,
pages 1-150
Physical Processes in Protoplanetary Disks
Publication type: Book Chapter
Publication date: 2019-02-02
SJR: —
CiteScore: —
Impact factor: —
ISSN: 18617980, 18618227
Abstract
This review, based on lectures given at the 45th Saas-Fee Advanced Course “From Protoplanetary Disks to Planet Formation”, introduces physical processes in protoplanetary disks relevant to accretion and the initial stages of planet formation. After a brief overview of the observational context, I introduce the elementary theory of disk structure and evolution, review the gas-phase physics of angular momentum transport through turbulence and disk winds, and discuss possible origins for the episodic accretion observed in Young Stellar Objects. Turning to solids, I review the evolution of single particles under aerodynamic forces, and describe the conditions necessary for the development of collective gas-particle instabilities. Observations show that disks can exhibit pronounced large-scale structure, and I discuss the types of structures that may form from gas and particle interactions at ice lines, vortices and zonal flows, prior to the formation of large planetary bodies. I conclude with disk dispersal.
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Metrics
29
Total citations:
29
Citations from 2024:
5
(17.24%)
Cite this
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RIS
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TY - GENERIC
DO - 10.1007/978-3-662-58687-7_1
UR - https://doi.org/10.1007/978-3-662-58687-7_1
TI - Physical Processes in Protoplanetary Disks
T2 - Saas-Fee Advanced Courses
AU - Armitage, Philip J
PY - 2019
DA - 2019/02/02
PB - Springer Nature
SP - 1-150
SN - 1861-7980
SN - 1861-8227
ER -
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@incollection{2019_Armitage,
author = {Philip J Armitage},
title = {Physical Processes in Protoplanetary Disks},
publisher = {Springer Nature},
year = {2019},
pages = {1--150},
month = {feb}
}