The primordial density perturbation in the curvaton scenario
arXiv:astro-ph/0208055 · doi:10.1103/PhysRevD.67.023503
Abstract
We analyse the primordial density perturbation when it is generated by a `curvaton' field different from the inflaton. In some cases this perturbation may have large isocurvature components, fully correlated or anti-correlated with the adiabatic component. It may also have a significant non-Gaussian component. All of these effects are calculated in a form which will enable direct comparison with current and forthcoming observational data.
13 pages, latex with revtex, no figures; v2 caveat added to calculation of isocurvature perturbations in section IV; v3 minor corrections, references added, to appear in Phys Rev D
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- Revisiting non-Gaussianity of multiple-field inflation from the field equation
- Mixed inflaton and curvaton scenario with sneutrinos
- Extended analysis of CMB constraints on non-Gaussianity in isocurvature perturbations
- Could the next generation of cosmology experiments exclude supergravity?
- Curvaton and the inhomogeneous end of inflation
- Anisotropic Massive Gauge-flation
- Cosmological constraints on the curvaton web parameters
- Curvaton Dynamics in Brane-worlds
- Inflaton or Curvaton? Constraints on Bimodal Primordial Spectra from Mixed Perturbations
- Wigner-Eckart theorem in cosmology: Bispectra for total-angular-momentum waves
- Uncorrelated Compensated Isocurvature Perturbations from kSZ Tomography
- How the curvaton scenario, modulated reheating and an inhomogeneous end of inflation are related
- A new bound on the low reheating temperature with dark matter
- Modulated reheating by curvaton
- Adiabatic versus Isocurvature Non--Gaussianity
- Non-Gaussianity from false vacuum inflation: Old curvaton scenario
- Higgs Boson in RG running Inflationary Cosmology
- Probing new physics with multi-vacua quantum tunnelings beyond standard model through gravitational waves
- Impact of the 1/f noise and the asymmetric beam on non-Gaussianity searches with Planck
- Primordial Black Holes from Pre-Big Bang inflation
- BBN constraints on dark radiation isocurvature
- Non-Gaussian bubbles in the sky
- Non-Gaussianity and gravitational wave background in curvaton with a double well potential
- Constraints on primordial non-Gaussianity from WMAP7 and Luminous Red Galaxies power spectrum and forecast for future surveys
- Probing local non-Gaussianities within a Bayesian framework
- Computing First-Passage Times with the Functional Renormalisation Group
- A weak lensing view on primordial non-Gaussianities
- Freeze-in Dark Matter Perturbations are Adiabatic
- Fully non-linear equivalence of delta N and covariant formalisms
- Primordial Black Holes without fine-tuning from a light stochastic spectator field
- Effect of intermediate Minkowskian evolution on CMB bispectrum
- Curvaton Decay into Baryons, anti-Baryons and Radiation
- CDM/baryon isocurvature perturbations in a sneutrino curvaton model
- Non-Gaussianity in rapid-turn multi-field inflation
- Sneutrinos as Mixed Inflaton and Curvaton
- Cosmic Perturbations from a Rotating Field
- Suppressed Non-Gaussianity in the Curvaton Model
- Single-Field Inflation and the Local Ansatz: Distinguishability and Consistency
- Different approaches to the second order Klein-Gordon equation
- The Origin of the Large-Scale Structure in the Universe: Theoretical and Statistical Aspects
- Statistics of the excursion sets in models with local primordial non-Gaussianity
- Cosmological Constraints on Rapid Roll Inflation
- Inflationary parameters and primordial perturbation spectra
- An improved estimator for non-Gaussianity in cosmic microwave background observations
- Hubble induced mass after inflation in spectator field models
- Spectral Index and Non-Gaussianity in Supersymmetric Hybrid Inflation
- A falsely fat curvaton with an observable running of the spectral tilt
- Planck constraints on neutrino isocurvature density perturbations
- Curvaton Potential Terms, Scale-Dependent Perturbation Spectra and Chaotic Initial Conditions
- Local Scale-Dependent Non-Gaussian Curvature Perturbations at Cubic Order
- Cosmological perturbations from a Spectator field during inflation
- Removing Interlopers From Intensity Mapping Probes Of Primordial Non-Gaussianity
- Revised parameter in Curvaton Scenario
- Thermal non-Gaussianity in Near-Milne universe
- Interpreting Pulsar Timing Array data of Gravitational Waves with Ekpyrosis-Bouncing Cosmology
- Curvaton scenarios with inflaton decays into curvatons
- Nambu-Goldstone Affleck-Dine Baryogenesis
- New natural shapes of non-Gaussianity from high-derivative interactions and their optimal limits from WMAP 9-year data
- Generating cosmological perturbations with mass variations
- Resolving primordial physics through correlated signatures
- Creating perturbations from a decaying field during inflation
- The TeV-mass curvaton
- Constraints on Non-Gaussianity from Sunyaev--Zeldovich Cluster Surveys
- A bulk inflaton from large volume extra dimensions
- Generation of perturbation after multi-field inflation
- Curvaton reheating in non-minimal derivative coupling to gravity: NO models
- Affleck-Dine baryogenesis with modulated reheating
