<?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>A Distance Conjecture for branes</dc:title><dc:creator>Etheredge, Muldrow (ORCID:0000000151446238); Heidenreich, Ben (ORCID:0000000305369985); Rudelius, Tom (ORCID:0000000289122789)</dc:creator><dc:corporate_author/><dc:editor/><dc:description>We use branes to generalize the Distance Conjecture. We conjecture that in any infinite-distance limit in the moduli space of a d-dimensional quantum gravity theory, among the set of particle towers and fundamental branes with at most pmax spacetime dimensions (where pmax is an integer between 1 and d-2), at least one has mass/tension decreasing exponentially T ~ exp(–α ∆) with the moduli space distance ∆ at a rate of at least α ≥ 1/sqrt(d-pmax-1). Since pmax can vary, this represents multiple conditions, where the Sharpened Distance Conjecture is the pmax = 1 case. This conjecture is a necessary condition imposed on higher-dimensional theories in order for the Sharpened Distance Conjecture to hold in lower-dimensional theories. We test our conjecture in theories with maximal and half-maximal supersymmetry in diverse dimensions, finding that it is satisfied and often saturated. In some cases where it is saturated — most notably, heterotic string theory in 10 dimensions — we argue that novel, low-tension non-supersymmetric branes must exist. We also identify patterns relating the rates at which various brane tensions vary in infinite-distance limits and relate these tensions to the species scale.</dc:description><dc:publisher>Springer</dc:publisher><dc:date>2025-09-18</dc:date><dc:nsf_par_id>10646705</dc:nsf_par_id><dc:journal_name>Journal of High Energy Physics</dc:journal_name><dc:journal_volume>2025</dc:journal_volume><dc:journal_issue>9</dc:journal_issue><dc:page_range_or_elocation/><dc:issn>1029-8479</dc:issn><dc:isbn/><dc:doi>https://doi.org/10.1007/JHEP09(2025)155</dc:doi><dcq:identifierAwardId>2112800; 2412570</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>