Coagulation in dusty plasmas

Details Coagulation in dusty plasmas Coagulation in dusty plasmas

Mar 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997lpi....28..895m&link_type=abstract

Conference Paper, 28th Annual Lunar and Planetary Science Conference, p. 895.

Other

Space Plasmas, Cosmic Dust, Protostars, Protoplanets, Comet Tails, Coagulation, Planetary Rings, Mathematical Models, Charged Particles

Scientific paper

Dusty plasmas are a ubiquitous component of space, found in protostellar clouds, protoplanetary disks, cometary tails, and in the planetary rings. As a result, the physics underlying the manner in which microscopic dust grains interact with one another and their plasma/gas environment is a field of research having broad implications for the development of astrophysical systems. This paper examines a numerical model for coagulation based on the Box Tree code. Preliminary results are given showing coagulation of dust grains with no self-interactions, grains interacting through self-gravity only, and charged grains interacting gravitationally and electrostatically.

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