Particle Concentration in an Evolving Disk: Implications for Early Accretion and Planetesimal Formation

Details Particle Concentration in an Evolving Disk: Implications for Early Accretion and Planetesimal Formation Particle Concentration in an Evolving Disk: Implications for Early Accretion and Planetesimal Formation

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010lpi....41.1847h&link_type=abstract

41st Lunar and Planetary Science Conference, held March 1-5, 2010 in The Woodlands, Texas. LPI Contribution No. 1533, p.1847

Physics

Scientific paper

We model the radial drift and turbulent diffusion of particles in a
one-dimensional viscously evolving and accreting gas disk to examine the
potential for possibilities for dust-to-gas concentration above cosmic.

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