A new solution for inflation
arXiv:physics/0006030 · doi:10.1119/1.1290250
Abstract
Many pedagogical introductions of cosmological inflation are effective due to the simplicity of the relevant equations. Here an analytic solution of the cosmological equations is presented and used as an example to discuss fundamental aspects of the inflationary paradigm.
14 pages, LaTeX, to appear in Am. J. Phys
References in corpus (3)
Cited by in corpus (15)
- Superquintessence
- Non-Gaussian tail of the curvature perturbation in stochastic ultra-slow-roll inflation: implications for primordial black hole production
- Planck scale black hole dark matter from Higgs inflation
- Imperfect fluid description of modified gravities
- The correspondence between a scalar field and an effective perfect fluid
- Critical point Higgs inflation in the Palatini formulation
- Cosmological dynamics with non-minimally coupled scalar field and a constant potential function
- Primordial black hole compaction function from stochastic fluctuations in ultra-slow-roll inflation
- Inflationary Cosmologies in an Anisotropic Brane World
- From model dynamics to oscillating dark energy parameterisation
- Multi-fluid cosmology in Einstein gravity: analytical solutions
- A new symmetry of the spatially flat Einstein-Friedmann equations
- On Non-triviality of Units Transformations
- The harmonic oscillator, dimensional analysis and inflationary solutions
- Effect of stochastic kicks on primordial black hole abundance and mass via the compaction function