Automating the ABCD method with machine learning

被引:32
|
作者
Kasieczka, Gregor [1 ]
Nachman, Benjamin [2 ]
Schwartz, Matthew D. [3 ]
Shih, David [2 ,4 ,5 ]
机构
[1] Univ Hamburg, Inst Expt Phys, Luruper Chaussee 149, D-22761 Hamburg, Germany
[2] Lawrence Berkeley Natl Lab, Phys Div, Berkeley, CA 94720 USA
[3] Harvard Univ, Dept Phys, Cambridge, MA 02138 USA
[4] Rutgers State Univ, Dept Phys & Astron, NHETC, Piscataway, NJ 08854 USA
[5] Univ Calif Berkeley, Berkeley Ctr Theoret Phys, Berkeley, CA 94720 USA
关键词
PHYSICS; UNCERTAINTIES; SEARCHES;
D O I
10.1103/PhysRevD.103.035021
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The ABCD method is one of the most widely used data-driven background estimation techniques in high energy physics. Cuts on two statistically independent classifiers separate signal and background into four regions, so that background in the signal region can be estimated simply using the other three control regions. Typically, the independent classifiers are chosen "by hand" to be intuitive and physically motivated variables. Here, we explore the possibility of automating the design of one or both of these classifiers using machine learning. We show how to use state-of-the-art decorrelation methods to construct powerful yet independent discriminators. Along the way, we uncover a previously unappreciated aspect of the ABCD method: its accuracy hinges on having low signal contamination in control regions not just overall, but relative to the signal fraction in the signal region. We demonstrate the method with three examples: a simple model consisting of three-dimensional Gaussians; boosted hadronic top jet tagging; and a recasted search for paired dijet resonances. In all cases, automating the ABCD method with machine learning significantly improves performance in terms of ABCD closure, background rejection, and signal contamination.
引用
收藏
页数:20
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