A New Method of Generating Exact Inflationary Solutions
arXiv:gr-qc/9407041 · doi:10.1103/PhysRevD.50.4794
Abstract
The mechanism of the initial inflation of the universe is based on gravitationally coupled scalar fields . Various scenarios are distinguished by the choice of an {\it effective self--interaction potential} which simulates a {\it temporarily} non--vanishing {\em cosmological term}. Using the Hubble expansion parameter as a new ``time" coordinate, we can formally derive the {\it general} Robertson--Walker metric for a {\em spatially flat} cosmos. Our new method provides a classification of allowed inflationary potentials and is broad enough to embody all known {\it exact} solutions involving one scalar field as special cases. Moreover, we present new inflationary and deflationary exact solutions and can easily predict the influence of the form of on density perturbations.
32 pages, REVTeX, 9 postscript figures (or hardcopy) available upon request, Cologne-thp-1994-H8
References in corpus (11)
- Metric-Affine Gauge Theory of Gravity: Field Equations, Noether Identities, World Spinors, and Breaking of Dilation Invariance
- Hybrid Inflation
- False Vacuum Inflation with Einstein Gravity
- COBE, Gravitational Waves, Inflation and Extended Inflation
- Inflation Deflation and Frame-Independence in String Cosmology
- Perturbation Spectra from Intermediate Inflation
- Reconstructing the Inflaton Potential---in Principle and in Practice
- Gravitational Stability of Boson Stars
- Spin-driven inflation
- Recent advances in extended inflationary cosmology
- The massive scalar field in a closed Friedmann universe model - new rigorous results
Cited by in corpus (26)
- Metric-Affine Gauge Theory of Gravity: Field Equations, Noether Identities, World Spinors, and Breaking of Dilation Invariance
- Inflationary Models with Logarithmic Potentials
- Assisted Tachyonic Inflation
- Tree-level String Cosmology
- Arbitrary scalar field and quintessence cosmological models
- Dynamical instability of fluid spheres in the presence of a cosmological constant
- Cosmology with exponential potentials
- Why Does Gravity Ignore the Vacuum Energy?
- Cornell Potential: A Neural Network Approach
- The method of generating functions in exact scalar field cosmology
- The generalized Chaplygin-Jacobi gas
- Decoupling of the general scalar field mode and the solution space for Bianchi type I and V cosmologies coupled to perfect fluid sources
- Reconstructing the inflaton potential for an almost flat COBE spectrum
- Shear-free rotating inflation
- Jacobi stability analysis of scalar field models with minimal coupling to gravity in a cosmological background
- Classification of Inflationary Einstein--Scalar--Field--Models via Catastrophe Theory
- Multi-fluid cosmology in Einstein gravity: analytical solutions
- Self-interacting scalar field cosmologies: unified exact solutions and symmetries
- Bianchi V inflation in the Brans-Dicke theory?
- Another exact inflationary solution
- A Jacobian elliptic single-field inflation
- Period-doubling bifurcation in strongly anisotropic Bianchi I quantum cosmology
- The Andante Regime of Scalar Field Dynamics
- Thermodynamics of Modified Chaplygin-Jacobi Gas and Modified Chaplygin-Abel Gas: Stability Analysis and Observational Constraints
- Exact inflationary solutions
- Eigenvalues of the Stewart-Lyth equation for inflation with a blue spectrum