Home News About Us Contact Contributors Disclaimer Privacy Policy Help FAQ

Quick Search
My eDoc
Session History
Support Wiki
Direct access to
document ID:

          Institute: MPI für Astronomie     Collection: Publikationen_mpia     Display Documents

ID: 308787.0, MPI für Astronomie / Publikationen_mpia
A comparative study of disc-planet interaction
Authors:de Val-Borro, M.; Edgar, R. G.; Artymowicz, P.; Ciecielag, P.; Cresswell, P.; D'Angelo, G.; Delgado-Donate, E. J.; Dirksen, G.; Fromang, S.; Gawryszczak, A.; Klahr, H.; Kley, W.; Lyra, W.; Masset, F.; Mellema, G.; Nelson, R. P.; Paardekooper, S. J.; Peplinski, A.; Pierens, A.; Plewa, T.; Rice, K.; Schäfer, C.; Speith, R.
Date of Publication (YYYY-MM-DD):2006
Journal Abbrev.:Monthly Notices of the Royal Astronomical Society
Start Page:529
End Page:558
Audience:Not Specified
Abstract / Description:We perform numerical simulations of a disc-planet system using various grid-based and smoothed particle hydrodynamics (SPH) codes. The tests are run for a simple setup where Jupiter and Neptune mass planets on a circular orbit open a gap in a protoplanetary disc during a few hundred orbital periods. We compare the surface density contours, potential vorticity and smoothed radial profiles at several times. The disc mass and gravitational torque time evolution are analysed with high temporal resolution. There is overall consistency between the codes. The density profiles agree within about 5 per cent for the Eulerian simulations. The SPH results predict the correct shape of the gap although have less resolution in the low-density regions and weaker planetary wakes. The disc masses after 200 orbital periods agree within 10 per cent. The spread is larger in the tidal torques acting on the planet which agree within a factor of 2 at the end of the simulation. In the Neptune case, the dispersion in the torques is greater than for Jupiter, possibly owing to the contribution from the not completely cleared region close to the planet.
Free Keywords:accretion; accretion discs: hydrodynamics: planets and satellites: general
External Publication Status:published
Document Type:Article
Communicated by:N. N.
Affiliations:MPI für Astronomie
The scope and number of records on eDoc is subject to the collection policies defined by each institute - see "info" button in the collection browse view.