Uncertainty quantification of mass models using ensemble Bayesian model averaging

被引:1
|
作者
Saito, Yukiya [1 ,2 ,3 ,4 ]
Dillmann, I. [1 ,5 ]
Krucken, R.
Mumpower, M. R. [6 ,7 ]
Surman, R. [3 ]
机构
[1] TRIUMF, 4004 Wesbrook Mall, Vancouver, BC V6T 2A3, Canada
[2] Univ British Columbia, Dept Phys & Astron, Vancouver, BC V6T 1Z1, Canada
[3] Univ Notre Dame, Dept Phys, Notre Dame, IN 46556 USA
[4] Univ Tennessee, Dept Phys & Astron, Knoxville, TN 37996 USA
[5] Univ Victoria, Dept Phys & Astron, Victoria, BC V8P 5C2, Canada
[6] Los Alamos Natl Lab, Theoret Div, Los Alamos, NM 87545 USA
[7] Los Alamos Natl Lab, Ctr Theoret Astrophys, Los Alamos, NM 87545 USA
基金
加拿大自然科学与工程研究理事会; 美国国家科学基金会;
关键词
GROUND-STATE MASSES; NUCLEAR; FORMULA; IMPACT;
D O I
10.1103/PhysRevC.109.054301
中图分类号
O57 [原子核物理学、高能物理学];
学科分类号
070202 ;
摘要
Developments in the description of the masses of atomic nuclei have led to various nuclear mass models that provide predictions for masses across the whole chart of nuclides. These mass models play an important role in understanding the synthesis of heavy elements in the rapid neutron capture (r) process. However, it is still a challenging task to estimate the size of uncertainty associated with the predictions of each mass model. In this work, a method called ensemble Bayesian model averaging (EBMA) is introduced to quantify the uncertainty of one-neutron separation energies (S1n) which are directly relevant in the calculations of r-process observables. This Bayesian method provides a natural way to perform model averaging, selection, and uncertainty quantification, by combining the mass models as a mixture of normal distributions whose parameters are optimized against the experimental data, employing the Markov chain Monte Carlo method using the no-u-turn sampler. The EBMA model optimized with all the experimental S1n from the AME2003 nuclides are shown to provide reliable uncertainty estimates when tested with the new data in the AME2020.
引用
收藏
页数:14
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