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• W1964900193 abstract "We give a new theoretical basis for examination of the presence of the Kerr black hole (KBH) or the Kerr naked singularity (KNS) in the central engine of different astrophysical objects around which astrophysical jets are typically formed: X-ray binary systems, gamma ray bursts (GRBs), active galactic nuclei (AGN), etc. Our method is based on the study of the exact solutions of the Teukolsky master equation for electromagnetic perturbations of the Kerr metric. By imposing original boundary conditions on the solutions so that they describe a collimated electromagnetic outflow, we obtain the spectra of possible primary jets of radiation, introduced here for the first time. The theoretical spectra of primary electromagnetic jets are calculated numerically. Our main result is a detailed description of the qualitative change of the behavior of primary electromagnetic jet frequencies under the transition from the KBH to the KNS, considered here as a bifurcation of the Kerr metric. We show that quite surprisingly the novel spectra describe linearly stable primary electromagnetic jets from both the KBH and the KNS. Numerical investigation of the dependence of these primary jet spectra on the rotation of the Kerr metric is presented and discussed." @default.
• W1964900193 created "2016-06-24" @default.
• W1964900193 creator A5010870214 @default.
• W1964900193 creator A5057528185 @default.
• W1964900193 date "2010-11-17" @default.
• W1964900193 modified "2023-09-26" @default.
• W1964900193 title "The spectrum of electromagnetic jets from Kerr black holes and naked singularities in the Teukolsky perturbation theory" @default.
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• W1964900193 doi "https://doi.org/10.1007/s10509-010-0520-x" @default.
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