<?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>2026-04-17T20:41:43Z</responseDate><request verb="GetRecord" identifier="oai:www.recercat.cat:2445/12405" metadataPrefix="oai_dc">https://recercat.cat/oai/request</request><GetRecord><record><header><identifier>oai:recercat.cat:2445/12405</identifier><datestamp>2025-12-04T20:48:42Z</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>Cosmic strings and Einstein-Rosen soliton waves</dc:title>
   <dc:creator>Garriga Torres, Jaume</dc:creator>
   <dc:creator>Verdaguer Oms, Enric, 1950-</dc:creator>
   <dc:subject>Relativitat general (Física)</dc:subject>
   <dc:subject>Matèria interstel·lar</dc:subject>
   <dc:subject>Solitons</dc:subject>
   <dc:subject>Cordes còsmiques</dc:subject>
   <dc:subject>Solucions numèriques</dc:subject>
   <dc:subject>General relativity (Physics)</dc:subject>
   <dc:subject>Interstellar matter</dc:subject>
   <dc:subject>Solitons</dc:subject>
   <dc:subject>Cosmic strings</dc:subject>
   <dc:subject>Numerical solutions</dc:subject>
   <dc:description>We consider all generalized soliton solutions of the Einstein-Rosen form in the cylindrical context. They are Petrov type-I solutions which describe solitonlike waves interacting with a line source placed on the symmetry axis. Some of the solutions develop a curvature singularity on the axis which is typical of massive line sources, whereas others just have the conical singularity revealing the presence of a static cosmic string. The analysis is based on the asymptotic behavior of the Riemann and metric tensors, the deficit angle, and a C-velocity associated to Thornes C-energy. The C-energy is found to be radiated along the null directions.</dc:description>
   <dc:date>2010-05-06T09:58:17Z</dc:date>
   <dc:date>2010-05-06T09:58:17Z</dc:date>
   <dc:date>1987</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/2445/12405</dc:identifier>
   <dc:identifier>79603</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.36.2250</dc:relation>
   <dc:relation>Physical Review D, 1987, vol. 36, núm. 8, p. 2250-2258</dc:relation>
   <dc:relation>http://dx.doi.org/10.1103/PhysRevD.36.2250</dc:relation>
   <dc:rights>(c) The American Physical Society, 1987</dc:rights>
   <dc:rights>info:eu-repo/semantics/openAccess</dc:rights>
   <dc:format>9 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>