<?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>2026-04-17T17:14:24Z</responseDate><request verb="GetRecord" identifier="oai:www.recercat.cat:2445/12400" metadataPrefix="oai_dc">https://recercat.cat/oai/request</request><GetRecord><record><header><identifier>oai:recercat.cat:2445/12400</identifier><datestamp>2025-12-04T20:45:29Z</datestamp><setSpec>com_2072_1057</setSpec><setSpec>col_2072_478822</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>Classical cross sections for relativistic spinning particles</dc:title>
   <dc:creator>Bona, Carles</dc:creator>
   <dc:creator>Fustero, X. (Xavier)</dc:creator>
   <dc:creator>Verdaguer Oms, Enric, 1950-</dc:creator>
   <dc:subject>Electromagnetisme</dc:subject>
   <dc:subject>Gravitació</dc:subject>
   <dc:subject>Interaccions febles (Física nuclear)</dc:subject>
   <dc:subject>Partícules (Física nuclear)</dc:subject>
   <dc:subject>Electromagnetism</dc:subject>
   <dc:subject>Gravitation</dc:subject>
   <dc:subject>Weak interactions (Nuclear physics)</dc:subject>
   <dc:subject>Particles (Nuclear physics)</dc:subject>
   <dc:description>We propose a definition of classical differential cross sections for particles with essentially nonplanar orbits, such as spinning ones. We give also a method for its computation. The calculations are carried out explicitly for electromagnetic, gravitational, and short-range scalar interactions up to the linear terms in the slow-motion approximation. The contribution of the spin-spin terms is found to be at best 10-6 times the post-Newtonian ones for the gravitational interaction.</dc:description>
   <dc:date>2010-05-06T09:54:37Z</dc:date>
   <dc:date>2010-05-06T09:54:37Z</dc:date>
   <dc:date>1983</dc:date>
   <dc:type>info:eu-repo/semantics/article</dc:type>
   <dc:type>info:eu-repo/semantics/publishedVersion</dc:type>
   <dc:identifier>0556-2821</dc:identifier>
   <dc:identifier>https://hdl.handle.net/2445/12400</dc:identifier>
   <dc:identifier>79587</dc:identifier>
   <dc:language>eng</dc:language>
   <dc:relation>Reproducció digital del document publicat en format paper, proporcionada per PROLA i http://dx.doi.org/10.1103/PhysRevD.28.317</dc:relation>
   <dc:relation>Physical Review D, 1983, vol. 28, núm. 2, p. 317-324</dc:relation>
   <dc:relation>http://dx.doi.org/10.1103/PhysRevD.28.317</dc:relation>
   <dc:rights>(c) The American Physical Society, 1983</dc:rights>
   <dc:rights>info:eu-repo/semantics/openAccess</dc:rights>
   <dc:format>8 p.</dc:format>
   <dc:format>application/pdf</dc:format>
   <dc:publisher>The American Physical Society</dc:publisher>
   <dc:source>Articles publicats en revistes (Física de la Matèria Condensada)</dc:source>
</oai_dc:dc></metadata></record></GetRecord></OAI-PMH>