about
Precision cosmology defeats void models for accelerationGravitational backreaction in cosmological spacetimesProbing violation of the Copernican principle via the integrated Sachs-Wolfe effectPlanck intermediate results XIII. Constraints on peculiar velocitiesSpatial and temporal tuning in void models for accelerationReconciling the local void with the CMBKinematic Sunyaev-Zel’dovich effect as a test of general radial inhomogeneity in Lemaître-Tolman-Bondi cosmology
P2860
Q21651289-2E0E773A-416A-43AE-AEAB-DC83D6254F24Q27335640-AA68EA5E-51C9-4E04-9D58-0FC4248E676FQ27335736-59E2037E-C81D-474C-9E58-8A2BEA544E31Q56057757-81608E71-62F2-493C-B1EF-6EB5CD6B03E2Q57644490-67F37952-6931-44C0-923B-0F8E551D8BE8Q57740252-6C1A0F73-DE87-410B-B8D7-5889F8FC2D36Q58468561-0BC8A8CC-3435-4064-B246-262EF091771D
P2860
description
article publié dans la revue scientifique Physical Review Letters
@fr
im Dezember 2008 veröffentlichter wissenschaftlicher Artikel
@de
scientific article published in Physical Review Letters
@en
wetenschappelijk artikel
@nl
наукова стаття, опублікована в грудні 2008
@uk
name
Can We Avoid Dark Energy?
@en
Can We Avoid Dark Energy?
@nl
type
label
Can We Avoid Dark Energy?
@en
Can We Avoid Dark Energy?
@nl
prefLabel
Can We Avoid Dark Energy?
@en
Can We Avoid Dark Energy?
@nl
P2860
P1476
Can we avoid dark energy?
@en
P2093
James P Zibin
P2860
P304
P356
10.1103/PHYSREVLETT.101.251303
P407
P577
2008-12-18T00:00:00Z