General-Relativistic MHD Simulation of Jets from a Geometrically Thin Accretion Disk Around a Schwarzschild Black Hole
2000 ◽
Vol 195
◽
pp. 373-374
Keyword(s):
We have performed a 2.5D, nonsteady, general-relativistic MHD simulation. Initially, we assumed a uniform magnetic field, a geometrically thin accretion disk rotating at Keplerian velocity, and a hydrostatic corona around a Schwarzschild black hole. We have investigated the formation mechanism of gas-pressure driven jets expected by Koide et al. and found the strong dependence of jet velocities Lorentz factor of jets) on the ratio of the density of the accretion disk to that of the corona (ρd/ρc), where γ2j - γj ∝ (ρd/ρc)0.75.
2000 ◽
Vol 15
(19)
◽
pp. 2979-2986
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1997 ◽
Vol 163
◽
pp. 667-671
Keyword(s):
2015 ◽
Vol 32
(16)
◽
pp. 165009
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Keyword(s):
2007 ◽
Vol 22
(10)
◽
pp. 1875-1898
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Keyword(s):
2006 ◽
Vol 2
(S238)
◽
pp. 367-368