Dissipationless Disk Accretion
arXiv:0710.2986 · doi:10.1134/1.1850206
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.
17 pages, 6 figures, published in Astronomy Reports, Vol.49, No.1, 2005, p.57 (submitted September 13, 2003). Unfortunately, we did not upload the paper to astro-ph before, but since the topic is now of interest we feel that the paper would benefit the community
References in corpus (5)
- Unified Schemes for Radio-Loud Active Galactic Nuclei
- Discovery of Spatial and Spectral Structure in the X-Ray Emission from the Crab Nebula
- On the origin of the torus and jet-like structures in the centre of Crab Nebula
- A class of exact MHD models for astrophysical jets
- Magnetized accretion-ejection structures IV. Magnetically-driven jets from resistive, viscous, Keplerian discs
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