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--Robert Fisher 09:47, 10 June 2010 (UTC)

Supernovae/White Dwarf Research

FLASHXnet on Expanse

[A] On the login node:

1. Run these commands: module reset conda activate py2

here py2 is a python2 environment which one needs to set up first for the setup.py to work. We need to re-write the setup.py in python3 in near future.

2. After that, setup the model by:

./setup Hybrid_WDs_scatter -objdir=D6_test_scatter -3d -auto +cube32 -maxblocks=30 +uhd +newMpole +hdf5typeIO withParticles=False xnet=True xnetGPU=True xnetData=Data_SN55 -opt
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Then enter an interactive job on a GPU node by running the following command:

srun --partition=gpu-debug --pty --account=TG-AST100038 --ntasks-per-node=40 --nodes=1 --mem=356G --gpus=1 -t 0:30:00 --wait=0 --export=ALL /bin/bash


This will request an interactive session on 1 node with 40 cores, 1 GPU, 356GB of memory for 30 minutes.

[B] On the GPU node (after srun):

1. Load the following modules:

conda activate py2
module reset
module load subversion
module load intel
module load openmpi
module load hdf5/1.8.21
module load cuda10.2/toolkit

2. Enter the build directory and then perform:

make -j4

FLASH - TORCH - SUPERNU - SNID Pipeline
Turbulently driven DDT in thermonuclear flames 
Alpha-disk model for long-time evolution of binary white dwarfs post-merger
Theory
Progenitor study of Supernova remnant 3C397
Nucleosynthetic Yields and Synthetic Spectra of Type Ia Supernovae using Torch and SuperNu
Crash course in fluid dynamics
Fluid description
Tensors and some important identities
Theorems in tensor calculus
Conservation of mass, Reynolds mass transport theorem
Lagrangian and Eulerian prescriptions
Conservation of momentum, Navier-Stokes equation
Fluid instabilities
High Re flows, turbulence
Other Transients
White Dwarf TDEs
SLSNe
Binary Black Holes
Numerical Methods Research
PPM on GPUs
Visualization and System Administration
Touch Interface Visualizations
 Proposal Development
NSF STCI
NSF IGERT
UMass Dartmouth Administration
 Teaching
Teaching Resources