<?xml version="1.0" encoding="UTF-8"?><?xml-stylesheet type="text/xsl" href="static/style.xsl"?><OAI-PMH xmlns="http://www.openarchives.org/OAI/2.0/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/ http://www.openarchives.org/OAI/2.0/OAI-PMH.xsd"><responseDate>2026-04-18T03:28:54Z</responseDate><request verb="GetRecord" identifier="oai:www.recercat.cat:2445/119410" metadataPrefix="oai_dc">https://recercat.cat/oai/request</request><GetRecord><record><header><identifier>oai:recercat.cat:2445/119410</identifier><datestamp>2025-12-05T16:42:17Z</datestamp><setSpec>com_2072_1057</setSpec><setSpec>col_2072_478823</setSpec><setSpec>col_2072_478904</setSpec><setSpec>col_2072_478917</setSpec></header><metadata><oai_dc:dc xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/" xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns:doc="http://www.lyncode.com/xoai" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/ http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
   <dc:title>Search for a muonic dark force at BaBar</dc:title>
   <dc:creator>Graugés Pous, Eugeni</dc:creator>
   <dc:creator>BABAR Collaboration</dc:creator>
   <dc:subject>Partícules (Matèria)</dc:subject>
   <dc:subject>Matèria fosca (Astronomia)</dc:subject>
   <dc:subject>Particles</dc:subject>
   <dc:subject>Dark matter (Astronomy)</dc:subject>
   <dc:description>Many models of physics beyond the standard model predict the existence of new Abelian forces with new gauge bosons mediating interactions between "dark sectors" and the standard model. We report a search for a dark boson Z ′ coupling only to the second and third generations of leptons in the reaction e + e − → μ + μ − Z ′ , Z ′ → μ + μ − using 514     fb − 1 of data collected by the BABAR experiment. No significant signal is observed for Z ′ masses in the range 0.212-10 GeV. Limits on the coupling parameter g ′ as low as 7 × 10 − 4 are derived, leading to improvements in the bounds compared to those previously derived from neutrino experiments.</dc:description>
   <dc:date>2018-01-30T12:14:28Z</dc:date>
   <dc:date>2018-01-30T12:14:28Z</dc:date>
   <dc:date>2016-07-19</dc:date>
   <dc:date>2018-01-30T12:14:28Z</dc:date>
   <dc:type>info:eu-repo/semantics/article</dc:type>
   <dc:type>info:eu-repo/semantics/publishedVersion</dc:type>
   <dc:identifier>1550-7998</dc:identifier>
   <dc:identifier>https://hdl.handle.net/2445/119410</dc:identifier>
   <dc:identifier>669776</dc:identifier>
   <dc:language>eng</dc:language>
   <dc:relation>Reproducció del document publicat a: https://doi.org/10.1103/PhysRevD.94.011102</dc:relation>
   <dc:relation>Physical Review D, 2016, vol. 94, num. 1, p. 11102-1-11102-7</dc:relation>
   <dc:relation>https://doi.org/10.1103/PhysRevD.94.011102</dc:relation>
   <dc:rights>(c) American Physical Society, 2016</dc:rights>
   <dc:rights>info:eu-repo/semantics/openAccess</dc:rights>
   <dc:format>1 p.</dc:format>
   <dc:format>application/pdf</dc:format>
   <dc:publisher>American Physical Society</dc:publisher>
   <dc:source>Articles publicats en revistes (Física Quàntica i Astrofísica)</dc:source>
</oai_dc:dc></metadata></record></GetRecord></OAI-PMH>