Dissipationless Disk Accretion

Details Dissipationless Disk Accretion Dissipationless Disk Accretion

2007-10-16

arxiv.org/abs/0710.2986v1

Astron.Rep.49:57,2005

Astronomy and Astrophysics

Astrophysics

17 pages, 6 figures, published in Astronomy Reports, Vol.49, No.1, 2005, p.57 (submitted September 13, 2003). Unfortunately, w

Scientific paper

10.1134/1.1850206

We consider disk accretion resulting purely from the loss of angular momentum due to the outflow of plasma from a magnetized disk. In this limiting case, the dissipation due to the viscosity and finite electrical conductivity of the plasma can be neglected. We have obtained self-consistent, self-similar solutions for dissipationless disk accretion. Such accretion may result in the formation of objects whose bolometric luminosities are lower than the flux of kinetic energy in the ejected material.

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