Gradient instability for w < -1
arXiv:astro-ph/0406043 · doi:10.1016/j.physletb.2004.07.025
Abstract
We show that in single scalar field models of the dark energy with equations of state satisfying , the effective Lagrangian for fluctuations about the homogeneous background has a wrong sign spatial kinetic term. In most cases, spatial gradients are ruled out by microwave background observations. The sign of is not connected to the sign of the time derivative kinetic term in the effective Lagrangian.
revtex4, 8 pages, 1 figure. v2: corrected typo in Eq. 16, added references and a paragraph on quintessence models; v3: reordering of references. To appear in Phys. Lett. B
References in corpus (17)
- The Cosmological Constant and Dark Energy
- A Phantom Menace? Cosmological consequences of a dark energy component with super-negative equation of state
- The Case for a Positive Cosmological Lambda-term
- New Constraints on , , and w from an Independent Set of Eleven High-Redshift Supernovae Observed with HST
- Kinetically Driven Quintessence
- Can the dark energy equation-of-state parameter w be less than -1?
- Reconstruction of a scalar-tensor theory of gravity in an accelerating universe
- Ghost Condensation and a Consistent Infrared Modification of Gravity
- The State of the Dark Energy Equation of State
- Super-Acceleration from Massless, Minimally Coupled
- Quintessence, super-quintessence and observable quantities in Brans-Dicke and non-minimally coupled theories
- Probing the dark side: Constraints on the dark energy equation of state from CMB, large scale structure and Type Ia supernovae
- Measuring the Equation-of-state of the Universe: Pitfalls and Prospects
- Superquintessence
- Non-perturbative effects of vacuum energy on the recent expansion of the universe
- The Tensor to Scalar Ratio of Phantom Dark Energy Models
- How to Test Stringy Dark Energy?
Cited by in corpus (94)
- The Effective Field Theory of Inflation
- The Cosmology of Generalized Modified Gravity Models
- Starting the Universe: Stable Violation of the Null Energy Condition and Non-standard Cosmologies
- Quantum effects can render w<-1 on cosmological scales
- Constraints on holographic dark energy from type Ia supernova observations
- Null energy condition and superluminal propagation
- Super-acceleration as Signature of Dark Sector Interaction
- The Effective Theory of Quintessence: the w<-1 Side Unveiled
- Crossing of the w=-1 Barrier by D3-brane Dark Energy Model
- The stability of modified gravity models
- "Expansion" around the vacuum equation of state - sudden future singularities and asymptotic behavior
- Two Loop Scalar Self-Mass during Inflation
- A Single Scalar Field Model of Dark Energy with Equation of State Crossing -1
- Quantum Stability of a w < - 1 Phase of Cosmic Acceleration
- Spherical collapse in quintessence models with zero speed of sound
- Phantom cosmology with general potentials
- Exactly Solvable SFT Inspired Phantom Model
- Can we be tricked into thinking that w is less than -1?
- Bouncing and Accelerating Solutions in Nonlocal Stringy Models
- Noether symmetry approach in phantom quintessence cosmology
- Exorcising w < -1
- Phantom Friedmann Cosmologies and Higher-Order Characteristics of Expansion
- Which cosmological model with dark energy -- phantom or LambdaCDM
- Cosmological consequences of an adiabatic matter creation process
- Two loop stress-energy tensor for inflationary scalar electrodynamics
- Non-minimal coupling, exponential potentials and the regime of dark energy
- The generalized second law in phantom dominated universes in the presence of black holes
- Dynamics in Nonlocal Cosmological Models Derived from String Field Theory
- Dark energy transition between quintessence and phantom regimes - an equation of state analysis
- Dark Energy, Inflation and Extra Dimensions
- A Symmetry for the Cosmological Constant
- The null energy condition and instability
- Instabilities and the null energy condition
- Phantom behavior via cosmological creation of particles
- Cosmological apparent and trapping horizons
- A Completely Regular Quantum Stress Tensor with
- Making sense of the bizarre behaviour of horizons in the McVittie spacetime
- The correspondence between a scalar field and an effective perfect fluid
- Which cosmological models -- with dark energy or modified FRW dynamics?
