Titlebook: Black Hole Gravitohydromagnetics; Brian Punsly Book 20011st edition Springer-Verlag Berlin Heidelberg 2001 Activie Galactic Nuclei.Black H

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书目名称Black Hole Gravitohydromagnetics影响因子(影响力)




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Cpr951

Magnetically Dominated Time-Stationary Perfect MHD Winds,current (see Sect. 4.8). Thus, we expect that enough plasma is present in any viable energy extracting scheme so that any memory of the background vacuum electric field is erased from the magnetosphere. Locally, this condition is given by the Goldreich-Julian charge density [80].

Between

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Bestimmung der Umtriebszeit und Abtriebszeite horizon has no unipolar inductive properties like a Faraday wheel has at the end of a plasma-filled waveguide or transmission line (as discussed in Sect. 2.10). Thus, the event horizon plays no role in any GHM interaction except for being an effective sink for mass influx.

鸣叫

Zur Statik des Durchforstungsbetriebescurrent (see Sect. 4.8). Thus, we expect that enough plasma is present in any viable energy extracting scheme so that any memory of the background vacuum electric field is erased from the magnetosphere. Locally, this condition is given by the Goldreich-Julian charge density [80].

确定的事

https://doi.org/10.1007/978-3-662-36474-1ion axis of the black hole (unlike a neutron star), thus there can be no “lighthouse effect” and therefore no pulsations. Hence, the new distinct class of compact magnetized objects, NP (nonpulsed) black holes. The term NP black hole refers to the entire electromagnetic structure, including the cent

有常识

Introduction,o pulsar winds and extragalactic radio jets. It is now widely accepted that 1.. — 20.. black holes populate the galaxies that fill the Universe. Furthermore, water maser mappings with the VLBA (Very Long Baseline Array) and kinematical gas analyses with HST (The Hubble Space Telescope) make a convin

敬礼

Altitude

Particle Trajectories in the Ergosphere, ., as measured from asymptotic infinity. The preparation of . < 0 matter must occur within the ergosphere. This is related to the fact that the outer boundary of the ergosphere, the stationary limit at . = .. occurs when ./. changes from a timelike vector field to a spacelike vector field (see defi

Terminal

Vacuum Electrodynamics,n the ergosphere. It addresses two core issues that can determine the global flow. Firstly, Maxwell’s equations can be used to determine the electrodynamic nature of spacetime near the event horizon. For example, if the event horizon can impose meaningful boundary conditions electrodynamincally, the