Discriminating different models of luminosity-redshift distribution
arXiv:1303.5484 · doi:10.1088/0264-9381/30/9/095011
Abstract
The beginning of the cosmological phase bearing the direct kinematic imprints of supernovae dimming may significantly vary within different models of late-time cosmology, even if such models are able to fit present SNe data at a comparable level of statistical accuracy. This effect -- useful in principle to discriminate among different physical interpretations of the luminosity-redshift relation -- is illustrated here with a pedagogical example based on the LTB geometry.
11 pages, 6 figures. To appear in Class. Quantum Grav
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