Effects of particle production during inflation
arXiv:0809.5142 · doi:10.1103/PhysRevD.78.103522
Abstract
The impact of particle production during inflation on the primordial curvature perturbation spectrum is investigated both analytically and numerically. We obtain an oscillatory behavior on small scales, while on large scales the spectrum is unaffected. The amplitude of the oscillations is proportional to the number of coupled fields, their mass, and the square of the coupling constant. The oscillations are due a discontinuity in the second time derivative of the inflaton, arising from a temporary violation of the slow-roll conditions. A similar effect on the power spectrum should be produced also in other inflationary models where the slow-roll conditions are temporarily violated.
7 pages, 5 figures
References in corpus (10)
- First Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Determination of Cosmological Parameters
- Wilkinson Microwave Anisotropy Probe (WMAP) Three Year Results: Implications for Cosmology
- Inflationary perturbations from a potential with a step
- Probing Planckian physics: resonant production of particles during inflation and features in the primordial power spectrum
- Enhancement of superhorizon scale inflationary curvature perturbations
- New Universal Local Feature in the Inflationary Perturbation Spectrum
- The CMB Quadrupole depression produced by early fast-roll inflation: MCMC analysis of WMAP and SDSS data
- CMB quadrupole suppression: II. The early fast roll stage
- Breaking scale invariance from a singular inflaton potential
- Observational constraints on particle production during inflation
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- Primordial feature constraints from BOSS+eBOSS
- Effects of local features of the inflaton potential on the spectrum and bispectrum of primordial perturbations
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- Cosmological Particle Production and Pairwise Hotspots on the CMB
- Explaining low l anomalies in the CMB power spectrum with resonant superstring excitations during inflation
- Possible Evidence for Planck-Scale Resonant Particle Production during Inflation from the CMB Power Spectrum
- Enhanced Preheating after Multi-Field Inflation: On the Importance of being Special
- Particle Production during Inflation in Light of PLANCK
- Jump in fluid properties of inflationary universe to reconcile scalar and tensor spectra
- Particle production during Inflation with a non-minimally coupled spectator scalar field
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