<?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>2026-06-29T08:02:32Z</responseDate><request verb="GetRecord" identifier="oai:docta.ucm.es:20.500.14352/113585" metadataPrefix="oai_dc">https://docta.ucm.es/rest/oai/request</request><GetRecord><record><header><identifier>oai:docta.ucm.es:20.500.14352/113585</identifier><datestamp>2025-01-10T01:10:10Z</datestamp><setSpec>com_20.500.14352_14</setSpec><setSpec>col_20.500.14352_15</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>States of low energy in the Schwinger effect</dc:title>
   <dc:creator>Álvarez Domínguez, Álvaro</dc:creator>
   <dc:creator>Garay Elizondo, Luis Javier</dc:creator>
   <dc:creator>Martín Benito, Mercedes</dc:creator>
   <dc:creator>Neves, Rita B.</dc:creator>
   <dc:subject>53</dc:subject>
   <dc:subject>Nonperturbative effects</dc:subject>
   <dc:subject>Cosmological models</dc:subject>
   <dc:subject>Particle creation</dc:subject>
   <dc:subject>Quantum</dc:subject>
   <dc:subject>Field</dc:subject>
   <dc:subject>Física (Física)</dc:subject>
   <dc:subject>2212 Física Teórica</dc:subject>
   <dc:description>SFRH/BD/143525/2019</dc:description>
   <dc:description>States of low energy in cosmology minimise the energy density when smeared in a chosen time interval. We extend such construction to generic homogeneous (possibly anisotropic) particle creation settings. Focusing on the Schwinger effect, we study the role played by the support of the smearing function and identify the vacua obtained in the limiting cases of small and large time intervals. We also analyse the spectral properties of the power spectrum and the number of created particles, which are complementary in characterising the vacuum, and investigate the multipolar contributions coming from the anisotropies.</dc:description>
   <dc:description>Ministerio de Ciencia e Investigación (España)</dc:description>
   <dc:description>Agencia Estatal de Investigación (España)</dc:description>
   <dc:description>Fundação para a Ciência e a Tecnologia (Portugal)</dc:description>
   <dc:description>Depto. de Física Teórica</dc:description>
   <dc:description>Fac. de Ciencias Físicas</dc:description>
   <dc:description>Instituto de Física de Partículas y del Cosmos (IPARCOS)</dc:description>
   <dc:description>TRUE</dc:description>
   <dc:description>pub</dc:description>
   <dc:date>2025-01-09T17:07:15Z</dc:date>
   <dc:date>2025-01-09T17:07:15Z</dc:date>
   <dc:date>2023-06-15</dc:date>
   <dc:type>journal article</dc:type>
   <dc:type>VoR</dc:type>
   <dc:identifier>https://hdl.handle.net/20.500.14352/113585</dc:identifier>
   <dc:identifier>1126-6708</dc:identifier>
   <dc:identifier>10.1007/jhep06(2023)093</dc:identifier>
   <dc:identifier>1029-8479</dc:identifier>
   <dc:language>eng</dc:language>
   <dc:relation>info:eu-repo/grantAgreement/AEI/Plan Estatal de Investigación Científica y Técnica y de Innovación 2017-2020/PID2020-118159GB-C44/ES/UNIVERSO CUANTICO GRAVITATORIO: CAMPOS, LAZOS Y GRAVEDAD DE WEYL/</dc:relation>
   <dc:relation>Álvarez-Domínguez, Á., Garay, L.J., Martín-Benito, M. et al. States of low energy in the Schwinger effect. J. High Energ. Phys. 2023, 93 (2023). https://doi.org/10.1007/JHEP06(2023)093</dc:relation>
   <dc:rights>Attribution 4.0 International</dc:rights>
   <dc:rights>http://creativecommons.org/licenses/by/4.0/</dc:rights>
   <dc:rights>open access</dc:rights>
   <dc:format>application/pdf</dc:format>
   <dc:publisher>Springer</dc:publisher>
</oai_dc:dc></metadata></record></GetRecord></OAI-PMH>