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Vector theories in cosmology

2009/12/02 by Gilles Esposito-Farèse, Gilles Esposito-Farese, Cyril Pitrou +2 · 127 citations
Mathematics · Physics and Astronomy · #Advanced Differential Geometry Research #Black Holes and Theoretical Physics #Classical mechanics #Cosmology #Cosmology and Gravitation Theories #Curvature #Field (mathematics) #Geometry #Gravitation #Hamiltonian (control theory) #Magnetic field #Mathematical physics #Mathematics #Physics #Pure mathematics #Quantum mechanics #Theoretical physics #Vector field #Vector potential #astro-ph.CO #gr-qc

paper · pdf · doi:10.1103/physrevd.81.063519

published in Physical review. D. Particles, fields, gravitation, and cosmology/Physical review. D. Particles and fields 81(6) (American Physical Society) · 17 pages, no figure

arxiv created 2009/12/02 · openalex publication_date 2010/03/15 · arxiv updated 2010/04/29 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05

Abstract

This article provides a general study of the Hamiltonian stability and the hyperbolicity of vector field models involving both a general function of the Faraday tensor and its dual, f(F2,F\stackrel\texttildelowF), as well as a Proca potential for the vector field, V(A2). In particular it is demonstrated that theories involving only f(F2) do not satisfy the hyperbolicity conditions. It is then shown that in this class of models, the cosmological dynamics always dilutes the vector field. In the case of a nonminimal coupling to gravity, it is established that theories involving Rf(A2) or Rf(F2) are generically pathologic. To finish, we exhibit a model where the vector field is not diluted during the cosmological evolution, because of a nonminimal vector field-curvature coupling which maintains second-order field equations. The relevance of such models for cosmology is discussed.

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