<?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>2026-06-28T04:47:48Z</responseDate><request verb="GetRecord" identifier="oai:docta.ucm.es:20.500.14352/6078" metadataPrefix="qdc">https://docta.ucm.es/rest/oai/request</request><GetRecord><record><header><identifier>oai:docta.ucm.es:20.500.14352/6078</identifier><datestamp>2023-08-26T19:31:22Z</datestamp><setSpec>com_20.500.14352_14</setSpec><setSpec>col_20.500.14352_15</setSpec></header><metadata><qdc:qualifieddc xmlns:qdc="http://dspace.org/qualifieddc/" xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:dcterms="http://purl.org/dc/terms/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns:doc="http://www.lyncode.com/xoai" xsi:schemaLocation="http://purl.org/dc/elements/1.1/ http://dublincore.org/schemas/xmls/qdc/2006/01/06/dc.xsd http://purl.org/dc/terms/ http://dublincore.org/schemas/xmls/qdc/2006/01/06/dcterms.xsd http://dspace.org/qualifieddc/ http://www.ukoln.ac.uk/metadata/dcmi/xmlschema/qualifieddc.xsd">
   <dc:title>Quantum corrections to minimal surfaces with mixed three-form flux</dc:title>
   <dc:creator>Hernández Redondo, Rafael</dc:creator>
   <dc:creator>Miguel Nieto, Juan</dc:creator>
   <dc:creator>Ruiz Gil, Roberto</dc:creator>
   <dcterms:abstract>We obtain the ratio of semiclassical partition functions for the extension under mixed flux of the minimal surfaces subtending a circumference and a line in Euclidean AdS(3) x S-3 x T-4. We reduce the problem to the computation of a set of functional determinants. If the Ramond-Ramond flux does not vanish, we find that the contribution of the B-field is comprised in the conformal anomaly. In this case, we successively apply the Gel'fand-Yaglom method and the Abel-Plana formula to the flat-measure determinants. To cancel the resultant infrared divergences, we shift the regularization of the sum over half-integers depending on whether it corresponds to massive or massless fermionic modes. We show that the result is compatible with the zeta-function regularization approach. In the limit of pure Neveu-Schwarz-Neveu-Schwarz flux we argue that the computation trivializes. We extend the reasoning to other surfaces with the same behavior in this regime.</dcterms:abstract>
   <dcterms:dateAccepted>2023-06-16T15:16:10Z</dcterms:dateAccepted>
   <dcterms:available>2023-06-16T15:16:10Z</dcterms:available>
   <dcterms:created>2023-06-16T15:16:10Z</dcterms:created>
   <dcterms:issued>2020-01-27</dcterms:issued>
   <dc:type>journal article</dc:type>
   <dc:identifier>https://hdl.handle.net/20.500.14352/6078</dc:identifier>
   <dc:identifier>2470-0045</dc:identifier>
   <dc:identifier>10.1103/PhysRevD.101.026019</dc:identifier>
   <dc:language>eng</dc:language>
   <dc:relation>PGC2018-095382-B-I00</dc:relation>
   <dc:relation>GR3/14-A 910770</dc:relation>
   <dc:relation>EP/S020888/1</dc:relation>
   <dc:rights>https://creativecommons.org/licenses/by/3.0/es/</dc:rights>
   <dc:rights>open access</dc:rights>
   <dc:rights>Atribución 3.0 España</dc:rights>
   <dc:publisher>American Physical Society</dc:publisher>
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