6 November 2015

Abstract

We present a privileged Fock quantization of a massive Dirac field in a closed Friedmann–Robertson–Walker cosmology, partially selected by the criteria of invariance of the vacuum under the symmetries of the field equations, and unitary implementation of the dynamics. When quantizing free scalar fields in homogeneous and isotropic spacetimes with compact spatial sections, these criteria have been shown to pick out a unique Fock representation (up to unitary equivalence). Here, we employ the same criteria for fermion fields and explore whether that uniqueness result can be extended to the case of the Fock quantization of fermions. For the massive Dirac field, we start by introducing a specific choice of the complex structure that determines the Fock representation. Such a structure is invariant under the symmetries of the equations of motion. We then prove that the corresponding representation of the canonical anticommutation relations admits a unitary implementation of the dynamics. Moreover, we construct a rather general class of representations that satisfy the above criteria, and we demonstrate that they are all unitarily equivalent to our previous choice. The complex structures in this class are restricted only by certain conditions on their asymptotic behavior for modes in the ultraviolet sector of the Dirac operator. We finally show that, if one assumes that these asymptotic conditions are in fact trivial once our criteria are fulfilled, then the time-dependent scaling in the definition of the fermionic annihilation and creationlike variables is essentially unique.

  • Received 29 September 2015

DOI:https://doi.org/10.1103/PhysRevD.92.105013

© 2015 American Physical Society

Authors & Affiliations

Jerónimo Cortez1,*, Beatriz Elizaga Navascués2,†, Mercedes Martín-Benito3,‡, Guillermo A. Mena Marugán2,§, and José M. Velhinho4,¶

  • 1Departamento de Física, Facultad de Ciencias, Universidad Nacional Autónoma de México, México D.F. 04510, México
  • 2Instituto de Estructura de la Materia, IEM-CSIC, Serrano 121, 28006 Madrid, Spain
  • 3Radboud University Nijmegen, Institute for Mathematics, Astrophysics and Particle Physics, Heyendaalseweg 135, NL-6525 AJ Nijmegen, Netherlands
  • 4Dept. de Física, Universidade da Beira Interior, 6201-001 Covilhã, Portugal

  • *jacq@ciencias.unam.mx
  • beatriz.elizaga@iem.cfmac.csic.es
  • m.martin@hef.ru.nl
  • §mena@iem.cfmac.csic.es
  • jvelhi@ubi.pt

Article Text (Subscription Required)

Click to Expand

References (Subscription Required)

Click to Expand
Issue

Vol. 92, Iss. 10 — 15 November 2015

Reuse & Permissions
Access Options
Author publication services for translation and copyediting assistance advertisement

Authorization Required


×
×

Images

×

Sign up to receive regular email alerts from Physical Review D

Log In

Cancel
×

Search


Article Lookup

Paste a citation or DOI

Enter a citation
×