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The cosmological constant and dark energyQuintessence, Cosmic Coincidence, and the Cosmological ConstantOne-loop quantum corrections to cosmological scalar field potentialsDark energy and supermassive black holesDetecting dark energy in orbit: The cosmological chameleonRunning Newton constant, improved gravitational actions, and galaxy rotation curvesObservational constraints on dark energy and cosmic curvatureCosmological tracking solutionsUncorrelated measurements of the cosmic expansion history and dark energy from supernovaeNew Dark Energy Constraints from Supernovae, Microwave Background, and Galaxy ClusteringCosmology from start to finishVacuum quanta and the nature of gravityThe Cosmological ConstantASTROPHYSICS. Atom-interferometry constraints on dark energy.Dilatation symmetry in higher dimensions and the vanishing of the cosmological constant.No-go theorem for k-essence dark energy.Scalar-field-dominated cosmology with a transient acceleration phase.Cosmology with massive neutrinos coupled to dark energy.Evolving dark energy with w not = -1.Black hole mass decreasing due to phantom energy accretion.Cosmological Higgs fields.Measuring the speed of sound of quintessence.Limitations in Using Luminosity Distance to Determine the Equation of State of the Universe.Decaying vacuum energy and deflationary cosmology in open and closed universes.Inflation in an open universe.Quintessence and the Rest of the World: Suppressing Long-Range InteractionsWarping with dilatation symmetry and self-tuning of the cosmological constantQuintessence cosmologies with a growing matter componentCan structure formation influence the cosmological evolution?Cosmon dark matter?On quintessential cosmological models and exponential potentialsQuintessence and Born-Infeld cosmologyThe clustering of galaxies in the SDSS-III DR9 Baryon Oscillation Spectroscopic Survey: testing deviations from Λ and general relativity using anisotropic clustering of galaxiesTensor to scalar ratio of phantom dark energy modelsObservationally determining the properties of dark matterSeesaw Mechanism for Scalar Fields as Possible Basis for Dark EnergyEvading equivalence principle violations, cosmological, and other experimental constraints in scalar field theories with a strong coupling to matterCosmology of mass-varying neutrinos driven by quintessence: Theory and observationsOn the spherical collapse model in dark energy cosmologiesThe clustering of galaxies in the completed SDSS-III Baryon Oscillation Spectroscopic Survey: tomographic BAO analysis of DR12 combined sample in Fourier space
P2860
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P2860
description
article publié dans la revue scientifique Astrophysical Journal
@fr
im Februar 1988 veröffentlichter wissenschaftlicher Artikel
@de
scientific article published in the Astrophysical Journal
@en
wetenschappelijk artikel
@nl
наукова стаття, опублікована в лютому 1988
@uk
name
Cosmology with a time-variable cosmological 'constant'
@en
Cosmology with a time-variable cosmological 'constant'
@nl
type
label
Cosmology with a time-variable cosmological 'constant'
@en
Cosmology with a time-variable cosmological 'constant'
@nl
prefLabel
Cosmology with a time-variable cosmological 'constant'
@en
Cosmology with a time-variable cosmological 'constant'
@nl
P356
P1476
Cosmology with a time-variable cosmological 'constant'
@en
P356
10.1086/185100
P407
P577
1988-02-01T00:00:00Z