activity
20022026
most citedSPLASH: An interactive visualisation tool for Smoothed Particle Hydrodynamics simulations

757 citations · 12.6k across the 181 of their papers we have counts for

collaborators
Showing 2018Show all

16 papers · 1 filter

physics.comp-ph2018★ 14 cited

Stable anisotropic heat conduction in smoothed particle hydrodynamics

Sergei Biriukov, Daniel J. Price

We investigate how to simulate anisotropic heat conduction in a stable manner in Smoothed Particle Hydrodynamics. We show that the requirement for stability is that entropy must in…

astro-ph.EP2018★ 142 cited

Flybys in protoplanetary discs: I. Gas and dust dynamics

Nicolás Cuello, Giovanni Dipierro, Daniel Mentiplay +7

We present 3D smoothed particle hydrodynamics simulations of protoplanetary discs undergoing a flyby by a stellar perturber on a parabolic orbit lying in a plane inclined relative…

astro-ph.EP2018★ 22 cited

Super-Earths in the TW Hya disc

Daniel Mentiplay, Daniel J. Price, Christophe Pinte

We test the hypothesis that the sub-millimetre thermal emission and scattered light gaps seen in recent observations of TW Hya are caused by planet-disc interactions. We perform gl…

astro-ph.EP2018

F.S.I.: Flyby Scene Investigation

Nicolás Cuello, Giovanni Dipierro, Daniel Mentiplay +7

We present a methodology to interpret observations of protoplanetary discs where a flyby, also called a tidal encounter, is suspected. In case of a flyby, protoplanetary discs can…

astro-ph.SR2018★ 82 cited

Extending Common Envelope Simulations from Roche Lobe Overflow to the Nebular Phase

Thomas A. Reichardt, Orsola De Marco, Roberto Iaconi +2

We have simulated a common envelope interaction of a 0.88-M, 90-R, red giant branch star and a 0.6-M, compact companion with the smoothed particle hyd…

astro-ph.SR2018★ 34 cited

On the origin of magnetic fields in stars

James Wurster, Matthew R. Bate, Daniel J. Price

Are the kG-strength magnetic fields observed in young stars a fossil field left over from their formation or are they generated by a dynamo? We use radiation non-ideal magnetohydro…