Particle rings and astrophysical accretion discs
Creators
- 1. Department of Astronomy, Cornell University, Ithaca, NY 14850 (United States)
Description
Norman Rostoker had a wide range of interests and significant impact on the plasma physics research at Cornell during the time he was a Cornell professor. His interests ranged from the theory of energetic electron and ion beams and strong particle rings to the related topics of astrophysical accretion discs. We outline some of the topics related to rings and discs including the Rossby wave instability which leads to formation of anticyclonic vortices in astrophysical discs. These vorticies are regions of high pressure and act to trap dust particles which in turn may facilitate planetesimals growth in proto-planetary disks and could be important for planet formation. Analytical methods and global 3D magneto-hydrodynamic simulations have led to rapid advances in our understanding of discs in recent years.
Additional details
Identifiers
- DOI
- 10.1063/1.4944026;
Publishing Information
- Journal Title
- AIP Conference Proceedings
- Journal Volume
- 1721
- Journal Issue
- 1
- Journal Page Range
- p. 050004-050004.16
- ISSN
- 0094-243X
- CODEN
- APCPCS
Conference
- Title
- Norman Rostoker memorial symposium
- Dates
- 24-25 Aug 2015
- Place
- Newport Beach, CA (United States)
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 48035485
- Subject category
- S71: CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- ACCRETION DISKS; ASTROPHYSICS; COMPUTERIZED SIMULATION; COSMIC DUST; ELECTRON BEAMS; INSTABILITY; ION BEAMS; MAGNETOHYDRODYNAMICS; PLANETS; PLASMA; PROTOPLANETS; STAR ACCRETION; TAIL ELECTRONS; THREE-DIMENSIONAL CALCULATIONS; VORTICES
- Descriptors DEC
- BEAMS; DUSTS; ELECTRONS; ELEMENTARY PARTICLES; EVOLUTION; FERMIONS; FLUID MECHANICS; HYDRODYNAMICS; LEPTON BEAMS; LEPTONS; MECHANICS; PARTICLE BEAMS; PHYSICS; SIMULATION; STAR EVOLUTION
Optional Information
- Notes
- (c) 2016 AIP Publishing LLC