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Bayesian Statistics at Work: the Troublesome Extraction of the CKM Phase alpha

In Bayesian statistics, one's prior beliefs about underlying model parameters are revised with the information content of observed data from which, using Bayes' rule, a posterior belief is obtained. A non-trivial example taken from the isospin analysis of B->PP (P = pi or rho) decays in...

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Autores principales: Charles, J, Höcker, A, Lacker, L, Le Diberder, F R, T'Jampens, S
Lenguaje:eng
Publicado: 2006
Materias:
Acceso en línea:http://cds.cern.ch/record/973852
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author Charles, J
Höcker, A
Lacker, L
Le Diberder, F R
T'Jampens, S
author_facet Charles, J
Höcker, A
Lacker, L
Le Diberder, F R
T'Jampens, S
author_sort Charles, J
collection CERN
description In Bayesian statistics, one's prior beliefs about underlying model parameters are revised with the information content of observed data from which, using Bayes' rule, a posterior belief is obtained. A non-trivial example taken from the isospin analysis of B->PP (P = pi or rho) decays in heavy-flavor physics is chosen to illustrate the effect of the naive "objective" choice of flat priors in a multi-dimensional parameter space in presence of mirror solutions. It is demonstrated that the posterior distribution for the parameter of interest, the phase alpha strongly depends on the choice of the parameterization in which the priors are uniform, and on the validity range in which the (un-normalizable) priors are truncated. We prove that the most probable values found by the Bayesian treatment do not coincide with the explicit analytical solution, in contrast to the frequentist approach. It is also shown in the appendix that the alpha->0 limit cannot be consistently treated in the Bayesian paradigm, because the latter violates the physical symmetries of the problem.
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institution Organización Europea para la Investigación Nuclear
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spelling cern-9738522019-09-30T06:29:59Zhttp://cds.cern.ch/record/973852engCharles, JHöcker, ALacker, LLe Diberder, F RT'Jampens, SBayesian Statistics at Work: the Troublesome Extraction of the CKM Phase alphaParticle Physics - PhenomenologyIn Bayesian statistics, one's prior beliefs about underlying model parameters are revised with the information content of observed data from which, using Bayes' rule, a posterior belief is obtained. A non-trivial example taken from the isospin analysis of B->PP (P = pi or rho) decays in heavy-flavor physics is chosen to illustrate the effect of the naive "objective" choice of flat priors in a multi-dimensional parameter space in presence of mirror solutions. It is demonstrated that the posterior distribution for the parameter of interest, the phase alpha strongly depends on the choice of the parameterization in which the priors are uniform, and on the validity range in which the (un-normalizable) priors are truncated. We prove that the most probable values found by the Bayesian treatment do not coincide with the explicit analytical solution, in contrast to the frequentist approach. It is also shown in the appendix that the alpha->0 limit cannot be consistently treated in the Bayesian paradigm, because the latter violates the physical symmetries of the problem.CERN-OPEN-2006-029CPT-P-2006-56LAL-2006-122LAPP-2006-02oai:cds.cern.ch:9738522006-07-21
spellingShingle Particle Physics - Phenomenology
Charles, J
Höcker, A
Lacker, L
Le Diberder, F R
T'Jampens, S
Bayesian Statistics at Work: the Troublesome Extraction of the CKM Phase alpha
title Bayesian Statistics at Work: the Troublesome Extraction of the CKM Phase alpha
title_full Bayesian Statistics at Work: the Troublesome Extraction of the CKM Phase alpha
title_fullStr Bayesian Statistics at Work: the Troublesome Extraction of the CKM Phase alpha
title_full_unstemmed Bayesian Statistics at Work: the Troublesome Extraction of the CKM Phase alpha
title_short Bayesian Statistics at Work: the Troublesome Extraction of the CKM Phase alpha
title_sort bayesian statistics at work: the troublesome extraction of the ckm phase alpha
topic Particle Physics - Phenomenology
url http://cds.cern.ch/record/973852
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