http://arxiv.org/abs/2111.04231
We look at the distribution of the Bayesian evidence for mock realizations of supernova and baryon acoustic oscillation data. The ratios of Bayesian evidences of different models are often used to perform model selection. The significance of these Bayes factors are then interpreted using scales such as the Jeffreys or Kass \& Raftery scale. First, we demonstrate how to use the evidence itself to validate the model, that is to say how well a model fits the data, regardless of how well other models perform. The basic idea is that if, for some real dataset a model’s evidence lies outside the distribution of evidences that result when the same fiducial model that generates the datasets is used for the analysis, then the model in question is robustly ruled out. Further, we show how to asses the significance of a hypothetically computed Bayes factor. We show that range of the distribution of Bayes factors can greatly depend on the models in question and also the number of independent degrees of freedom in the dataset. Thus, we have demonstrated that the significance of Bayes factors need to be calculated for each unique dataset.
R. Keeley and A. Shafieloo
Tue, 9 Nov 21
98/102
Comments: 6 pages, 4 figures
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