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Testing $$R_h=ct$$ R h = c t cosmology from fundamental considerations: Is the Friedmann universe intrinsically flatThe cosmic equation of stateThe H ii galaxy Hubble diagram strongly favoursRh=ctover ΛCDMCosmological test with the QSO Hubble diagramA two-point diagnostic for the H ii galaxy Hubble diagramAnalysing H(z) data using two-point diagnosticsAlcock–Paczyński test with model-independent BAO dataThe epoch of reionization in theRh = ctuniversePhysical basis for the symmetries in the Friedmann–Robertson–Walker metricConstancy of the cluster gas mass fraction in theRh=ctUniverseSupermassive black holes in the early UniverseThe AGN Hubble Diagram and its implications for cosmologyCosmological tests using the angular size of galaxy clustersOn recent claims concerning the Rh = ct UniverseCosmological tests using gamma-ray bursts, the star formation rate and possible abundance evolutionAngular correlation of the cosmic microwave background in theRh=ctUniverseCosmic chronometers in the Rh = ct UniverseTheRh =ctuniverse without inflationPhoton geodesics in Friedmann-Robertson-Walker cosmologiesReconciling the cosmic age problem in the $$R_\mathrm{h}=ct$$ R h = c t universe
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description
im November 2011 veröffentlichter wissenschaftlicher Artikel
@de
wetenschappelijk artikel
@nl
наукова стаття, опублікована в листопаді 2011
@uk
name
The Rh=ct universe
@en
The Rh=ct universe
@nl
type
label
The Rh=ct universe
@en
The Rh=ct universe
@nl
prefLabel
The Rh=ct universe
@en
The Rh=ct universe
@nl
P2860
P1476
The Rh=ct universe
@en
P2093
A. S. H. Shevchuk
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P304
P356
10.1111/J.1365-2966.2011.19906.X
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P50
P577
2011-11-08T00:00:00Z
P5875
P818
P819
2012MNRAS.419.2579M