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arXiv · 0710.2986

Dissipationless Disk Accretion

Sergey V. Bogovalov·Stanislav R. Kelner
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Abstract

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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Sergey V. Bogovalov, Stanislav R. Kelner. 2007-10-16. Dissipationless Disk Accretion. https://doi.org/10.1134/1.1850206

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