What happens when the inflaton stops during inflation
arXiv:astro-ph/9911119 · doi:10.1103/PhysRevD.61.103504
Abstract
The spectrum of adiabatic density perturbation generated during inflation is studied in the case the time derivative of an inflation-driving scalar field (inflaton) vanishes at some time during inflation. It is shown that the nondecaying mode of perturbation has a finite value even in this case and that its amplitude is given by the standard formula with the time derivation of the scalar field replaced by the potential gradient using the slow-roll equation.
References in corpus (1)
Cited by in corpus (31)
- Horizon crossing and inflation with large η
- Ultra Slow-Roll Inflation and the non-Gaussianity Consistency Relation
- Enhancement of superhorizon scale inflationary curvature perturbations
- Primordial Black Holes from Inflation and Quantum Diffusion
- Stochastic growth of quantum fluctuations during slow-roll inflation
- Loop quantum gravity effects on inflation and the CMB
- Inflationary perturbations near horizon crossing
- Curvature perturbation at the local extremum of the inflaton's potential
- Axion inflation with gauge field production and primordial black holes
- Implications of stochastic effects for primordial black hole production in ultra-slow-roll inflation
- An analytic approach to non-slow-roll inflation
- On the constant-roll inflation
- The attractive behaviour of ultra-slow-roll inflation
- Nonlinear superhorizon perturbations in Horava-Lifshitz gravity
- What do WMAP and SDSS really tell about inflation?
- Warm inflation in loop quantum cosmology: a model with a general dissipative coefficient
- Non-Gaussianity of superhorizon curvature perturbations beyond N formalism
- Pre - Inflationary Clues from String Theory ?
- A new mechanism to enhance primordial tensor fluctuations in single field inflation
- Slow roll in simple non-canonical inflation
- Making waves on CMB power spectrum and inflaton dynamics
- The observational constraint on constant-roll inflation
- Sudden braking and turning with a two-field potential bump: primordial black hole formation
- Ambiguity in running spectral index with an extra light field during inflation
- Full nonlinear growing and decaying modes of superhorizon curvature perturbations
- Stochastic inflation and primordial black holes
- Curvatons and inhomogeneous scenarios with deviation from slow-roll
- On the Hamilton-Jacobi approach to inflation beyond slow roll
- What we can learn from the spectral index of the tensor mode
- Inflation: a quantum laboratory on cosmological scales
- Wronskian Formulation of the Spectrum of Curvature Perturbations