2026-06-08T08:27:05Zhttps://docta.ucm.es/rest/oai/request

oai:docta.ucm.es:20.500.14352/120142024-09-03T13:27:56Zcom_20.500.14352_14col_20.500.14352_15

00925njm 22002777a 4500 dc Blázquez Salcedo, José Luis author Kunz, Jutta author Navarro Lerida, Francisco author Radu, Eugen author 2018-02-09 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. 1029-8479 10.1007/JHEP02(2018)061 https://hdl.handle.net/20.500.14352/12014 http://dx.doi.org/10.1007/JHEP02(2018)061 https://link.springer.com/ Squashed, magnetized black holes in D=5 minimal gauged supergravity