A Jacobian elliptic single-field inflation
arXiv:1505.03096 · doi:10.1140/epjc/s10052-015-3464-z
Abstract
In the scenario of single-field inflation, this field is done in terms of Jacobian elliptic functions. This approach provides, when constrained to particular cases, analytic solutions already known in the past, generalizing them to a bigger family of analytical solutions. The emergent cosmology is analysed using the Hamilton-Jacobi approach and then, the main results are contrasted with the recent measurements obtained from the Planck 2015 data.
7 pages, 5 figures
References in corpus (13)
- A Probe of Primordial Gravity Waves and Vorticity
- Formalising the Slow-Roll Approximation in Inflation
- A limit on the detectability of the energy scale of inflation
- A Hamilton-Jacobi approach to non-slow-roll inflation
- Arbitrary scalar field and quintessence cosmological models
- Inflationary Attractor from Tachyonic Matter
- Inflation on a single brane - exact solutions
- A New Method of Generating Exact Inflationary Solutions
- Approach to exact inflation in modified Friedmann equation
- Single-field inflation à la generalized Chaplygin gas
- Inflation as an attractor in scalar cosmology
- Inflationary Attractor in Braneworld Scenario
- Inflation as a response to protect the Holographic Principle
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- The generalized Chaplygin-Jacobi gas
- Roles of Modified Chaplygin-Jacobi and Chaplygin-Abel Gases in FRW Universe
- Hamilton-Jacobi approach for quasi-exponential inflation: predictions and constraints after Planck 2015 results
- Thermodynamics of Modified Chaplygin-Jacobi Gas and Modified Chaplygin-Abel Gas: Stability Analysis and Observational Constraints
- No slow-roll inflation à la Generalized Chaplygin Gas in General Relativity
- Frame-Dependence of the Hamilton-Jacobi Formalism for Inflation and Reheating in Non-Minimal Gravity
- A Jacobian generalization of the pseudo Nambu-Goldstone bosons potential