Entropic Priors and Bayesian Model Selection

被引:5
|
作者
Brewer, Brendon J. [1 ]
Francis, Matthew J. [2 ]
机构
[1] Univ Calif Santa Barbara, Dept Phys, Santa Barbara, CA 93106 USA
[2] SiSSA, Trieste, Italy
关键词
Inference; Model Selection; Dark Energy; COSMOLOGY; SUPERNOVAE; LAMBDA;
D O I
10.1063/1.3275612
中图分类号
O29 [应用数学];
学科分类号
070104 ;
摘要
We demonstrate that the principle of maximum relative entropy (ME), used judiciously, can ease the Specification of priors in model selection problems. The resulting effect is that models that make sharp predictions are disfavoured, weakening the usual Bayesian "Occam's Razor". This is illustrated with a simple example involving what Jaynes called a "sure thing" hypothesis. Jaynes' resolution of the situation involved introducing a large number of alternative "sure thing" hypotheses that were possible before we observed the data. However, in more complex situations, it may not be possible to explicitly enumerate large numbers of alternatives. The entropic priors formalism produces the desired result without modifying the hypothesis space or requiring explicit enumeration of alternatives; all that is required is a good model for the prior predictive distribution for the data. This idea is illustrated with a simple rigged-lottery example, and we outline how this idea may help to resolve a recent debate amongst cosmologists: is dark energy a cosmological constant, or has it evolved with time in some way? And how shall we decide, when the data are in?
引用
收藏
页码:179 / +
页数:2
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