Bumpy inflation from explosive particle production
Abstract
We present a first-principles derivation of an effective inflaton potential with a bumpy feature. We consider the coupling of a spectator field χto the inflaton ϕsuch that χis massive enough for almost all values of ϕ, but becomes massless when the inflaton crossed the value ϕ_\star. This gives rise to a burst of χ-particle production at ϕ=ϕ_\star. By taking the backreaction of the particle production, we obtain a bumpy feature in the effective potential. We discover that for certain choices of the interaction constants and field scale relevant for particle production, the backreaction-induced bumpy effective potential can lead to a sizable enhancement in the curvature perturbation. In particular, the enhancement can be large enough to generate observationally relevant amounts of primordial black holes and stochastic gravitational wave backgrounds.
Related
- Gravitational Dark Matter Production from Spectator Field in R2-Higgs Inflation
- Particle production from bubble collisions
- Tachyonic particle production in strongly supercooled phase transitions
- On Particle Production from Bubble Collisions in the Non-runaway Regime
- ALMA Reveals an Explosive Outflow Candidate in IRAS 16119--5048
BibTeX
@misc{lozanov2026bumpy,
title = {{Bumpy inflation from explosive particle production}},
author = {Kaloian D. Lozanov and Xavier Pritchard and Misao Sasaki},
howpublished = {arXiv},
year = {2026},
month = sep,
doi = {10.48550/arxiv.2608.26920},
eprint = {2608.26920},
archivePrefix = {arXiv},
url = {https://arxiv.org/abs/2608.26920},
note = {CC BY 4.0},
}
RIS
TY - UNPB
TI - Bumpy inflation from explosive particle production
AU - Kaloian D. Lozanov
AU - Xavier Pritchard
AU - Misao Sasaki
PY - 2026
DA - 2026/09/11
PB - arXiv
DO - 10.48550/arxiv.2608.26920
UR - https://arxiv.org/abs/2608.26920
AB - We present a first-principles derivation of an effective inflaton potential with a bumpy feature. We consider the coupling of a spectator field χto the inflaton ϕsuch that χis massive enough for almost all values of ϕ, but becomes massless when the inflaton crossed the value ϕ_\star. This gives rise to a burst of χ-particle production at ϕ=ϕ_\star. By taking the backreaction of the particle production, we obtain a bumpy feature in the effective potential. We discover that for certain choices of the interaction constants and field scale relevant for particle production, the backreaction-induced bumpy effective potential can lead to a sizable enhancement in the curvature perturbation. In particular, the enhancement can be large enough to generate observationally relevant amounts of primordial black holes and stochastic gravitational wave backgrounds.
ER -