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thundermoose/Anicre
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========== Anicre ========== This is Anicre, a program that computes among other things transition densities needed for JupiterNCSM. ========== License ========== This software is published under GPL v 2, and comes without any warranty. See LICENSE for more details. ========== Usage ========== This is a quick note on how to use Anicre Build mfr: --- make To generate index lists for JupiterNCSM --- 1. Prerequisites: - pAntoine wave function file exists in <egv_dir>/<egv_name>.egv - all run files will be generated in the scratch dir <rundir>/anicr_runs/<egv_name>.jtd - the mfr executable is in the present working directory 2. Set envvars (here assuming bash): export WAVEFUNCTION_PATH=<egv_dir> export SCRATCHDIR=<rundir> export MFR_PATH=$PWD 3. Build greedyorder: g++ --std=c++11 -Wall -W -o greedyorder greedyorder.cc -O3 4. Run: ./compile_for_jupiter.sh <egv_name> ./run_for_jupiter.sh <egv_name> 5. Output in: <rundir>/anicr_runs/<egv_name>.jtd/ ========== Authors ========== * Daniel Sääf Primary developer epost: daniel.saaf@gmail.com * Christian Forssén Contact and maintainer epost: christian.forssen@chalmers.se * Håkan T. Johansson epost: f96hajo@chalmers.se * Tor Djärv epost: djarv@chalmers.se
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