Gas Giant Protoplanet Formation: Disk Instability Models with Detailed Thermodynamics and Varied Artificial Viscosity

Details Gas Giant Protoplanet Formation: Disk Instability Models with Detailed Thermodynamics and Varied Artificial Viscosity Gas Giant Protoplanet Formation: Disk Instability Models with Detailed Thermodynamics and Varied Artificial Viscosity

Mar 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003lpi....34.1075b&link_type=abstract

34th Annual Lunar and Planetary Science Conference, March 17-21, 2003, League City, Texas, abstract no.1075

Physics

5

Scientific paper

We show that when artificial viscosity is included in 3D disk
instability models with radiative and convective cooling, the tendency
to form clumps is reduced somewhat, but not eliminated, unless the
artificial viscosity is increased by a factor of ten over the nominal
value.

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