Complete Optimal Non-Resonant Anomaly Detection

Fuente: arXiv
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Autori principali: Kasieczka, Gregor, Raine, John Andrew, Shih, David, Upadhyay, Aman
Natura: Preprint
Pubblicazione: 2024
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author Kasieczka, Gregor
Raine, John Andrew
Shih, David
Upadhyay, Aman
author_facet Kasieczka, Gregor
Raine, John Andrew
Shih, David
Upadhyay, Aman
contents We propose the first-ever complete, model-agnostic search strategy based on the optimal anomaly score, for new physics on the tails of distributions. Signal sensitivity is achieved via a classifier trained on auxiliary features in a weakly-supervised fashion, and backgrounds are predicted using the ABCD method in the classifier output and the primary tail feature. The independence between the classifier output and the tail feature required for ABCD is achieved by first training a conditional normalizing flow that yields a decorrelated version of the auxiliary features; the classifier is then trained on these features. Both the signal sensitivity and background prediction require a sample of events accurately approximating the SM background; we assume this can be furnished by closely related control processes in the data or by accurate simulations, as is the case in countless conventional analyses. The viability of our approach is demonstrated for signatures consisting of (mono)jets and missing transverse energy, where the main SM background is $Z(νν) +\text{jets}$, and the data-driven control process is $γ+\text{jets}$.
format Preprint
id arxiv_https___arxiv_org_abs_2404_07258
institution arXiv
publishDate 2024
record_format arxiv
spellingShingle Complete Optimal Non-Resonant Anomaly Detection
Kasieczka, Gregor
Raine, John Andrew
Shih, David
Upadhyay, Aman
High Energy Physics - Phenomenology
High Energy Physics - Experiment
Data Analysis, Statistics and Probability
We propose the first-ever complete, model-agnostic search strategy based on the optimal anomaly score, for new physics on the tails of distributions. Signal sensitivity is achieved via a classifier trained on auxiliary features in a weakly-supervised fashion, and backgrounds are predicted using the ABCD method in the classifier output and the primary tail feature. The independence between the classifier output and the tail feature required for ABCD is achieved by first training a conditional normalizing flow that yields a decorrelated version of the auxiliary features; the classifier is then trained on these features. Both the signal sensitivity and background prediction require a sample of events accurately approximating the SM background; we assume this can be furnished by closely related control processes in the data or by accurate simulations, as is the case in countless conventional analyses. The viability of our approach is demonstrated for signatures consisting of (mono)jets and missing transverse energy, where the main SM background is $Z(νν) +\text{jets}$, and the data-driven control process is $γ+\text{jets}$.
title Complete Optimal Non-Resonant Anomaly Detection
topic High Energy Physics - Phenomenology
High Energy Physics - Experiment
Data Analysis, Statistics and Probability
url https://arxiv.org/abs/2404.07258