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Rotating Hairy Blach holes


The present project serves the purpose of the construction of new types of rotating black holes with scalar hair, and the investigation of their physical properties. These represent solutions of Einstein gravity coupled to a (possibly self-interacting) complex scalar field in asymptotically flat 4dspacetime. A further aim of the project is to construct rotating hairy dyonic black holes in Einstein-Klein-Gordon theory and in Einstein-Skyrme theory, and to analyze the parameter space of these solutions. (AU)

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Scientific publications
(References retrieved automatically from Web of Science and SciELO through information on FAPESP grants and their corresponding numbers as mentioned in the publications by the authors)
FERREIRA, L. A.; SHNIR, YA. Exact self-dual skyrmions. Physics Letters B, v. 772, p. 621-627, SEP 10 2017. Web of Science Citations: 5.
SAMOILENKA, A.; SHNIR, YA. Gauged baby Skyrme model with a Chern-Simons term. Physical Review D, v. 95, n. 4 FEB 6 2017. Web of Science Citations: 6.
PERAPECHKA, I.; SHNIR, YA. Generalized Skyrmions and hairy black holes in asymptotically AdS(4) spacetime. Physical Review D, v. 95, n. 2 JAN 30 2017. Web of Science Citations: 8.

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