Density Evolution of Dust Aggregates Growing in Protoplanetary Disks

Details Density Evolution of Dust Aggregates Growing in Protoplanetary Disks Density Evolution of Dust Aggregates Growing in Protoplanetary Disks

Mar 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008lpi....39.1473s&link_type=abstract

39th Lunar and Planetary Science Conference, (Lunar and Planetary Science XXXIX), held March 10-14, 2008 in League City, Texas.

Computer Science

Scientific paper

In protoplanetary disks, dust aggregates grow through mutual collisions.
Such collision results in not only coalescence but also compression. We
perform the N-body simulation of aggregate collisions and examine the
density change.

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