activity
20162022
most citedLithium depletion in solar-like stars: effect of overshooting based on realistic multi-dimensional simulations

64 citations · 195 across the 7 of their papers we have counts for

collaborators

12 papers

astro-ph.SR202219 cited

Two-dimensional simulations of solar-like models with artificially enhanced luminosity. II. Impact on internal gravity waves

A. Le Saux, T. Guillet, I. Baraffe +7

Artificially increasing the luminosity and the thermal diffusivity of a model is a common tactic adopted in hydrodynamical simulations of stellar convection. In this work, we analy…

astro-ph.SR202124 cited

Two-dimensional simulations of solar-like models with artificially enhanced luminosity -- I. Impact on convective penetration

I. Baraffe, J. Pratt, D. G. Vlaykov +4

We perform 2D, fully compressible, time-implicit simulations of convection in a solar-like model with the MUSIC code. Our main motivation is to explore the impact of a common tacti…

astro-ph.SR20211 cited

Suppression of lithium depletion in young low-mass stars from fast rotation

Thomas Constantino, Isabelle Baraffe, Thomas Goffrey +4

We compute rotating 1D stellar evolution models that include a modified temperature gradient in convection zones and criterion for convective instability inspired by rotating 3D hy…

physics.plasm-ph2020

Inflationary stimulated Raman scattering in shock-ignition plasmas

SJ Spencer, Alexander Seaton, Tom Goffrey +1

In the shock-ignition inertial confinement fusion scheme, high-intensity lasers propagate through an inhomogeneous coronal plasma, driving a shock designed to cause fuel ignition.…

astro-ph.SR202018 cited

Unveiling the magnetic nature of chromospheric vortices

Mariarita Murabito, Juie Shetye, Marco Stangalini +5

Vortex structures in the Sun's chromosphere are believed to channel energy between different layers of the solar atmosphere. We investigate the nature and dynamics of two small-sca…

astro-ph.SR2020

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…