Dynamical Evolution of Protoplanetary Disks
Abstract
This paper reviews the theory of protostellar debris disks. After a brief introduction to accretion disk physics, I describe coagulation models of planet formation in the outer regions of planetesimal disks. Coagulation models for the Kuiper Belt produce Pluto-sized objects on timescales of 10-40 Myr. These models yield size distributions which agree with observations of Kuiper Belt objects with red magnitudes, R = 20-27. Velocity stirring models for other debris disk systems demonstrate that 500 km or larger objects can stir the velocities of small objects up to the shattering limit needed to begin a collisional cascade.
Cite
@article{arxiv.astro-ph/0010036,
title = {Dynamical Evolution of Protoplanetary Disks},
author = {Scott J. Kenyon},
journal= {arXiv preprint arXiv:astro-ph/0010036},
year = {2007}
}
Comments
24 pages with 6 figures; to appear in the Proceedings of Galactic Structure, Stars, and the Interstellar Medium, a NASA Legacy meeting, edited by M. D. Bicay and C. E. Woodward