- On the Null Energy Condition and Cosmology
- Cosmological tachyon condensation
- Cheng-Weyl Vector Field and its Cosmological Application
- Relaxing the Cosmological Constant: a Proof of Concept
- Patch dualities and remarks on nonstandard cosmologies
- Stringy Dark Energy Model with Cold Dark Matter
- On Wormholes supported by phantom energy
- Cosmological perturbations in an effective and genuinely phantom dark energy Universe
- Localization of nonlocal cosmological models with quadratic potentials in the case of double roots
- Phantom-like behaviour in a brane-world model with curvature effects
- Dynamical analysis of interacting dark energy model in the framework of particle creation mechanism
- The Accelerated Acceleration of the Universe
- Non-chaotic dynamics in general-relativistic and scalar-tensor cosmology
- Null Energy Condition Violation and Classical Stability in the Bianchi I Metric
- Connecting inflation with late cosmic acceleration by particle production
- Model for a Universe described by a non-minimally coupled scalar field and interacting dark matter
- Oxidised cosmic acceleration
- Accretion of nonminimally coupled scalar fields into black holes
- On Energy Conditions and Stability in Effective Loop Quantum Cosmology
- Stability and the Gauge Problem in Non-Perturbative Cosmology
- Infrared modified gravity with propagating torsion: instability of torsionfull de Sitter-like solutions
- Crossing the cosmological constant line in a dilatonic brane-world model with and without curvature corrections
- Future state of the Universe
- A no-go for no-go theorems prohibiting cosmic acceleration in extra dimensional models
- Observational Constraints on the Generalized Chaplygin Gas
- Scale Factor Duality for Conformal Cyclic Cosmologies
- Exploring cosmological imprints of phantom crossing with dynamical dark energy in Horndeski gravity
- Interacting quintessence cosmology from Noether symmetries: comparing theoretical predictions with observational data
- Gravitationally induced particle production and its impact on structure formation
- Ghost Condensate Busting
- Presence of anisotropic pressures in Lemaître-Tolman-Bondi cosmological models
- Higher Order Lagrangians inspired by the Pais-Uhlenbeck Oscillator and their cosmological applications
- Dark energy with a shift-symmetric scalar field: obstacles, loophole hunting and dead ends
- Constraining Temporal Oscillations of Cosmological Parameters Using Type Ia Supernovae
- Lower Limit to the Scale of an Effective Theory of Gravitation
- Understanding large scale CMB anomalies with the generalized non-minimal derivative coupling during inflation
- Primordial Gravitational Waves Enhancement
- Fractons in effective field theories for spontaneously broken translations
- Possible Enhancement of High Frequency Gravitational Waves
- The effect of curvature in thawing models
- Cosmological applications in Kaluza-Klein theory
- Crossing of the Cosmological Constant Boundary - an Equation of State Description
- How Much NEC Breaking Can the Universe Endure?
- Geodesic completeness, cosmological bounces and inflation
- Entropic considerations on the Universe and Universe-Black Hole Systems
- D-bound and Bekenstein bound for McVittie solution surrounded by dark energy cosmological fields
- Hitchhiker's Guide to the Swampland: The Cosmologist's Handbook to the string-theoretical Swampland Programme
- D-bound and Bekenstein Bound for the Surrounded Vaidya Black Hole
- An entropy-driven cosmic expansion
- Power-law solutions for TeVeS
- Semi-classical wormholes and time machines are unstable
- K-nonizing
- Precision cosmological measurements: independent evidence for dark energy
- Surface Layers in the Gravity/Hydrodynamics Correspondence
- Weakly Broken Galileon Symmetry in Cosmology