924 citations · 3.5k across the 35 of their papers we have counts for
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Dependence of Convective Boundary Mixing on Boundary Properties and Turbulence Strength
A. Cristini, R. Hirschi, C. Meakin +3
Convective boundary mixing is one of the major uncertainties in stellar evolution. In order to study its dependence on boundary properties and turbulence strength in a controlled w…
Turbulent Mixing and Nuclear Burning in Stellar Interiors
Miroslav Mocák, Casey Meakin, Simon Wattana Campbell +1
The turbulent burning of nuclei is a common phenomenon in the evolution of stars. Here we examine a challenging case: the merging of the neon and oxygen burning shells in a 23 M$_{…
Progenitors of Core-Collapse Supernovae
Raphael Hirschi, David Arnett, Andrea Cristini +3
Massive stars have a strong impact on their surroundings, in particular when they produce a core-collapse supernova at the end of their evolution. In these proceedings, we review t…
The First 3D Simulations of Carbon Burning in a Massive Star
Andrea Cristini, Casey Meakin, Raphael Hirschi +3
We present the first detailed three-dimensional hydrodynamic implicit large eddy simulations of turbulent convection for carbon burning. The simulations start with an initial radia…
3D Hydrodynamic Simulations of Carbon Burning in Massive Stars
Andrea Cristini, Casey Meakin, Raphael Hirschi +3
We present the first detailed three-dimensional (3D) hydrodynamic implicit large eddy simulations of turbulent convection of carbon burning in massive stars. Simulations begin with…
Linking 1D Evolutionary to 3D Hydrodynamical Simulations of Massive Stars
Andréa Cristini, Casey Meakin, Raphael Hirschi +3
Stellar evolution models of massive stars are important for many areas of astrophysics, for example nucleosynthesis yields, supernova progenitor models and understanding physics un…