Cosmology of extended proca-nuevo

• Verfasst von: Rham, Claudia de [VerfasserIn]
• Verfasst von: Garcia-Saenz, Sebastian [VerfasserIn]
• Verfasst von: Heisenberg, Lavinia [VerfasserIn]
• Verfasst von: Pozsgay, Victor [VerfasserIn]
• Titel: Cosmology of extended proca-nuevo
• Verf.angabe: Claudia de Rham, Sebastian Garcia-Saenz, Lavinia Heisenberg, Victor Pozsgay
• E-Jahr: 2022
• Jahr: March 23, 2022
• Umfang: 50 S.
• Fussnoten: Gesehen am 29.06.2022
• Titel Quelle: Enthalten in: Journal of cosmology and astroparticle physics
• Ort Quelle: London : IOP, 2003
• Jahr Quelle: 2022
• Band/Heft Quelle: (2022), 3, Artikel-ID 053, Seite 1-50
• ISSN Quelle: 1475-7516
• DOI: doi:10.1088/1475-7516/2022/03/053
• Datenträger: Online-Ressource
• Sprache: eng
• K10plus-PPN: 1808536177

Abstract

Proca-Nuevo is a non-linear theory of a massive spin-1 field which enjoys a non-linearly realized constraint that distinguishes it among other generalized vector models. We show that the theory may be extended by the addition of operators of the Generalized Proca class without spoiling the primary constraint that is necessary for consistency, allowing to interpolate between Generalized Proca operators and Proca-Nuevo ones. The constraint is maintained on flat spacetime and on any fixed curved background. Upon mixing extended Proca-Nuevo dynamically with gravity, we show that the constraint gets broken in a Planck scale suppressed way. We further prove that the theory may be covariantized in models that allow for consistent and ghost-free cosmological solutions. We study the models in the presence of perfect fluid matter, and show that they describe the correct number of dynamical variables and derive their dispersion relations and stability criteria. We also exhibit, in a specific set-up, explicit hot Big Bang solutions featuring a late-time self-accelerating epoch, and which are such that all the stability and subluminality conditions are satisfied and where gravitational waves behave precisely as in General Relativity.