Cosmography: Extracting the Hubble series from the supernova data
arXiv:gr-qc/0703122
Abstract
We perform a number of inter-related cosmographic fits to the legacy05 and gold06 supernova datasets. We pay particular attention to the influence of both statistical and systematic uncertainties, and also to the extent to which the choice of distance scale and manner of representing the redshift scale affect the cosmological parameters. While the "preponderance of evidence" certainly suggests an accelerating universe, we would argue that (based on the supernova data) this conclusion is not currently supported "beyond reasonable doubt". As part of the analysis we develop two particularly transparent graphical representations of the redshift-distance relation -- representations in which acceleration versus deceleration reduces to the question of whether the graph slopes up or down. Turning to the details of the cosmographic fits, three issues in particular concern us: First, the fitted value for the deceleration parameter changes significantly depending on whether one performs a chi^2 fit to the luminosity distance, proper motion distance, angular diameter distance, or other suitable distance surrogate. Second, the fitted value for the deceleration parameter changes significantly depending on whether one uses the traditional redshift variable z, or what we shall argue is on theoretical grounds an improved parameterization y=z/(1+z). Third, the published estimates for systematic uncertainties are sufficiently large that they certainly impact on, and to a large extent undermine, the usual purely statistical tests of significance. We conclude that the case for an accelerating universe is considerably less watertight than commonly believed.
V3: 50 pages, 10 figures, 10 tables, uses iopart.cls; Discussion extended and clarified, additional references, treatment of systematic uncertanties now in line with NIST guidelines and the norms of the supernova community. More discussion and historical context; some historical graphs, additional clarifying comments - no change in physics conclusions
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- Cosmological particle production in emergent rainbow spacetimes
- Probing the anisotropic expansion from supernovae and GRBs in a model-independent way
- Quantifying the evidence for the current speed-up of the Universe with low and intermediate-redshift data. A more model-independent approach
- Conformally Friedmann-Lemaitre-Robertson-Walker cosmologies
- Pantheon update on a model-independent analysis of cosmological supernova data
- A covariant treatment of cosmic parallax
- BAO cosmography
- Dark Energy: The Shadowy Reflection of Dark Matter?
- Constraints on kinematic parameters at
- Emergent spacetimes
- Cosmology In Terms Of The Deceleration Parameter. Part II
- Non-perturbative results for the luminosity and area distances
- Bounding the Hubble flow in terms of the w parameter
- Cosmic acceleration driven by dark matter self-interactions: a phenomenological treatment
- Delineating cosmic expansion history with recent supernova data: A Bayesian model-independent approach