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Welcome to the Fisher Group Wiki!


An artist's rendition of the protoplanetary disk surrounding a young star. An artist's rendition of the single-degenerate model of Type Ia Supernovae, before and after.(ESO)


Wiki Organization

This top-level page structures the Wiki into major topics of current research within the group. Please do not add to this page directly, but instead drill down to the next level to begin editing your area of research. To learn more about editing pages, please see the page About the Fisher Group Wiki.

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

Tutorials / Computer Systems

Reference Materials

Star Formation Research

Astrochemical Evolution of Giant Molecular Clouds

Brown Dwarf Desert

Numerical Analysis of the Jeans Instability

Turbulence in Giant Molecular Clouds

Determing Stellar Multiplicity Criteria at the Molecular Cloud Core Scale from Simulations of Supersonic, Self-Gravitational Isothermal Turbulence

Supernovae/White Dwarf Research

Background Reading

Dark Energy

White Dwarfs

MESA White Dwarf Type Ia Progenitors

Rotating White Dwarf Progenitor Models for Type Ia Supernovae

Turbulent Detonation Conditions for Type Ia Supernovae

Single Degenerate Model for Type Ia Supernovae

Double Degenerate Model for Type Ia Supernovae

Magnetized White Dwarf Mergers

Hydrodynamical run of Hot envelope models

Type Iax Supernovae

Setting Up a Double Degenerate Merger Simulation with Gadget-2

Double Detonation Model for Type Ia Supernovae

Gravitational Waves from Single-Degenerate Channel of Type Ia Supernovae

Semi-Analytic Model of Deflagration Phase of Turbulent Nuclear Burning in Type Ia Supernovae

Effect of Varying Progenitor Central Density in Single-Degenerate Scenario

Radiative Transfer Modeling of Type Ia Supernovae

Debris Disk White Dwarf Systems

Rotating Nuclear-Burning White Dwarfs

Supernova Remnants

Single Degenerate Model for Type Ia Supernovae: GCD

Nucleosynthetic Yields with the FLASH + Torch pipeline

Creating White Dwarf profiles

Supernova Spectra and Light Curves

Supernova Spectra Analysis

Analysis of the Propeller Regime of White Dwarf Merger

Binary Population Synthesis of SNe Ia

D6 Simulation Notes

FLASHXnet on Summit

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

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