Speaker
Stanislav Komarov
(Belarusian State University)
Description
The charged axially-symmetric conductor with charge in the vicinity of Kerr black hole is considered. The electromagnetic field of this conductor in the form of multipole expansion is calculated by using the Teukolsky equation. The structure of electric and magnetic field lines is analyzed. The case when conductor is located almost at the event horizon is considered. The astrophysical applications of the results are discussed.
Author
Stanislav Komarov
(Belarusian State University)
Co-authors
Prof.
Alexander Gorbatsievich
(Belarusian State University)
Dr
Alexander Garkun
(Institute of Applied Physics, National Academy of Sciences of Belarus)
Gregory Vereshchagin
(ICRANet)