Inflation in a scalar-vector-tensor theory

DOI10.1007/S10714-022-02901-YzbMath1484.83147arXiv2201.03629OpenAlexW4206215405MaRDI QIDQ2667399

A. Oliveros, Cristhian J. Rodríguez

Publication date: 4 March 2022

Published in: General Relativity and Gravitation (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/2201.03629

zbMATH Keywords

inflationcosmologylinear cosmological perturbationsno-ghosts and stability conditionsscalar-vector-tensor theories

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Classes of solutions; algebraically special solutions, metrics with symmetries for problems in general relativity and gravitational theory (83C20) Foliations (differential geometric aspects) (53C12) Equations of motion in general relativity and gravitational theory (83C10) Lagrangian formalism and Hamiltonian formalism in mechanics of particles and systems (70S05) Propagation of singularities; initial value problems on manifolds (58J47) Matrix models and tensor models for quantum field theory (81T32)

Related Items (2)

Odd-parity perturbations in the most general scalar–vector–tensor theory ⋮ An effective fluid description of scalar-vector-tensor theories under the sub-horizon and quasi-static approximations

Cites Work

• Superconformal inflationary \(\alpha\)-attractors
• Gauge fields and inflation
• Hairy black hole solutions in \(U(1)\) gauge-invariant scalar-vector-tensor theories
• Modified gravity theories on a nutshell: inflation, bounce and late-time evolution
• A new type of isotropic cosmological models without singularity
• Cosmological Inflation and Large-Scale Structure
• Scalar-vector-tensor gravity theories
• Dark energy in scalar-vector-tensor theories
• Late-time cosmology of scalar-coupled f(R,G) gravity
• Inflationary universe: A possible solution to the horizon and flatness problems

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