about
Causality and superluminal behavior in classical field theories: Applications to k -essence theories and modified-Newtonian-dynamics-like theories of gravityInflation driven by the Galileon field.Impact of three years of data from the Wilkinson Microwave Anisotropy Probe on cosmological models with dynamical dark energyPHANTOM ENERGY FROM GRADED ALGEBRASUnveiling the Dynamics of the UniverseSmooth Crossing ofwΛ=−1Line in a Single Scalar Field ModelUnified Dark Matter Scalar Field ModelsInflation with violation of the null energy conditionConsidering Late-Time Acceleration in Some Cosmological ModelsCosmological Dynamics of a Hybrid Chameleon ScenarioGauss-Bonnet Braneworld Cosmology with Modified Induced Gravity on the BraneDynamics of Mixed Dark Energy Domination in Teleparallel Gravity and Phase-Space AnalysisSpinor Quintom Cosmology with Intrinsic SpinInteracting Dark Matter andq-Deformed Dark Energy Nonminimally Coupled to GravityCouplingq-Deformed Dark Energy to Dark MatterGravitational Quasinormal Modes of Regular Phantom Black Hole
P2860
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P2860
description
im Januar 2005 veröffentlichter wissenschaftlicher Artikel
@de
wetenschappelijk artikel
@nl
наукова стаття, опублікована в січні 2005
@uk
name
Can dark energy evolve to the phantom?
@en
Can dark energy evolve to the phantom?
@nl
type
label
Can dark energy evolve to the phantom?
@en
Can dark energy evolve to the phantom?
@nl
prefLabel
Can dark energy evolve to the phantom?
@en
Can dark energy evolve to the phantom?
@nl
P2860
P1433
P1476
Can dark energy evolve to the phantom?
@en
P2860
P356
10.1103/PHYSREVD.71.023515
P407
P577
2005-01-18T00:00:00Z
P818
astro-ph/0407107