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19962025
most citedFundamental differences between SPH and grid methods

623 citations · 2.2k across the 49 of their papers we have counts for

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13 papers · 1 filter

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.SR2017★ 64 cited

Lithium depletion in solar-like stars: effect of overshooting based on realistic multi-dimensional simulations

I. Baraffe, J. Pratt, T. Goffrey +5

We study lithium depletion in low-mass and solar-like stars as a function of time, using a new diffusion coefficient describing extra-mixing taking place at the bottom of a convect…

astro-ph.SR2017★ 48 cited

Extreme value statistics for two-dimensional convective penetration in a pre-Main Sequence star

J. Pratt, I. Baraffe, T. Goffrey +5

We examine a penetration layer formed between a central radiative zone and a large convection zone in the deep interior of a young low-mass star. Using the Multidimensional Stellar…

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…