Pushed to zach_etienne/nrpy
7ef2441 plotting constant-r surfaces as frames that can later be stitched into a movie
NRPy+: Python-based Code Generation for Numerical Relativity... and Beyond! Core Developers: Zachariah B. Etienne Ian Ruchlin ================================================= This repository contains NRPy+ as well as the following codes that depend on NRPy+: 1) SENR: a Simple, Efficient Numerical Relativity code SENR/NRPy+ Homepage: http://math.wvu.edu/~zetienne/SENR SENR/NRPy+ Paper: https://arxiv.org/abs/1712.07658 2) scalarwave: a tiny, pedagogic code for solving the scalar wave equation in many coordinate systems 3) FishboneMoncrief: a black hole accretion disk initial data module ("thorn") for the Einstein Toolkit ("Cactus"). Uses a Kerr-Schild background metric for the black hole. ================================================= Quick Start for new users of NRPy+: 0) Download NRPy+ using git (https://git-scm.com/downloads): git clone https://bitbucket.org/zach_etienne/nrpy.git 1) Go to the tutorial/ subdirectory, generate the scalar wave tutorial PDF file with `make` (you will need LaTeX installed), and then follow the tutorial. This will familiarize you with NRPy+ in the context of solving the scalar wave equation. Quick Start for SENR ("a Simple, Efficient Numerical Relativity code"): 0) Download SENR/NRPy+ using git (https://git-scm.com/downloads): git clone https://bitbucket.org/zach_etienne/senr.git 1) Follow directions in SENR_NRPy_quick_intro.txt to generate needed C code for SENR. 2) Go to the SENR/ subdirectory. This is where the NRPy+/SENR (BSSN) code is located. 3) If you have the Intel C Compiler (icc) installed, (RECOMMENDED), to compile the SENR (BSSN) code, type: make -j If you have only the GCC C compiler installed, (NOT RECOMMENDED, much slower executables), to compile the BSSN code, type: make -f Makefile-gcc -j 4) Run SENR (BSSN) via the command ./SENR 128 32 2 1000.0 0.15 Tip: Install 'taskset' to use processor core affinity for better performance. If you have N cores, type taskset -c 0,1,..,(N/2)-1 ./SENR 128 32 2 1000.0 0.15 For example, if you have 8 cores, type: taskset -c 0,1,2,3 ./SENR 128 32 2 1000.0 0.15 You will find output files in the output/ directory. To see what is stored in these files, check out diagnostics/Data_File_Output.c Repository Directory Contents: - [root directory, probably "nrpy"]/ > NRPy+, the Python-based code generator for SENR, scalar wave, and Fishbone-Moncrief (Einstein Toolkit initial data module) exists in the NRPy+/ subdirectory. * See SENR_NRPy_quick_intro.txt for a brief introduction - SENR/ (a.k.a. SENR/NRPy+; the numerical relativity code) > Currently contains: * Full BSSN implementation in spherical polar, sinh-radial (r -> sinh(r)) spherical polar, Cartesian, cylindrical, sinh-cylindrical, and modified (symmetric) TwoPunctures, including - RK4 timestepping (same stability features as PIRK2, except without the additional algorithmic complications) - Outer boundary conditions: quadratic extrapolation (default), linear extrapolation, Sommerfeld - Diagnostics: . Hamiltonian and momentum constraints . ADM Mass, ADM angular momentum, ADM linear momentum . 1D, 2D, and (disabled by default) 3D output of grid and diagnostic functions . SinhSpherical-to-Cartesian Einstein Toolkit diagnostic compatibility layer (enable with -DENABLE_SPHERICAL_TO_CARTESIAN_ETK_LAYER compiler flag in Makefile, currently only for SinhSpherical coordinates). * Initial data modules in arbitrary coordinates for - Single black hole in UIUC coordinates (https://arxiv.org/abs/1001.4077) - Two nonspinning black holes initially at rest (Brill-Lindquist initial data) - Static trumpet solution (https://arxiv.org/abs/1403.5484) - Boosted Schwarzschild black hole (https://arxiv.org/abs/1410.8607) - Minkowski spacetime (add initial random perturbation to this initial data to perform Apples-to-Apples robust stability test: https://arxiv.org/abs/0709.3559) - utilities/DynamicalCoordinates/ > Various utilities for visualizing & testing dynamical coords: * TP_mods/ + A code to generate both original and modified TwoPunctures coordinate distributions. * WaveToy1D/ + A 1D scalar wave evolved with a second- order PIRK integration scheme, on a logarithmic coordinate grid. - utilities/EinsteinToolkit/ET__SENR_bridge__ET_thorn/ > This Einstein Toolkit thorn enables the large suite of diagnostics within the Einstein Toolkit to be used directly with SENR/NRPy+ output files. - utilities/EinsteinToolkit/compute_spin > Computes the dimensionless black hole spin parameter based on (apparent) horizon proper polar to circumferential radii, using Eq 5.2 of https://arxiv.org/pdf/gr-qc/0411149.pdf > Can process output from AHFinderDirect - SENR/old-BSSN-Cartesian-firsttry-arborder-agreeswithKranc/ > Original (early, experimental) implementation of the BSSN equations (right-hand-sides) in Cartesian coordinates. Implements arbitrary-order finite-difference stencils via adjustment of single parameter ORDER. Results demonstrated to agree to roundoff error with Kranc output at 2nd, 4th, 6th, and 8th orders. - SENR/version_of_SENR_roundoff_agreement_with_Baumgarte_code/ > Unmaintained version of SENR that implements PIRK2 timestepping, in spherical polar coordinates. Used for validation, as this version has been shown to agree with Baumgarte et al's code to roundoff error.