A note on the equivalence of a barotropic perfect fluid with a K-essence scalar field
arXiv:1002.1376 · doi:10.1103/PhysRevD.81.107301
Abstract
In this short note, we obtain the necessary and sufficient condition for a class of non-canonical single scalar field models to be exactly equivalent to barotropic perfect fluids, under the assumption of an irrotational fluid flow. An immediate consequence of this result is that the non-adiabatic pressure perturbation in this class of scalar field systems vanishes exactly at all orders in perturbation theory and on all scales. The Lagrangian for this general class of scalar field models depends on both the kinetic term and the value of the field. However, after a field redefinition, it can be effectively cast in the form of a purely kinetic K-essence model.
arXiv comment4 pages, 1 figure; v2: References and footnotes 3 and 4 added. Replaced to match published version
References in corpus (40)
- Dynamics of dark energy
- Non-Gaussian features of primordial fluctuations in single field inflationary models
- k-Inflation
- Non-Gaussianity from Inflation: Theory and Observations
- Perturbations in k-inflation
- DBI in the Sky
- Observational Signatures and Non-Gaussianities of General Single Field Inflation
- A new approach to the evolution of cosmological perturbations on large scales
- A general proof of the conservation of the curvature perturbation
- Scalar Speed Limits and Cosmology: Acceleration from D-cceleration
- Cosmological perturbations
- Primordial non-gaussianities in single field inflation
- Primordial non-gaussianities from multiple-field inflation
- Primordial perturbations and non-Gaussianities in DBI and general multi-field inflation
- Perturbations in generalized multi-field inflation
- Inflation from Warped Space
- Multi-Throat Brane Inflation
- Evolution of second-order cosmological perturbations
- The Inflationary Trispectrum for Models with Large Non-Gaussianities
- The inflationary trispectrum
- Primordial fluctuations and non-Gaussianities in multi-field DBI inflation
- Evolution of non-linear cosmological perturbations
- Non-gaussianity from the trispectrum in general single field inflation
- Non-gaussianity from the bispectrum in general multiple field inflation
- The non-adiabatic pressure in general scalar field systems
- On the full trispectrum in single field DBI-inflation
- How the Scalar Field of Unified Dark Matter Models Can Cluster
- On the full quantum trispectrum in multi-field DBI inflation
- Action approach to cosmological perturbations: the 2nd order metric in matter dominance
- Lorentz boost and non-Gaussianity in multi-field DBI-inflation
- Affine equation of state from quintessence and k-essence fields
- Relativistic hydrodynamics with sources for cosmological K-fluids
- Combined local and equilateral non-Gaussianities from multifield DBI inflation
- Inflationary trispectrum from graviton exchange
- Large Primordial Trispectra in General Single Field Inflation
- Nonlinear perturbations of cosmological scalar fields with non-standard kinetic terms
- A not so short note on the Klein-Gordon equation at second order
- Stationary Configurations Imply Shift Symmetry: No Bondi Accretion for Quintessence / k-Essence
- Practical tools for third order cosmological perturbations
- CMB temperature anisotropies from third order gravitational perturbations
Cited by in corpus (50)
- Beyond the Cosmological Standard Model
- Dark energy in Horndeski theories after GW170817: A review
- The Imperfect Fluid behind Kinetic Gravity Braiding
- Cosmology in generalized Proca theories
- Beyond generalized Proca theories
- Viable cosmology in bimetric theory
- Unified Dark Matter Scalar Field Models
- Anisotropy in solid inflation
- Pure kinetic k-essence as the cosmic speed-up
- Imperfect fluid description of modified gravities
- Wormholes minimally violating the null energy condition
- Consistent perturbations in an imperfect fluid
- The correspondence between a scalar field and an effective perfect fluid
- Generalizing a Unified Model of Dark Matter, Dark Energy, and Inflation with Non Canonical Kinetic Term
- Dark energy scenario consistent with GW170817 in theories beyond Horndeski gravity
- Conserved cosmological perturbation in Galileon models
- Anisotropic cosmological solutions in massive vector theories
- Cosmology in beyond-generalized Proca theories
- Noether analysis of Scalar-Tensor Cosmology
- Unified Dark Matter scalar field models with fast transition
- Phase-space analysis of a class of k-essence cosmology
- Observational signatures of the theories beyond Horndeski
- Stability of scalar perturbations in scalar-torsion gravity theories in the presence of a matter fluid
- Scalar field as a perfect fluid: thermodynamics of minimally coupled scalars and Einstein frame scalar-tensor gravity
- Viable tensor-to-scalar ratio in a symmetric matter bounce
- Anisotropic -form dark energy
- Fluid Inflation
- Cosmology with a successful Vainshtein screening in theories beyond Horndeski
- Equivalence between Horndeski and beyond Horndeski theories and imperfect fluids
- Global adiabaticity and non-Gaussianity consistency condition
- Stability of relativistic stars with scalar hairs
- Quantum fractionary cosmology: K-essence theory
- Field Theories and Fluids for an Interacting Dark Sector
- Cosmological disformal transformations to the Einstein frame and gravitational couplings with matter perturbations
- Lagrangian description of cosmic fluids: mapping dark energy into unified dark energy
- Note on scalars, perfect fluids, constrained field theories, and all that
- Perfect fluid in Lagrangian formulation due to generalized three-form field
- Dynamic Field Theory and Equations of Motion in Cosmology
- Perfect fluids from high power sigma-models
- Dissipative quintessence, and its cosmological implications
- Non-Stationary Dark Energy Around a Black Hole
- Inflation with exotic kinetic terms in Einstein-Chern-Simons gravity
- Primordial perturbations and inflation in holographic cosmology
- On tachyonic stability priors for dark energy
- Cosmological Perturbations: Vorticity, Isocurvature and Magnetic Fields
- Adiabatic and non-adiabatic perturbations for loop quantum cosmology
- Reconstruction of a kinetic k--essence Lagrangian from a modified of dark energy equation of state
- A Scaling Relation in Inhomogeneous Cosmology with k-essence scalar fields
- Effective field theory of coupled dark energy and dark matter
- Primordial perturbations and inflation in a holography inspired Gauss-Bonnet cosmology