3 citations · 5 across the 3 of their papers we have counts for
6 papers · 1 filter
Experimental evidence for granular shear-flow instability in the Epstein regime
Holly L. Capelo, Jean-David Bodénan, Martin Jutzi +7
Stability analysis of two-fluid protoplanetary disc models has enriched our understanding of how solids can grow into larger bodies called planetesimals. Dust particles entrained i…
Meridional Circulation of Dust and Gas in the Circumstellar Disk: Delivery of Solids onto the Circumplanetary Region
J. Szulágyi, F. Binkert, C. Surville
We carried out 3D dust+gas radiative hydrodynamic simulations of forming planets. We investigated a parameter grid of Neptune-, Saturn-, Jupiter-, and 5 Jupiter-mass planets at 5.2…
Concurrent effects of gas drag and planet migration on pebble accretion
Clément Surville, Lucio Mayer, Yann Alibert
We study the effect of a migrating planet ( Earth mass) on the dynamics of pebbles in a radiative disk using 2D two-fluid simulations carried out with the RoSSBi code. T…
Can chondrules be produced by the interaction of Jupiter with the protosolar disk?
Jean-David Bodénan, Clément Surville, Judit Szulágyi +2
Chondrules are crystallised droplets of silicates formed by rapid heating to high temperatures (> 1800 K) of solid precursors followed by hours or days of cooling. Dating of chondr…
A sub-grid model for the growth of dust particles in hydrodynamical simulations of protoplanetary disks
Tomas Tamfal, Joanna Drazkowska, Lucio Mayer +1
We present the first 2D hydrodynamical finite volume simulations in which dust is fully coupled with the gas, including its back-reaction onto it, and at the same time the dust siz…
Dust-vortex instability in the regime of well-coupled grains
Clément Surville, Lucio Mayer
We present a novel study of dust-vortex evolution in global two-fluid disk simulations to find out if evolution toward high dust-to-gas ratios can occur in a regime of well-coupled…