Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
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Constraints on the Dark Side of the Universe and Observational Hubble Parameter DataAxions and the strong C P problemTheoretical aspects of massive gravityThe fundamental constants and their variation: observational and theoretical statusMore on ghosts in the Dvali-Gabadaze-Porrati modelMechanics and Newton-Cartan-like gravity on the Newton-Hooke space-timede Sitter vacua in string theoryImportance of supernovae at z > 1.5 to probe dark energyLong-term future of extragalactic astronomyLong γ-ray bursts and core-collapse supernovae have different environmentsPeculiar motions, accelerated expansion, and the cosmological axisQuark masses: An environmental impact statementA guided tour through the wild nuclear landscapeProbing violation of the Copernican principle via the integrated Sachs-Wolfe effectHolography and the large number hypothesisEvidence for Dark Energy from the Cosmic Microwave Background Alone Using the Atacama Cosmology Telescope Lensing MeasurementsMeasurement of the Casimir Force between Parallel Metallic SurfacesConfirmation of the Copernican Principle at Gpc Radial Scale and above from the Kinetic Sunyaev-Zel’dovich Effect Power SpectrumReconstructing the Cosmic Equation of State from Supernova DistancesCMB dipoles and other low-order multipoles in the quasispherical Szekeres modelA Test of the Copernican PrincipleWhy the universe is just soTesting general relativity with 21-cm intensity mappingIs cosmic speed-up due to new gravitational physics?Dark energy and supermassive black holesDetecting dark energy in orbit: The cosmological chameleonLate-time cosmology of a scalar-tensor theory with a universal multiplicative coupling between the scalar field and the matter LagrangianBlack-Hole No-Hair Theorems for a Positive Cosmological ConstantObservational constraints on dark energy and cosmic curvatureCoexistence of Black Holes and a Long-Range Scalar Field in CosmologyCosmological tracking solutionsQuintessence as a runaway dilatonUncorrelated measurements of the cosmic expansion history and dark energy from supernovaeDark energy or apparent acceleration due to a relativistic cosmological model more complex than the Friedmann-Lemaitre-Robertson-Walker model?Living in a Void: Testing the Copernican Principle with Distant SupernovaeNew Dark Energy Constraints from Supernovae, Microwave Background, and Galaxy ClusteringCosmology from start to finishSupernova SN 2011fe from an exploding carbon-oxygen white dwarf starThe type Ia supernova SNLS-03D3bb from a super-Chandrasekhar-mass white dwarf starEarth-mass dark-matter haloes as the first structures in the early Universe
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Observational Evidence from Supernovae for an Accelerating Universe and a Cosmological Constant
description
article publié dans la revue scientifique Astronomical Journal
@fr
im September 1998 veröffentlichter wissenschaftlicher Artikel
@de
scientific article published in Astronomical Journal
@en
wetenschappelijk artikel
@nl
наукова стаття, опублікована у вересні 1998
@uk
name
Observational Evidence from Su ...... se and a Cosmological Constant
@en
Observational Evidence from Su ...... se and a Cosmological Constant
@nl
type
label
Observational Evidence from Su ...... se and a Cosmological Constant
@en
Observational Evidence from Su ...... se and a Cosmological Constant
@nl
prefLabel
Observational Evidence from Su ...... se and a Cosmological Constant
@en
Observational Evidence from Su ...... se and a Cosmological Constant
@nl
P2093
P50
P356
P1476
Observational Evidence from Su ...... se and a Cosmological Constant
@en
P2093
Alan Diercks
Alejandro Clocchiatti
B. Leibundgut
Brian P. Schmidt
Craig J. Hogan
David Reiss
J. Spyromilio
John Tonry
M. M. Phillips
Peter Challis
P304
P356
10.1086/300499
P407
P577
1998-09-01T00:00:00Z
P5875
P818
astro-ph/9805201
P819
1998AJ....116.1009R