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Transcript
Mechanism that removes accretion disk angular momentum
while driving associated bi-directional astrophysical jets
P. M. Bellan1
1 Applied
Physics and Materials Science, Caltech, Pasadena CA 91125, USA
I propose a mechanism [1] that simultaneously drives astrophysical jets and
removes angular momentum from an accretion disk. The mechanism depends on
(i) the very great difference in ionization between the weakly ionized accretion
disk and the highly ionized exterior region and (ii) the complete circuit of poloidal
electric current. In the highly ionized exterior region collisionless Hamiltonian
mechanics and axisymmetry constrain charged particles to move on nested
poloidal flux surfaces whereas in the weakly ionized accretion disk particle
motion is very different. The weak ionization in the disk means that ions in the
disk collide very frequently with neutrals so any momentum a disk ion gains
electromagnetically is immediately shared with nearby neutrals. A fluid element
consisting of ions and neutrals thus behaves as if it has the charge of the ions
and the mass of the neutrals. This fluid element consequently behaves
dynamically like a collisionless meta-particle having charge to mass ratio reduced
from than that of an ion by the nominal accretion disk 10-15 – 10-8 fractional
ionization. This means that the meta-particle cyclotron frequency can be of the
order of the Kepler angular frequency in which case meta-particles with a critical
charge to mass ratio have zero canonical angular momentum. Hamiltonian
dynamics shows that meta-particles with zero canonical angular momentum
experience no centrifugal force and spiral inward towards the central body [2].
Because the metaparticles are positively charged, the accumulation of inward
spiraling meta-particles near the central body produces radially and axially
outward electric fields. The axial outward electric field drives an out-of-plane
poloidal electric current along arched poloidal flux surfaces in the collisionless
region external to the disk. This out-of-plane poloidal current and its associated
toroidal magnetic field produce forces that drive bidirectional astrophysical jets
flowing normal to and away from the disk [3,4]. The poloidal electric current
circuit is completed in the disk by a radially inward current that removes angular
momentum from the accreting mass in the disk via a -rJrBz counter-torque. The
complete poloidal electric circuit removes disk angular momentum and transports
it electrically to infinity in the disk plane in a manner analogous to how wires
connecting an electric generator to a distant electric motor transport angular
momentum from the generator to the motor. The disk region is an electric power
source (E⋅J<0) while the jet region is an electric power sink (E⋅J>0).
[1] P. M. Bellan, Monthly Notices Royal Astron. Soc., in press
[2] P. M. Bellan, Physics of Plasmas 14, 122901 (2007).
[3] D. Kumar and P. M. Bellan, Physical Review Letters 103, 105003 (2009)
[4] X. Zhai, H. Li, P. M. Bellan, and S. Li, ApJ 791, 40 (2014).
-Supported by USDOE and NSF.