Phantom Energy: Dark Energy with w < − 1 Causes a Cosmic Doomsday
about
Cosmological parameters from SDSS and WMAPLate-time cosmology in a (phantom) scalar-tensor theory: Dark energy and the cosmic speed-upDark energy and supermassive black holesNew Dark Energy Constraints from Supernovae, Microwave Background, and Galaxy ClusteringTurnaround in Cyclic CosmologyThe Hubble Constant.Theorems on Existence and Global Dynamics for the Einstein Equations.Neutrino masses and the dark energy equation of state: relaxing the cosmological neutrino mass bound.Phantom cosmology as a simple model with dynamical complexity.The flatness problem and Lambda.Phantom energy mediates a long-range repulsive force.Black hole mass decreasing due to phantom energy accretion.Constructing phantom cosmologies from standard scalar field universes.What if gravity becomes really repulsive in the future?More on the holographic Ricci dark energy model: smoothing Rips through interaction effects?Can dark energy evolve to the phantom?Grand rip and grand bang/crunch cosmological singularitiesGeodesics of McVittie spacetime with a phantom cosmological backgroundDISCRETE SYMMETRIES AND GENERAL RELATIVITY, THE DARK SIDE OF GRAVITYClassical and quantum cosmology of the little rip abrupt eventQuantum fate of singularities in a dark-energy dominated universePhantomlike behavior in a brane-world model with curvature effectsGravitinos tunneling from traversable Lorentzian wormholesTunnelling of vector particles from Lorentzian wormholes in 3+1 dimensionsThe Live Universe. A Biologist's PerspectiveSmooth Crossing ofwΛ=−1Line in a Single Scalar Field ModelA Scalar Field Dark Matter Model and Its Role in the Large-Scale Structure Formation in the UniverseKnot Universes in Bianchi Type I CosmologyEvolution of the cosmic microwave backgroundCosmological Dynamics of a Hybrid Chameleon ScenarioA Cosmological Model Based on a Quadratic Equation of State Unifying Vacuum Energy, Radiation, and Dark EnergyInteraction between Dark Matter and Dark Energy and the Cosmological Coincidence ProblemDynamics of Interacting Tachyonic Teleparallel Dark EnergyInteracting Quintessence Dark Energy Models in Lyra ManifoldStability of a Noncanonical Scalar Field Model during Cosmological DateSpinor Quintom Cosmology with Intrinsic SpinIsrael-Stewart Approach to Viscous Dissipative Extended Holographic Ricci Dark Energy Dominated UniverseGravitational Quasinormal Modes of Regular Phantom Black HoleEffects of time-varying $$\beta $$ β in SNLS3 on constraining interacting dark energy models
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Phantom Energy: Dark Energy with w < − 1 Causes a Cosmic Doomsday
description
2003 nî lūn-bûn
@nan
2003 թուականի Օգոստոսին հրատարակուած գիտական յօդուած
@hyw
2003 թվականի օգոստոսին հրատարակված գիտական հոդված
@hy
2003年の論文
@ja
2003年論文
@yue
2003年論文
@zh-hant
2003年論文
@zh-hk
2003年論文
@zh-mo
2003年論文
@zh-tw
2003年论文
@wuu
name
Phantom Energy: Dark Energy with w < − 1 Causes a Cosmic Doomsday
@ast
Phantom Energy: Dark Energy with w < − 1 Causes a Cosmic Doomsday
@en
Phantom Energy: Dark Energy with w < − 1 Causes a Cosmic Doomsday
@nl
type
label
Phantom Energy: Dark Energy with w < − 1 Causes a Cosmic Doomsday
@ast
Phantom Energy: Dark Energy with w < − 1 Causes a Cosmic Doomsday
@en
Phantom Energy: Dark Energy with w < − 1 Causes a Cosmic Doomsday
@nl
prefLabel
Phantom Energy: Dark Energy with w < − 1 Causes a Cosmic Doomsday
@ast
Phantom Energy: Dark Energy with w < − 1 Causes a Cosmic Doomsday
@en
Phantom Energy: Dark Energy with w < − 1 Causes a Cosmic Doomsday
@nl
P50
P1476
Phantom energy: dark energy with w <--1 causes a cosmic doomsday
@en
P2093
Nevin N. Weinberg
P304
P356
10.1103/PHYSREVLETT.91.071301
P407
P577
2003-08-13T00:00:00Z
P698
P818
astro-ph/0302506