HYM-flation: Yang-Mills cosmology with Horndeski coupling
arXiv:1512.02164 · doi:10.1016/j.physletb.2015.12.070
Abstract
We propose new mechanism for inflation using classical SU(2) Yang-Mills (YM) homogeneous and isotropic field non-minimally coupled to gravity via Horndeski prescription. This is the unique generally and gauge covariant ghost-free YM theory with the curvature-dependent action leading to second-order gravity and Yang-Mills field equations. We show that its solution space contains de Sitter boundary to which the trajectories are attracted for some finite time, ensuring the robust inflation with a graceful exit. The theory can be generalized to include the Higgs field leading to two-steps inflationary scenario, in which the Planck-scale YM-generated inflation naturally prepares the desired initial conditions for the GUT-scale Higgs inflation.
13 pages, 3 figures
References in corpus (12)
- The Standard Model Higgs boson as the inflaton
- The Unity of Cosmological Attractors
- Higgs inflation still alive
- Inflationary cosmology and the late-time accelerated expansion of the universe in non-minimal Yang-Mills- gravity and non-minimal vector- gravity
- Cosmological Attractors and Initial Conditions for Inflation
- Higgs inflation from Standard Model criticality
- Dark energy as a fixed point of the Einstein Yang-Mills Higgs Equations
- Effective metrics in the non-minimal Einstein-Yang-Mills-Higgs theory
- Cosmological consequences of classical flavor-space locked gauge field radiation
- Chiral Imprint of a Cosmic Gauge Field on Primordial Gravitational Waves
- Nonminimal isotropic cosmological model with Yang-Mills and Higgs fields
- Early and Late-time Cosmic Acceleration in Non-minimal Yang-Mills- Gravity
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- Constant-roll inflation in the generalized SU(2) Proca theory
- Non-trivial gravitational waves and structure formation phenomenology from dark energy
- Instabilities in Horndeski Yang-Mills inflation
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- Inflation driven by massive vector fields with derivative self-interactions
- Comparing metric and Palatini approaches to vector Horndeski theory
- Magnetic and Electric Black Holes in the Vector-Tensor Horndeski Theory
- Inflation with mixed helicities and its observational imprint on CMB