English

Bayesian model selection without evidences: application to the dark energy equation-of-state

Cosmology and Nongalactic Astrophysics 2017-01-26 v2 Instrumentation and Methods for Astrophysics

Abstract

A method is presented for Bayesian model selection without explicitly computing evidences, by using a combined likelihood and introducing an integer model selection parameter nn so that Bayes factors, or more generally posterior odds ratios, may be read off directly from the posterior of nn. If the total number of models under consideration is specified a priori, the full joint parameter space (θ,n)(\theta, n) of the models is of fixed dimensionality and can be explored using standard Markov chain Monte Carlo (MCMC) or nested sampling methods, without the need for reversible jump MCMC techniques. The posterior on nn is then obtained by straightforward marginalisation. We demonstrate the efficacy of our approach by application to several toy models. We then apply it to constraining the dark energy equation-of-state using a free-form reconstruction technique. We show that Λ\LambdaCDM is significantly favoured over all extensions, including the simple w(z)=constantw(z){=}{\rm constant} model.

Keywords

Cite

@article{arxiv.1506.09024,
  title  = {Bayesian model selection without evidences: application to the dark energy equation-of-state},
  author = {Sonke Hee and Will Handley and Mike P. Hobson and Anthony N. Lasenby},
  journal= {arXiv preprint arXiv:1506.09024},
  year   = {2017}
}

Comments

Published in MNRAS. Article is 13 pages long including 12 figures, 3 tables and 2 appendices