<?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>2026-06-27T06:05:27Z</responseDate><request verb="GetRecord" identifier="oai:docta.ucm.es:20.500.14352/60927" metadataPrefix="mods">https://docta.ucm.es/rest/oai/request</request><GetRecord><record><header><identifier>oai:docta.ucm.es:20.500.14352/60927</identifier><datestamp>2023-09-07T19:14:48Z</datestamp><setSpec>com_20.500.14352_14</setSpec><setSpec>col_20.500.14352_21</setSpec></header><metadata><mods:mods xmlns:mods="http://www.loc.gov/mods/v3" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns:doc="http://www.lyncode.com/xoai" xsi:schemaLocation="http://www.loc.gov/mods/v3 http://www.loc.gov/standards/mods/v3/mods-3-1.xsd">
   <mods:name>
      <mods:namePart>Gómez Nicola, Ángel</mods:namePart>
   </mods:name>
   <mods:extension>
      <mods:dateAvailable encoding="iso8601">2023-06-20T21:11:29Z</mods:dateAvailable>
   </mods:extension>
   <mods:extension>
      <mods:dateAccessioned encoding="iso8601">2023-06-20T21:11:29Z</mods:dateAccessioned>
   </mods:extension>
   <mods:originInfo>
      <mods:dateIssued encoding="iso8601">1999-03-11</mods:dateIssued>
   </mods:originInfo>
   <mods:identifier type="isbn">1-56396-927-0</mods:identifier>
   <mods:identifier type="doi">10.1063/1.1303025</mods:identifier>
   <mods:identifier type="uri">https://hdl.handle.net/20.500.14352/60927</mods:identifier>
   <mods:identifier type="officialurl">http://dx.doi.org/10.1063/1.1303025</mods:identifier>
   <mods:identifier type="relatedurl">http://scitation.aip.org</mods:identifier>
   <mods:identifier type="relatedurl">http://arxiv.org/abs/hep-ph/9910533</mods:identifier>
   <mods:abstract>We analyse the extension of Chiral Perturbation Theory to describe a meson gas out of thermal equilibrium. For that purpose, se let the pion decay constant be a time-dependent function and work within the Schwinger-Keldysh contour technique. A useful connection with curved space-time QFT allows to consistently renormalise the model, introducing two new low-energy constants in the chiral limit. We discuss the applicability of our approach within a Relativistic Heavy-Ion Collision environment. In particular, we investigate the formation of Disoriented Chiral Condensate domains in this model, via the parametric resonance mechanism.</mods:abstract>
   <mods:language>
      <mods:languageTerm>eng</mods:languageTerm>
   </mods:language>
   <mods:accessCondition type="useAndReproduction">open access</mods:accessCondition>
   <mods:titleInfo>
      <mods:title>Nonequilibrium chiral perturbation theory and disoriented chiral condensates</mods:title>
   </mods:titleInfo>
   <mods:genre>book part</mods:genre>
</mods:mods></metadata></record></GetRecord></OAI-PMH>