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GR: Fachverband Gravitation und Relativitätstheorie
GR 11: Black Holes
GR 11.1: Vortrag
Donnerstag, 22. März 2018, 14:00–14:20, NW-Bau - HS3
Solitons and Black Holes in 5d Einstein-Maxwell-Chern-Simons Theory — Jose Luis Blazquez-Salcedo1, •Jutta Kunz1, Francisco Navarro-Lerida2, and Eugen Radu3 — 1Universität Oldenburg, Germany — 2Universidad Complutense de Madrid, Spain — 3Universidade de Aveiro, Portugal
We consider black holes in 5-dimensional Einstein-Maxwell-Chern-Simons (EMCS) theory in the presence of a negative cosmological constant. These possess equal-magnitude angular momenta and a non-trivial magnetic field at spatial infinity. Their boundary metric corresponds to the product of time and a squashed 3-dimensional sphere. The black holes are then described by their mass, angular momenta, electric charge, magnetic flux, and squashing parameter. Under certain conditions globally regular solitonic configurations are approached. Supersymmetric solutions arise as well.