Emergence of cosmological scaling behavior in asymptotic regime
arXiv:1901.06036 · doi:10.1103/PhysRevD.100.043512
Abstract
In this paper we consider a scalar field system with a class of potentials given by the expression, ; for which as . We carry out dynamical analysis for the underlying system choosing a suitable set of autonomous variables and find all the fixed points. In particular, we show that the scaling solution is an attractor of the system in the asymptotic regime. We indicate the application of the solution to models of quintessential inflation.
arXiv comment20 pages, 9 figures, minor corrections, version to appear in Phys. Rev. D
References in corpus (50)
- Dynamics of dark energy
- Cosmological Imprint of an Energy Component with General Equation of State
- Cosmological Tracking Solutions
- Exponential potentials and cosmological scaling solutions
- Cosmology with a Primordial Scaling Field
- Quintessence: A Review
- Quintessential inflation
- Quintessence arising from exponential potentials
- Structure formation with a self-tuning scalar field
- Cosmological Dynamics of Phantom Field
- Deflationary Universe Scenario
- Aspects of Tachyonic Inflation with Exponential Potential
- Relic Gravity Waves from Braneworld Inflation
- Steep inflation: ending braneworld inflation by gravitational particle production
- Applications of scalar attractor solutions to Cosmology
- Mapping the Cosmological Expansion
- Turning Around the Sphaleron Bound: Electroweak Baryogenesis in an Alternative Post-inflationary Cosmology
- Dark energy, -attractors, and large-scale structure surveys
- Modeling Quintessential Inflation
- Quintessential Inflation with -attractors
- Reheating After Quintessential Inflation and Gravitational Waves
- Variable gravity: A suitable framework for quintessential inflation
- Variable gravity Universe
- Quintessential Inflation on the Brane and the Relic Gravity Wave Background
- Emergent scale symmetry: Connecting inflation and dark energy
- Instant Preheating in Quintessential Inflation with -Attractors
- Quintessential inflation with canonical and noncanonical scalar fields and Planck 2015 results
- Noninteracting dark matter
- From brane assisted inflation to quintessence through a single scalar field
- Unification of inflation and dark energy {\it à la} quintessential inflation
- Observational constraints on successful model of quintessential Inflation
- On the Construction of Quintessential Inflation Models
- Cosmological Scaling Solutions and Multiple Exponential Potentials
- Singular Inflation
- Low-scale Quintessential Inflation
- Generalised Scalar Field Potentials and Inflation
- A Simple Model for Quintessential Inflation
- Tachyonic Quintessential Inflation
- Reheating in quintessential inflation via gravitational production of heavy massive particles: A detailed analysis
- Towards a model of Quintessential Inflation
- Trapped Quintessential Inflation
- Relic gravitational waves from Quintessential Inflation
- Hybrid Quintessential Inflation
- Trapped Quintessential Inflation in the context of Flux Compactifications
- Reconstructing a model of quintessential inflation
- The Equation of State of Tracker Fields
- Different reheating mechanisms in quintessence inflation
- Dark energy and possible alternatives
- Braneworld inflation with effective α-attractor potential
- Quintessential inflation: A unified scenario of inflation and dark energy
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