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      <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: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: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>1029-8479</dc:identifier>
      <dc:identifier>10.1007/JHEP02(2018)061</dc:identifier>
      <dc:identifier>https://hdl.handle.net/20.500.14352/12014</dc:identifier>
      <dc:identifier>http://dx.doi.org/10.1007/JHEP02(2018)061</dc:identifier>
      <dc:identifier>https://link.springer.com/</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>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>Springer</dc:publisher>
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