<?xml version="1.0" encoding="UTF-8"?><rdf:RDF xmlns:rdf="http://www.w3.org/1999/02/22-rdf-syntax-ns#" xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:dcq="http://purl.org/dc/terms/"><records count="1" morepages="false" start="1" end="1"><record rownumber="1"><dc:product_type>Journal Article</dc:product_type><dc:title>Infrared-safe energy weighting does not guarantee small nonperturbative effects</dc:title><dc:creator>Bright-Thonney, Samuel; Nachman, Benjamin; Thaler, Jesse</dc:creator><dc:corporate_author/><dc:editor/><dc:description>&lt;p&gt;Infrared and collinear (IRC) safety has long been used a proxy for robustness when developing new jet substructure observables. This guiding philosophy has been carried into the deep learning era, where IRC-safe neural networks have been used for many jet studies. For graph-based neural networks, the most straightforward way to achieve IRC safety is to weight particle inputs by their energies. However, energy-weighting by itself does not guarantee that perturbative calculations of machine-learned observables will enjoy small nonperturbative corrections. In this paper, we demonstrate the sensitivity of IRC-safe networks to nonperturbative effects, by training an energy flow network (EFN) to maximize its sensitivity to hadronization. We then show how to construct Lipschitz energy flow networks (&lt;math display='inline'&gt;&lt;mrow&gt;&lt;mi&gt;L&lt;/mi&gt;&lt;/mrow&gt;&lt;/math&gt;-EFNs), which are both IRC safe and relatively insensitive to nonperturbative corrections. We demonstrate the performance of&lt;math display='inline'&gt;&lt;mi&gt;L&lt;/mi&gt;&lt;/math&gt;-EFNs on generated samples of quark and gluon jets, and showcase fascinating differences between the learned latent representations of EFNs and&lt;math display='inline'&gt;&lt;mi&gt;L&lt;/mi&gt;&lt;/math&gt;-EFNs.&lt;/p&gt; &lt;sec&gt;&lt;supplementary-material&gt;&lt;permissions&gt;&lt;copyright-statement&gt;Published by the American Physical Society&lt;/copyright-statement&gt;&lt;copyright-year&gt;2024&lt;/copyright-year&gt;&lt;/permissions&gt;&lt;/supplementary-material&gt;&lt;/sec&gt;</dc:description><dc:publisher>American Physical Society</dc:publisher><dc:date>2024-07-01</dc:date><dc:nsf_par_id>10532075</dc:nsf_par_id><dc:journal_name>Physical Review D</dc:journal_name><dc:journal_volume>110</dc:journal_volume><dc:journal_issue>1</dc:journal_issue><dc:page_range_or_elocation/><dc:issn>2470-0010</dc:issn><dc:isbn/><dc:doi>https://doi.org/10.1103/PhysRevD.110.014029</dc:doi><dcq:identifierAwardId>2209443; 2019786</dcq:identifierAwardId><dc:subject/><dc:version_number/><dc:location/><dc:rights/><dc:institution/><dc:sponsoring_org>National Science Foundation</dc:sponsoring_org></record></records></rdf:RDF>