Adiabatic and entropy perturbations with interacting fluids and fields
arXiv:astro-ph/0411703 · doi:10.1088/1475-7516/2005/02/007
Abstract
We develop a gauge-invariant formalism for the study of density perturbations in a Friedmann-Robertson-Walker universe with multiple interacting fluids and/or scalar fields. We show how N scalar fields may be described by N kinetic fluids (with maximally stiff equation of state) interacting with a non-dynamical potential (with vacuum equation of state). We split generic perturbations into adiabatic and entropic parts, and give the coupled first-order evolution equations on all scales, including energy and momentum exchange. We identify the non-adiabatic effects on large scales, and define adiabatic initial conditions in the presence of multiple fluids and fields.
20 pages, no figures, revtex4; v2: minor changes, typos corrected, references added
Cited by in corpus (96)
- Inflation Dynamics and Reheating
- Bouncing Cosmologies: Progress and Problems
- Cosmological perturbations in the Palatini formulation of modified gravity
- Growth of perturbations in dark matter coupled with quintessence
- The dark degeneracy: On the number and nature of dark components
- Multiple field inflation
- A numerical study of non-gaussianity in the curvaton scenario
- Density perturbations in f(R) gravity theories in metric and Palatini formalisms
- Crossing the Phantom Divide
- Effective Theory of Interacting Dark Energy
- The dark degeneracy and interacting cosmic components
- Cosmological constraints on a decomposed Chaplygin gas
- Non-thermal Histories and Implications for Structure Formation
- The non-adiabatic pressure in general scalar field systems
- Bouncing cosmological solutions from f(R,T) gravity
- The Full Second-Order Radiation Transfer Function for Large-Scale CMB Anisotropies
- Magnetized CMB observables: a dedicated numerical approach
- Gauge-invariant perturbations at second order: multiple scalar fields on large scales
- Late time transitions in the quintessence field and the tension
- Post- constraints on interacting vacuum energy
- Consistent perturbations in an imperfect fluid
- Metric preheating and radiative decay in single-field inflation
- Chiral Gravitational Waves and Baryon Superfluid Dark Matter
- Primordial black hole dark matter from inflation: the reverse engineering approach
- Interacting 3-form dark energy models: distinguishing interactions and avoiding the Little Sibling of the Big Rip
- MultiModeCode: An efficient numerical solver for multifield inflation
- A Concise Introduction to Perturbation Theory in Cosmology
- Calculating Non-adiabatic Pressure Perturbations during Multi-field Inflation
- Compensated isocurvature perturbations in the curvaton model
- Cosmological perturbations in SFT inspired non-local scalar field models
- Shortcomings of New Parametrizations of Inflation
- Cosmological perturbations for an inflaton field coupled to radiation
- Nonlinear perturbations for dissipative and interacting relativistic fluids
- Preheating and Entropy Perturbations in Axion Monodromy Inflation
- Analysis of scalar perturbations in cosmological models with a non-local scalar field
- Observable Chiral Gravitational Waves from Inflation in String Theory
- Mass varying neutrinos, symmetry breaking, and cosmic acceleration
- Viable tensor-to-scalar ratio in a symmetric matter bounce
- Dark Matter in the Standard Model?
- Constraints on a decomposed dark fluid with constant adiabatic sound speed by jointing the geometry test and growth rate after Planck data
- Quantization of Perturbations in an Inflating Elastic Solid
- Chain inflation revisited
- Evolution of the curvature perturbation during and after multi-field inflation
- Cosmological perturbations for imperfect fluids
- Interacting viscous mixtures
- Differentiating dark interactions with perturbation
- Non-Gaussianity in three fluid curvaton model
- Gauge-invariant perturbation theory for trans-Planckian inflation
- Observational constraints on interacting vacuum energy with linear interactions
- Viable scalar spectral tilt and tensor-to-scalar ratio in near-matter bounces
- Opening the reheating box in multifield inflation
- Perturbation spectra in the warm -inflation
- Reheating in tachyonic inflationary models: Effects on the large scale curvature perturbations
- Low Scale Inflation at High Energy Colliders and Meson Factories
- Testing the equivalence principle on cosmological scales using the odd multipoles of galaxy cross-power spectrum and bispectrum
- Probing a panoply of curvaton-decay scenarios using CMB data
- Entropy Production in Affine Inflation
- Effects of non-linearities on magnetic field generation
- How the curvaton scenario, modulated reheating and an inhomogeneous end of inflation are related
- Dark energy homogeneity in general relativity: Are we applying it correctly?
- Gauge conditions in combined dark energy and dark matter systems
- Linear Density Perturbations in Multifield Coupled Quintessence
- Embedding DBI inflation in scalar-tensor theory
- Observational Constraints on Two-field Warm Inflation
- Coupling structure of multi-field primordial perturbations
- Revealing the non-adiabatic nature of dark energy perturbations from galaxy clustering data
- Dark energy with the help of interacting dark sectors
- Non-adiabatic perturbations in multi-component perfect fluids
- The magnitude of the non-adiabatic pressure in the cosmic fluid
- A Fake Instability in String Inflation
- Impact of freeze-in on dark matter isocurvature
- Preheating in an Asymptotically Safe Quantum Field Theory
- Two-field Warm Inflation and Its Scalar Perturbations on Large Scales
- Degeneracy between nonadiabatic dark energy models and CDM: ISW effect and the cross correlation of CMB with galaxy clustering data
- Second order cosmological perturbations: new conserved quantities and the general solution at super-horizon scale
- Dynamics of entropy perturbations in assisted dark energy with mixed kinetic terms
- Consistent energy-momentum trace couplings of fluids
- A Separate Universe Approach to Quintessence Perturbations
- Dark Matter from freeze-in and its inhomogeneities
- Isocurvature modes and non-Gaussianity in affine inflation
- Structure Formation Constraints on Sommerfeld-Enhanced Dark Matter Annihilation
- Inhomogeneous and interacting vacuum energy
- The Effect of Curvaton Decay on the Primordial Power Spectrum
- Perturbation in an interacting dark universe
- Warm Ekpyrosis
- Dynamical aspects of asymmetric Eddington gravity with scalar fields
- The general solution at large scale for second order perturbations in a scalar field dominated universe
- The Non-Adiabatic Pressure Perturbation and Non-Canonical Kinetic Terms in Multifield Inflation
- Curvaton decay into relativistic matter
- CMB in the river frame and gauge invariance at second order
- Generation of CMB and Cosmological constant via bulk viscosity
- Suppression of the large scale curvature perturbation by interacting fluids
- Scalar Perturbations in Two-Temperature Cosmological Plasmas
- The frozen vanilla model: Exploring dark sector interactions with delta effective theories
- The intrinsic bispectrum of the CMB from isocurvature initial conditions
- Cosmological long-wavelength solutions in non-adiabatic multi-fluid systems