- The running curvaton
- Isocurvature initial conditions for second order Boltzmann solvers
- Refined Study of Isocurvature Fluctuations in the Curvaton Scenario
- The moduli problem at the perturbative level
- Mimetic Curvaton
- Density perturbations from both the inflaton and the curvaton
- Radiative corrections to scalar masses in de Sitter space
- What We Can Learn from the Running of the Spectral Index if no Tensors are Detected in the Cosmic Microwave Background Anisotropy
- Isocurvature modes: joint analysis of the CMB power spectrum and bispectrum
- Detecting the dark sector through scalar-induced gravitational waves
- Probing Lepton Asymmetry with 21 cm Fluctuations
- The Effect of Curvaton Decay on the Primordial Power Spectrum
- Volume Weighting the Measure of the Universe from Classical Slow-Roll Expansion
- Lensing Bias to CMB Polarization Measurements of Compensated Isocurvature Perturbations
- Adiabatic and non-adiabatic perturbations for loop quantum cosmology
- Non-Gaussian assembly bias from a semi-analytic galaxy formation model
- Axion-CMB Scenario in Supercooled Universe
- Magnetic Fields from Compensated Isocurvature Perturbations
- The interplay of CMB temperature lensing power reconstruction with primordial non-Gaussianity of local type
- Entropy production and curvature perturbation from dissipative curvatons
- Cosmic perturbations, baryon asymmetry and dark matter from the minimal supersymmetric standard model
- Non-Gaussianities and Primordial Black Holes
- Affleck-Dine baryogenesis in inflating curvaton scenario with O(TeV) mass moduli curvaton
- Theories of gravity with nonminimal matter-curvature coupling and the de Sitter swampland conjectures
- A maximal-entropy initial state of the Universe as a microscopic description of inflation
- 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
- Primordial black holes save inflation
- Non-gaussianity and Statistical Anisotropy in Cosmological Inflationary Models
- Primordial non-Gaussianity estimator: the inhomogeneous noise effect
- Compactification driven Hilltop Inflation in Einstein-Yang-Mills
- Warm Ekpyrosis
- Thermal Inflation with a Thermal Waterfall Scalar Field Coupled to a Light Spectator Scalar Field
- CMB lensing forecasts for constraining the primordial perturbations: adding to the CMB temperature and polarization information
- The quantum origin of cosmic structure: theory and observations
- SuperCool Inflation: A Graceful Exit from Eternal Inflation at LHC Scales and Below
- Mixed perturbations from an Inflaton and Two Curvatons - towards understanding non-gaussianity in more complicated curvaton scenarios
- Primordial black holes from a curvaton: the role of bimodal distributions
- f(R) in Holographic and Agegraphic Dark Energy Models and the Generalized Uncertainty Principle
- Zonal Modes of Cosmic Microwave Background Temperature Maps
- Large non-Gaussianity generated after D-term Inflation by Right-Handed Sneutrino Curvaton
- Flat Direction Dynamics in a Non-Topological Soliton-Dominated Universe
- Stabilising the Planck mass shortly after inflation
- QCD Axions and CMB Anisotropy
- Sneutrinos as two inflatons and curvaton and leptogenesis
- Viable Curvaton Models from the Parameter
- Curvature perturbations from kinetic preheating after -attractor inflation
- The Quantum Phase of Inflation
- Suppression of the large scale curvature perturbation by interacting fluids
- Curvaton: Perturbations and reheating
- Constraints on the three-fluid model of curvaton decay
- Cosmological correlation functions in scalar and vector inflationary models
- Curvaton decay into relativistic matter
- Right-Handed Sneutrino Curvaton and non-Gaussianity
- Possible origin of CMB temperature fluctuations: Vacuum fluctuations of Kaluza-Klein and string states during inflationary era
- Cosmic inflation in non-perturbative quantum gravity
- Spectator fields and their imprints on the Cosmic Microwave Background
- Curvaton mechanism and its implications to sneutrino cosmology
- The shape of high order correlation functions in CMB anisotropy maps
- Measuring CMB non-Gaussianity as a probe of Inflation and Cosmic Strings
- Non-linear effects in early Universe cosmology
- Constraining primordial non-Gaussianity using Neural Networks
- Comprehensive analysis of dissipative effects in the induced gravitational waves
- Forecasting isocurvature models with CMB lensing information: axion and curvaton scenarios
- Gravity of Cosmological Perturbations in the CMB
- Generalized neutrino isocurvature
- Curvature perturbations from vacuum transition during inflation
- Probing Dark Matter Isocurvature with Primordial Non-Gaussianity
- On the four-dimensional effective theories in brane-worlds
- Hidden in the background: a local approach to CMB anomalies
- Non-Gaussianity after many-field reheating
- Inhomogeneous Reheating Scenario with DBI fields
- Cosmic voids and BAO with relative baryon-CDM perturbations
- Unified Origin of Curvature Perturbation and Baryon Asymmetry of the Universe
- Primordial non-Gaussianity systematics from redshift mismatch with SPHEREx
- Testing Inflationary Cosmology
- Primordial Fluctuations in String Cosmology
- Searching for dark matter isocurvature initial conditions with N-body Simulations