activity
20112020
most citedA Jacobian-free Newton-Krylov method for time-implicit multidimensional hydrodynamics

41 citations · 224 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.SR2020★ 22 cited

Comparison of two- and three-dimensional compressible convection in a pre-main sequence star

J. Pratt, I. Baraffe, T. Goffrey +4

Extending our recent studies of two-dimensional stellar convection to 3D, we compare three-dimensional hydrodynamic simulations to identically set-up two-dimensional simulations, f…

astro-ph.SR2019★ 9 cited

A well-balanced scheme for the simulation tool-kit A-MaZe: implementation, tests, and first applications to stellar structure

M. V. Popov, R. Walder, D. Folini +6

Characterizing stellar convection in multiple dimensions is a topic at the forefront of stellar astrophysics. Numerical simulations are an essential tool for this task. We present…

astro-ph.IM2016★ 31 cited

Benchmarking the Multi-dimensional Stellar Implicit Code MUSIC

T. Goffrey, J. Pratt, M. Viallet +6

We present the results of a numerical benchmark study for the MUlti-dimensional Stellar Implicit Code (MUSIC) based on widely applicable two- and three-dimensional compressible hyd…

astro-ph.SR2016★ 27 cited

Spherical-shell boundaries for two-dimensional compressible convection in a star

J. Pratt, I. Baraffe, T. Goffrey +6

Context: We study the impact of two-dimensional spherical shells on compressible convection. Realistic profiles for density and temperature from a one-dimensional stellar evolution…

astro-ph.SR2016★ 23 cited

Multi-dimensional structure of accreting young stars

C. Geroux, I. Baraffe, M. Viallet +6

This work is the first attempt to describe the multi-dimensional structure of accreting young stars based on fully compressible time implicit multi-dimensional hydrodynamics simula…

astro-ph.IM2015★ 41 cited

A Jacobian-free Newton-Krylov method for time-implicit multidimensional hydrodynamics

Maxime Viallet, Tom Goffrey, Isabelle Baraffe +5

This work is a continuation of our efforts to develop an efficient implicit solver for multidimensional hydrodynamics for the purpose of studying important physical processes in st…

astro-ph.SR2014★ 12 cited

Radial Stellar Pulsation and Three-Dimensional Convection. IV. Full Amplitude Three-Dimensional Solutions

Christopher M. Geroux, Robert G. Deupree

Three dimensional hydrodynamic simulations of full amplitude RR Lyrae stars have been computed for several models across the instability strip. The three dimensional nature of the…

astro-ph.SR2014★ 9 cited

Radial Stellar Pulsation and Three-Dimensional Convection. III. Comparison of Two-Dimensional and Three-Dimensional Convection Effects on Radial Pulsation

Christopher M. Geroux, Robert G. Deupree

We have developed a multidimensional radiation hydrodynamics code to simulate the interaction of radial stellar pulsation and convection for full amplitude pulsating models. Convec…

astro-ph.SR2013★ 23 cited

Radial Stellar Pulsation and Three-Dimensional Convection. II. Two-Dimensional Convection In Full Amplitude Radial Pulsation

Chris M. Geroux, Robert G. Deupree

We have developed a three-dimensional radiation hydrodynamics code to simulate the interaction of convection and radial pulsation in classical variable stars. One key goal is the a…

astro-ph.SR2011★ 27 cited

Radial Stellar Pulsation and 3D Convection. I. Numerical Methods and Adiabatic Test Cases

Chris M. Geroux, Robert G. Deupree

We are developing a 3D radiation hydrodynamics code to simulate the interaction of convection and pulsation in classical variable stars. One key goal is the ability to carry these…