Quintessence, Cosmic Coincidence, and the Cosmological Constant
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Chameleon cosmologyWhy the universe is just soDark energy and supermassive black holesCoexistence of Black Holes and a Long-Range Scalar Field in CosmologyCosmological tracking solutionsQuintessence as a runaway dilatonCosmology from start to finishThe Cosmological ConstantGrowth rate in the dynamical dark energy models.Rigorous theoretical constraint on constant negative EoS parameter [Formula: see text] and its effect for the late UniverseASTROPHYSICS. Atom-interferometry constraints on dark energy.Solving the coincidence problem: tracking oscillating energy.Skewness as a test of the equivalence principle.Cosmology of a Friedmann-Lamaître-Robertson-Walker 3-brane, late-time cosmic acceleration, and the cosmic coincidence.Dark energy from primordial inflationary quantum fluctuations.Scalar-field-dominated cosmology with a transient acceleration phase.Constraining inverse-curvature gravity with supernovae.Limits of quintessence.Black hole mass decreasing due to phantom energy accretion.Model-independent dark energy differentiation with the integrated Sachs-Wolfe effect.Spinodal instabilities and the dark energy problem.Apparent clustering of intermediate-redshift galaxies as a probe of dark energy.Catastrophic consequences of kicking the chameleon.Constraining Dark Energy with Type Ia Supernovae and Large-Scale StructureCan dark energy evolve to the phantom?Multiple field modified gravity and localized energy in teleparallel frameworkPHANTOM ENERGY FROM GRADED ALGEBRASOn quintessential cosmological models and exponential potentialsQuintessence and Born-Infeld cosmologySeesaw Mechanism for Scalar Fields as Possible Basis for Dark EnergyQuantum field theory of interacting dark matter and dark energy: Dark monodromiesUnveiling the Dynamics of the UniverseScaling solutions from interacting fluidsWEIGHING THE UNIVERSE WITH ACCELERATORS AND DETECTORSBosonic coherent motions in the UniverseIntermediate Inflation or Late Time Acceleration?Smooth Crossing ofwΛ=−1Line in a Single Scalar Field ModelHiggs production as a probe of chameleon dark energyAttractors and isocurvature perturbations in quintessence modelsCosmological Dynamics of a Hybrid Chameleon Scenario
P2860
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P2860
Quintessence, Cosmic Coincidence, and the Cosmological Constant
description
1999 nî lūn-bûn
@nan
1999 թուականի Փետրուարին հրատարակուած գիտական յօդուած
@hyw
1999 թվականի փետրվարին հրատարակված գիտական հոդված
@hy
1999年の論文
@ja
1999年論文
@yue
1999年論文
@zh-hant
1999年論文
@zh-hk
1999年論文
@zh-mo
1999年論文
@zh-tw
1999年论文
@wuu
name
Quintessence, Cosmic Coincidence, and the Cosmological Constant
@ast
Quintessence, Cosmic Coincidence, and the Cosmological Constant
@en
Quintessence, Cosmic Coincidence, and the Cosmological Constant
@en-gb
type
label
Quintessence, Cosmic Coincidence, and the Cosmological Constant
@ast
Quintessence, Cosmic Coincidence, and the Cosmological Constant
@en
Quintessence, Cosmic Coincidence, and the Cosmological Constant
@en-gb
prefLabel
Quintessence, Cosmic Coincidence, and the Cosmological Constant
@ast
Quintessence, Cosmic Coincidence, and the Cosmological Constant
@en
Quintessence, Cosmic Coincidence, and the Cosmological Constant
@en-gb
P2860
P1476
Quintessence, Cosmic Coincidence, and the Cosmological Constant
@en
P2093
Ivaylo Zlatev
Limin Wang
P2860
P304
P356
10.1103/PHYSREVLETT.82.896
P407
P577
1999-02-01T00:00:00Z
P818
astro-ph/9807002