Shapes of non-Gaussianity in warm inflation
arXiv:2205.13227 · doi:10.1088/1475-7516/2023/02/012
Abstract
Sphaleron heating has been recently proposed as a mechanism to realize warm inflation when inflaton is an axion coupled to pure Yang-Mills. As a result of heating, there is a friction coefficient in the equation of motion for the inflaton, and a thermal contribution to cosmological fluctuations. Without the knowledge of the inflaton potential, non-Gaussianity is the most promising way of searching for the signatures of this model. Building on an earlier work by Bastero-Gil, Berera, Moss and Ramos, we compute the scalar three-point correlation function and point out some distinct features in the squeezed and folded limits. As a detection strategy, we show that the combination of the equilateral template and one new template has a large overlap with the shape of non-Gaussianity over the range , and in this range .
v2: JCAP version, 35 pages, 9 figures, extra refs and comments with respect to v1
References in corpus (10)
- The Sphaleron Rate in SU(N) Gauge Theory
- Trapped Inflation
- Chiral Anomaly, Schwinger Effect, Euler-Heisenberg Lagrangian, and application to axion inflation
- Theory of non-Gaussianity in warm inflation
- Gravitational Waves and the Scale of Inflation
- Thermalized Axion Inflation
- Gravitational wave background from non-Abelian reheating after axion-like inflation
- Warming up cold inflation
- Higher N-point function data analysis techniques for heavy particle production and WMAP results
- The spectrum of tensor perturbations in warm inflation
Cited by in corpus (20)
- Recent developments in warm inflation
- The warm inflation story
- The Open Effective Field Theory of Inflation
- Gravitational wave background from vacuum and thermal fluctuations during axion-like inflation
- Warm Inflation with the Standard Model
- Viability of warm inflation with standard model interactions
- WI2easy: warm inflation dynamics made easy
- Warm inflation with a heavy QCD axion
- Revisiting Isocurvature Bounds on the Minimal QCD Axion
- Primordial Black Holes Dark Matter and Secondary Gravitational Waves from Warm Higgs-G Inflation
- Evolution of coupled scalar perturbations through smooth reheating. I. Dissipative regime
- On Sphaleron Heating in the Presence of Fermions
- Non-Gaussianity in the warm k-inflation
- Evolution of coupled scalar perturbations through smooth reheating. II. Thermal fluctuation regime
- CMB bispectrum constraints on DHOST inflation
- Witten-O'Raifeartaigh potential revisited in the context of Warm Inflation
- Primordial non-Gaussianity in noncanonical warm inflation with nonminimal derivative coupling
- Not So Minimal Warm Inflation
- AliCPT Sensitivity to Cosmic Reheating
- Classical equipartition dynamics between axions and non-Abelian gauge fields