The simplest curvaton model
arXiv:astro-ph/0203076 · doi:10.1103/PhysRevD.65.121301
Abstract
We analyze the simplest possible realization of the curvaton scenario, where a nearly scale-invariant spectrum of adiabatic perturbations is generated by conversion of an isocurvature perturbation generated during inflation, rather than the usual inflationary mechanism. We explicitly evaluate all the constraints on the model, under both the assumptions of prompt and delayed reheating, and outline the viable parameter space.
5 pages RevTeX4 file with three figures incorporated
References in corpus (3)
Cited by in corpus (109)
- Seven-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
- Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Cosmological Interpretation
- Planck 2018 results. X. Constraints on inflation
- Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Likelihoods and Parameters from the WMAP data
- Planck 2013 results. XXII. Constraints on inflation
- The Pre-Big Bang Scenario in String Cosmology
- Non-Gaussianity of the primordial perturbation in the curvaton model
- The First Three Seconds: a Review of Possible Expansion Histories of the Early Universe
- Non-Gaussianities in models with a varying inflaton decay rate
- Probing Primordial Non-Gaussianity with Large-Scale Structure
- Review of local non-Gaussianity from multi-field inflation
- Cosmic Density Perturbations from Late-Decaying Scalar Condensations
- Observational constraints on the curvaton model of inflation
- Non-Gaussianity in Curvaton Models with Nearly Quadratic Potential
- The Curvaton as a Pseudo-Nambu-Goldstone Boson
- Constraining Isocurvature Initial Conditions with WMAP 3-year data
- Models of inflation liberated by the curvaton hypothesis
- Curvaton Dynamics
- Adiabatic density perturbations and matter generation from the MSSM
- Curvaton Reheating in Non-oscillatory Inflationary Models
- Stochastic inflation in phase space: Is slow roll a stochastic attractor?
- MSSM flat direction as a curvaton
- Correlation-consistency cartography of the double inflation landscape
- The CDM isocurvature perturbation in the curvaton scenario
- The curvaton scenario in supersymmetric theories
- Can the curvaton paradigm accommodate a low inflation scale?
- The Peccei-Quinn Field as Curvaton
- Curvaton reheating: an application to braneworld inflation
- The stochastic spectator
- Cosmic microwave background anomalies in an open universe
- Conformal Frame Dependence of Inflation
- Resonant decay of flat directions
- Encyclopaedia Curvatonis
- Low-scale Quintessential Inflation
- Primordial non-Gaussianity from two curvaton decays
- MSSM curvaton in the gauge-mediated SUSY breaking
- Isocurvature, non-gaussianity and the curvaton model
- Right-Handed Sneutrinos as Curvatons
- Inflation and non--Gaussianity
- WMAP, neutrino degeneracy and non-Gaussianity constraints on isocurvature perturbations in the curvaton model of inflation
- Curvatons in Supersymmetric Models
- Constraints on primordial isocurvature perturbations and spatial curvature by Bayesian model selection
- Large Scale Structure from the Higgs fields of the Supersymmetric Standard Model
- Curvature and isocurvature perturbations in a three-fluid model of curvaton decay
- Electromagnetic String Fluid in Rolling Tachyon
- Gauge-Invariant Initial Conditions and Early Time Perturbations in Quintessence Universes
- MSSM Higgses as the source of reheating and all matter
- Comprehensive analysis of the simplest curvaton model
- Draining the Swampland
- The trispectrum of the Cosmic Microwave Background on sub-degree angular scales: an analysis of the BOOMERanG data
- Squeezed Bispectrum in the Formalism: Local Observer Effect in Field Space
- Parametric Decay of the Curvaton
- Preheating curvature perturbations with a coupled curvaton
- Curvaton reheating in logamediate inflationary model
- Inflation with an extra light scalar field after Planck
- Superhorizon curvaton amplitude in inflation and pre-big bang cosmology
- A grounded perspective on New Early Dark Energy using ACT, SPT, and BICEP/Keck
- Supersymmetric Curvatons and Phase-Induced Curvaton Fluctuations
- Constraining Curvatonic Reheating
- A Supersymmetric Standard Model of Inflation with Extra Dimensions
- New universal property of cosmological gravitational wave anisotropies
- Scenarios of modulated perturbations
- Constraints on scalar and tensor perturbations in phenomenological and two-field inflation models: Bayesian evidences for primordial isocurvature and tensor modes
- Future constraints on neutrino isocurvature perturbations in the curvaton scenario
- Measuring the duration of inflation with the curvaton
- Correlating CMB Spectral Distortions with Temperature: what do we learn on Inflation?
- Conditions for a Successful Right-Handed Majorana Sneutrino Curvaton
- Tensor Spectra Templates for Axion-Gauge Fields Dynamics during Inflation
- Non-minimally coupled curvaton
- Sneutrino condensate as a candidate for the hot big bang cosmology
- A spherically symmetric and stationary universe from a weak modification of general relativity
- Fermionic Isocurvature Perturbations
- Non-Gaussianity in three fluid curvaton model
- Generic inference of inflation models by non-Gaussianity and primordial power spectrum reconstruction
- Curvaton Scenario with Affleck-Dine Baryogenesis
- Sgoldstino-less inflation and low energy SUSY breaking
- Extended Curvaton reheating in inflationary models
- Inhomogeneous reheating scenario with low scale inflation and/or MSSM flat directions
- Tracking Curvaton(s)?
- Non-Gaussianity and constraints for the variance of perturbations in the curvaton model
- Searching for non-Gaussianity in the VSA data
- Completing magnetic field generation from gravitationally coupled electrodynamics with the curvaton mechanism
- Bayesian evidence of the post-Planck curvaton
- Stochastic inflation and primordial black holes
- What Planck does not tell us about inflation
- Multiple spectator condensates from inflation
- Coupling structure of multi-field primordial perturbations
- Constraints from CMB in the intermediate Brans-Dicke inflation
- Brane-Antibrane Systems at Finite Temperature and Phase Transition near the Hagedorn Temperature
- Curvaton Potential Terms, Scale-Dependent Perturbation Spectra and Chaotic Initial Conditions
- Generation of perturbation after multi-field inflation
- Curvaton preheating revisited
- Curvaton scenarios with inflaton decays into curvatons
- The running curvaton
- The Effect of Curvaton Decay on the Primordial Power Spectrum
- Primordial black holes from the ultraslow-roll phase in the inflaton--curvaton mixed field inflation
- Curvaton and quantum gravity effect on the tensor to scalar ratio of the chaotic inflation
- A model of cosmology and particle physics at an intermediate scale
- Mixed perturbations from an Inflaton and Two Curvatons - towards understanding non-gaussianity in more complicated curvaton scenarios
- CMB lensing forecasts for constraining the primordial perturbations: adding to the CMB temperature and polarization information
- Primordial black holes from a curvaton: the role of bimodal distributions
- Curvaton decay into relativistic matter
- Curvaton: Perturbations and reheating
- Flat Direction Dynamics in a Non-Topological Soliton-Dominated Universe
- Stabilising the Planck mass shortly after inflation
- Spectator fields and their imprints on the Cosmic Microwave Background
- Curvaton mechanism and its implications to sneutrino cosmology
- Generic inference of inflation models by local non-Gaussianity
- Testing Inflationary Cosmology