An effective fluid description of scalar-vector-tensor theories under the sub-horizon and quasi-static approximations
DOI10.1088/1475-7516/2022/08/059OpenAlexW4293168164WikidataQ114096384 ScholiaQ114096384MaRDI QIDQ5104182
J. Bayron Orjuela-Quintana, Wilmar Cardona, César A. Valenzuela-Toledo
Publication date: 9 September 2022
Published in: Journal of Cosmology and Astroparticle Physics (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2206.02895
modified gravitydark energy theoryGauss-Bonnet-Lovelock-Horndeski-Palatini etc. gravity theoriescosmological perturbation theory in GR and beyond
Relativistic cosmology (83F05) Anisotropy in solid mechanics (74E10) Spectrum, resolvent (47A10) Hydro- and aero-acoustics (76Q05) Stress (74A10) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Perturbations in context of PDEs (35B20) Matrix models and tensor models for quantum field theory (81T32) Dark matter and dark energy (83C56)
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Cites Work
- Unnamed Item
- Cosmic acceleration from abelian symmetry breaking
- Derivative self-interactions for a massive vector field
- The MESS of cosmological perturbations
- Cosmology of a scalar field coupled to matter and an isotropy-violating Maxwell field
- Dark energy cosmology: the equivalent description via different theoretical models and cosmography tests
- Inflation in a scalar-vector-tensor theory
- Generalized G-Inflation: --Inflation with the Most General Second-Order Field Equations--
- A Cyclic Model of the Universe
- DYNAMICS OF DARK ENERGY
- INTRODUCTION TO MODIFIED GRAVITY AND GRAVITATIONAL ALTERNATIVE FOR DARK ENERGY
- A general theory of linear cosmological perturbations: stability conditions, the quasistatic limit and dynamics
- Scalar-vector-tensor gravity theories
- Dark energy in scalar-vector-tensor theories
- Proca in the sky
- Comparison of different approaches to the quasi-static approximation in Horndeski models
- Coupled vector dark energy
- Anisotropic Einstein Yang-Mills Higgs dark energy
- Cosmological constraints on sub-horizon scales modified gravity theories with MGCLASS II
- Einstein Yang–Mills Higgs dark energy revisited
- Dark energy in Horndeski theories after GW170817: A review
- The cosmological constant problem
- Dark sector evolution in Horndeski models
- The cosmological constant
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