贝叶斯模型选择:在基本物理常数调整中的应用

Olha Bodnar, V. Eriksson
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引用次数: 5

摘要

最初由Raymond Birge提出的一种方法,使用后来被称为Birge比率的方法,在计量学和物理学中广泛用于基本物理常数的调整,特别是在CODATA基本物理常数任务组(国际科学理事会数据委员会)进行的周期性重新评估中。该方法包括通过一个足够大的乘法因子来增加报告的不确定度,以使测量结果相互一致。另一种在医学研究的元分析中占主导地位的方法是,通过将报告的不确定性与从数据中估计的足够大的常数(通常称为暗不确定性)结合起来,利用平方根和来夸大不确定性。在这篇文章中,我们建立了基于Birge比率的方法与位置尺度模型之间的联系,这使得人们可以结合各种研究的结果,而在随机效应模型的通常背景下对加性调整进行了审查。将这些替代方法作为统计模型,便于使用用于模型比较的统计工具对它们进行定量比较。根据Berger和Bernardo先前的参考推导出内在贝叶斯因子(IBF),然后用它来为牛顿引力常数(“大G”)的一组测量选择一个模型,以估计该常数的一致值并评估相关的不确定性。我们的实证结果支持基于比奇比率的方法。使用Jeffreys先验所对应的IBF和基于赤池信息准则(Akaike information criterion, AIC)进行比较得到了相同的结论。最后,仿真研究结果表明,即使数据仅包含少量测量值,所建议的模型选择过程也能提供明确的指导。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Bayesian model selection: Application to the adjustment of fundamental physical constants
A method originally suggested by Raymond Birge, using what came to be known as the Birge ratio , has been widely used in metrology and physics for the adjustment of fundamental physical constants, particularly in the pe-riodic reevaluation carried out by the Task Group on Fundamental Physical Constants of CODATA (the Committee on Data of the International Science Council). The method involves increasing the reported uncertainties by a multiplicative factor large enough to make the measurement results mutually con-sistent. An alternative approach, predominant in the meta-analysis of medical studies, involves inflating the reported uncertainties by combining them, using the root sum of squares, with a sufficiently large constant (often dubbed dark uncertainty ) that is estimated from the data. In this contribution, we establish a connection between the method based on the Birge ratio and the location-scale model, which allows one to combine the results of various studies, while the additive adjustment is reviewed in the usual context of random effects models. Framing these alternative approaches as statistical models facilitates a quantitative comparison of them using statistical tools for model comparison. The intrinsic Bayes factor (IBF) is derived for the Berger and Bernardo reference prior, and then it is used to select a model for a set of measurements of the Newtonian constant of gravitation (“Big G”) to estimate a consensus value for this constant and to evaluate the associated uncertainty. Our empirical findings support the method based on the Birge ratio. The same conclusion is reached when the IBF corresponding to the Jeffreys prior is used and also when the comparison is based on the Akaike information criterion (AIC). Finally, the results of a simulation study indicate that the suggested procedure for model selection provides clear guid-ance even when the data comprise only a small number of measurements.
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