Hill crossing during preheating after hilltop inflation
arXiv:1503.06075 · doi:10.1088/1475-7516/2015/06/009
Abstract
In 'hilltop inflation', inflation takes place when the inflaton field slowly rolls from close to a maximum of its potential (i.e. the 'hilltop') towards its minimum. When the inflaton potential is associated with a phase transition, possible topological defects produced during this phase transition, such as domain walls, are efficiently diluted during inflation. It is typically assumed that they also do not reform after inflation, i.e. that the inflaton field stays on its side of the 'hill', finally performing damped oscillations around the minimum of the potential. In this paper we study the linear and the non-linear phases of preheating after hilltop inflation. We find that the fluctuations of the inflaton field during the tachyonic oscillation phase grow strong enough to allow the inflaton field to form regions in position space where it crosses 'over the top of the hill' towards the 'wrong vacuum'. We investigate the formation and behaviour of these overshooting regions using lattice simulations: Rather than durable domain walls, these regions form oscillon-like structures (i.e. localized bubbles that oscillate between the two vacua) which should be included in a careful study of preheating in hilltop inflation.
arXiv comment22 pages, 10 figures, v2 matches publication in JCAP. Animated movies of our simulations are available online at https://particlesandcosmology.unibas.ch/files/hilltop_preheating.html
References in corpus (28)
- The 6dF Galaxy Survey: Baryon Acoustic Oscillations and the Local Hubble Constant
- The clustering of galaxies in the SDSS-III Baryon Oscillation Spectroscopic Survey: Baryon Acoustic Oscillations in the Data Release 10 and 11 galaxy samples
- The Clustering of the SDSS DR7 Main Galaxy Sample I: A 4 per cent Distance Measure at z=0.15
- A Joint Analysis of BICEP2/Keck Array and Planck Data
- Semiclassicality and Decoherence of Cosmological Perturbations
- Hilltop Inflation
- Classical decay of inflaton
- Oscillons: Resonant Configurations During Bubble Collapse
- Topological Inflation
- Oscillons After Inflation
- LATTICEEASY: A Program for Lattice Simulations of Scalar Fields in an Expanding Universe
- Gravitational Waves from Oscillon Preheating
- More hilltop inflation models
- Natural New Inflation in Broken Supergravity
- New inflation, preinflation, and leptogenesis
- End of inflation, oscillons and matter-antimatter asymmetry
- Dynamical Tuning of the Initial Condition for New Inflation in Supergravity
- Emergence of Oscillons in an Expanding Background
- Transition To Order After Hilltop Inflation
- Unnatural Oscillon Lifetimes in an Expanding Background
- Preheating in New Inflation
- Smooth hybrid inflation in supergravity with a running spectral index and early star formation
- Long-lived oscillons from asymmetric bubbles
- Resonant nucleation of spatio-temporal order via parametric modal amplification
- Flavon Inflation
- Preheating after Small-Field Inflation
- Hilltop inflation with preinflation from coupling to matter fields
- Exploring Two-Field Inflation in the Wess-Zumino Model
Cited by in corpus (20)
- Cosmological Backgrounds of Gravitational Waves
- The art of simulating the early Universe -- Part I
- Gravitational waves from oscillons after inflation
- Oscillons from String Moduli
- Gravitational wave forest from string axiverse
- What can we learn from the stochastic gravitational wave background produced by oscillons?
- Characterizing the post-inflationary reheating history, Part I: single daughter field with quadratic-quadratic interaction
- Properties of oscillons in hilltop potentials: energies, shapes, and lifetimes
- Impact of other scalar fields on oscillons after hilltop inflation
- Parametric resonance after hilltop inflation caused by an inhomogeneous inflaton field
- Irreversible thermodynamical description of warm inflationary cosmological models
- Electroweak Vacuum Metastability and Low-scale Inflation
- The Linear Regime of Tachyonic Preheating
- The -Higgs inflation: contribution and preheating after ACT and SPT data
- Non-thermal Leptogenesis after Majoron Hilltop Inflation
- Supersymmetric Majoron Inflation
- Ephemeral Oscillons in Scalar-Tensor Theories: The Higgs-like case
- A model with two periods of inflation
- Preheating and gravitational waves in large-field hilltop inflation
- The -Higgs inflation with two Higgs doublets