output
20162023
most cited3D Hydrodynamic Simulations of Carbon Burning in Massive Stars

88 citations

8 papers

cs.LG2023★ 18 cited

Support Vector Machine Guided Reproducing Kernel Particle Method for Image-Based Modeling of Microstructures

Yanran Wang, Jonghyuk Baek, Yichun Tang +3

This work presents an approach for automating the discretization and approximation procedures in constructing digital representations of composites from Micro-CT images featuring i…

astro-ph.SR2019★ 51 cited

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…

astro-ph.SR2018★ 25 cited

3D Simulations and MLT: I. Renzini's Critique

W. David Arnett, Casey Meakin, Raphael Hirschi +5

Renzini (1987) wrote an influential critique of mixing-length theory (MLT) as used in stellar evolution codes, and concluded that three-dimensional (3D) fluid dynamical simulations…

astro-ph.SR2018★ 32 cited

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$_{…

astro-ph.SR2018

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…

cond-mat.mtrl-sci2018★ 10 cited

Quasi-static and Dynamic Behavior of Additively Manufactured Metallic Lattice Cylinders

Hossein Sadeghi, Dhruv Bhate, Joseph Abraham +1

Lattice structures have tailorable mechanical properties which allows them to exhibit superior mechanical properties (per unit weight) beyond what is achievable through natural mat…

astro-ph.SR2017★ 1 cited

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…

astro-ph.SR2016★ 88 cited

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…