<?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>2026-06-08T11:26:10Z</responseDate><request verb="GetRecord" identifier="oai:docta.ucm.es:20.500.14352/12014" metadataPrefix="oai_dc">https://docta.ucm.es/rest/oai/request</request><GetRecord><record><header><identifier>oai:docta.ucm.es:20.500.14352/12014</identifier><datestamp>2024-09-03T13:27:56Z</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>Squashed, magnetized black holes in D=5 minimal gauged supergravity</dc:title>
   <dc:creator>Blázquez Salcedo, José Luis</dc:creator>
   <dc:creator>Kunz, Jutta</dc:creator>
   <dc:creator>Navarro Lerida, Francisco</dc:creator>
   <dc:creator>Radu, Eugen</dc:creator>
   <dc:subject>53</dc:subject>
   <dc:subject>Cosmological constant</dc:subject>
   <dc:subject>5 dimensions</dc:subject>
   <dc:subject>Spacetimes</dc:subject>
   <dc:subject>Holography</dc:subject>
   <dc:subject>Rotation</dc:subject>
   <dc:subject>Strings</dc:subject>
   <dc:subject>Tensor.</dc:subject>
   <dc:subject>Física (Física)</dc:subject>
   <dc:subject>22 Física</dc:subject>
   <dc:description>© 2018 Springer.
We gratefully acknowledge support by the DFG Research Training Group 1620 "Models of Gravity". E. R. acknowledges funding from the FCT-IF programme. This work was also partially supported by the H2020-MSCA-RISE-2015 Grant No. StronGrHEP-690904, and by the CIDMA project UID/MAT/04106/2013. F. N.-L. acknowledges funding from Complutense University - Santander under project PR26/16-20312. J. L. B.-S. and J. K. acknowledge support from FP7, Marie Curie Actions, People, International Research Staff Exchange Scheme (IRSES-606096).</dc:description>
   <dc:description>We construct a new class of black hole solutions in five-dimensional Einstein-Maxwell-Chern-Simons theory with a negative cosmological constant. These configurations are cohomogeneity-1, with two equal-magnitude angular momenta. In the generic case, they possess a non-vanishing magnetic potential at infinity with a boundary metric which is the product of time and a squashed three-dimensional sphere. Both extremal and non-extremal black holes are studied. The non-extremal black holes satisfying a certain relation between electric charge, angular momenta and magnitude of the magnetic potential at infinity do not trivialize in the limit of vanishing event horizon size, becoming particle-like (non-topological) solitonic configurations. Among the extremal black holes, we show the existence of a new one-parameter family of supersymmetric solutions, which bifurcate from a critical Gutowski-Reall configuration.</dc:description>
   <dc:description>Unión Europea. H2020</dc:description>
   <dc:description>Unión Europea. FP7</dc:description>
   <dc:description>DFG Research Training Group</dc:description>
   <dc:description>FCT-IF programme</dc:description>
   <dc:description>CIDMA</dc:description>
   <dc:description>Universidad Complutense de Madrid/Banco de Santander</dc:description>
   <dc:description>Depto. de Física Teórica</dc:description>
   <dc:description>Fac. de Ciencias Físicas</dc:description>
   <dc:description>TRUE</dc:description>
   <dc:description>pub</dc:description>
   <dc:date>2023-06-17T12:26:30Z</dc:date>
   <dc:date>2023-06-17T12:26:30Z</dc:date>
   <dc:date>2018-02-09</dc:date>
   <dc:type>journal article</dc:type>
   <dc:identifier>https://hdl.handle.net/20.500.14352/12014</dc:identifier>
   <dc:identifier>1029-8479</dc:identifier>
   <dc:identifier>10.1007/JHEP02(2018)061</dc:identifier>
   <dc:language>eng</dc:language>
   <dc:relation>StronGrHEP (690904)</dc:relation>
   <dc:relation>IRSES (606096)</dc:relation>
   <dc:relation>1620</dc:relation>
   <dc:relation>UID/MAT/04106/2013</dc:relation>
   <dc:relation>PR26/16-20312</dc:relation>
   <dc:rights>Atribución 3.0 España</dc:rights>
   <dc:rights>https://creativecommons.org/licenses/by/3.0/es/</dc:rights>
   <dc:rights>open access</dc:rights>
   <dc:format>application/pdf</dc:format>
   <dc:publisher>Springer</dc:publisher>
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