Volume 82, Number 1, April 2008
|Number of page(s)||6|
|Section||Geophysics, Astronomy and Astrophysics|
|Published online||12 March 2008|
Thermo-rotational instability in plasma disks around compact objects
Massachusetts Institute of Technology, Cambridge, MA, USA
Corresponding author: firstname.lastname@example.org
Accepted: 12 February 2008
Differentially rotating plasma disks, around compact objects, that are imbedded in a “seed” magnetic field are shown to develop vertically localized ballooning modes that are driven by the combined radial gradient of the rotation frequency and vertical gradients of the plasma density and temperature. When the electron mean free path is shorter than the disk height and the relevant thermal conductivity can be neglected, the vertical particle flows produced by these modes have the effect to drive the density and temperature profiles toward the “adiabatic condition” where = 2/3 . Here T is the plasma temperature and n the particle density. The faster growth rates correspond to steeper temperature profiles ( > 2/3) such as those produced by an internal (e.g., viscous) heating process. In the end, ballooning modes excited for various values of can lead to the evolution of the disk into a different current carrying configuration such as a sequence of plasma rings.
PACS: 98.62.Mw – Infall, accretion, and accretion disks / 52.35.Py – Macroinstabilities (hydromagnetic, e.g., kink, fire-hose, mirror, ballooning, tearing, trapped-particle, flute, Rayleigh-Taylor, etc.) / 47.65.Md – Plasma dynamos
© EPLA, 2008
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