Inflation driven by scalar field with non-minimal kinetic coupling with Higgs and quadratic potentials
arXiv:1104.2253 · doi:10.1088/1475-7516/2011/04/016
Abstract
We study a scalar field with non-minimal kinetic coupling to itself and to the curvature. The slow rolling conditions allowing an inflationary background have been found. The quadratic and Higgs type potentials have been considered, and the corresponding values for the scalar fields at the end of inflation allows to recover the connection with particle physics.
16 pages, to appear in JCAP
References in corpus (10)
- Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
- Class of viable modified gravities describing inflation and the onset of accelerated expansion
- Vector Inflation
- New models of chaotic inflation in supergravity
- Quintessence and phantom cosmology with non-minimal derivative coupling
- From inflation to dark energy in the non-minimal modified gravity
- Unifying inflation with dark energy in modified F(R) Horava-Lifshitz gravity
- Consequences of a Cosmic Scalar with Kinetic Coupling to Curvature
- SUGRA chaotic inflation and moduli stabilisation
- Gravitational waves in vector inflation