[Users] Simulation of GW150914 binary black hole merger
Barry Wardell
barry.wardell at gmail.com
Fri Sep 30 10:08:51 CDT 2016
Dear Einstein Toolkit users,
We have prepared a new example for the Einstein Toolkit gallery
consisting of a simulation of the spacetime of the gravitational wave
event GW150914 detected by LIGO in September 2015. The example can be
found at
https://einsteintoolkit.org/about/gallery/gw150914
The gallery page consists of a short description, some details of the
physics parameters and computational requirements, as well as the
parameter file and thornlist. We provide a tutorial for obtaining and
compiling the code and running the simulation, which should work on
any of the machines supported by SimFactory (http://simfactory.org).
We also provide a tutorial for visualising the spacetime using the
VisIt visualisation software. Also available is a ~600 MB archive
containing a subset of the simulation output, including waveforms and
horizon quantities, as well as two time slices of 3D data for
visualisation. Lastly, we provide a set of Mathematica notebooks
demonstrating how the simulation data can be processed an analysed
using the SimulationTools (http://simulationtools.org) software package.
The simulation utilises entirely open and public codes including the
Einstein Toolkit and the Llama multiblock infrastructure
(http://llamacode.org).
We ask that if you make use of the parameter file or the example data,
then please cite the GW150914 Einstein Toolkit example and data [1],
the Einstein Toolkit [2], the Llama multi-block infrastructure [3],
the Carpet mesh-refinement driver [4], the apparent horizon finder
AHFinderDirect [5], the TwoPunctures initial data code [6],
QuasiLocalMeasures [7], Cactus [8], and the McLachlan spacetime
evolution code [9].
Please let us know if you have any problems; we will be happy to help!
Barry Wardell, Ian Hinder and Eloisa Bentivegna
--
[1] Barry Wardell, Ian Hinder and Eloisa Bentivegna. Simulation of
GW150914 binary black hole merger using the Einstein Toolkit
(doi:10.5281/zenodo.155394)
[2] Frank Löffler, Joshua Faber, Eloisa Bentivegna, Tanja Bode, Peter
Diener, Roland Haas, Ian Hinder, Bruno C. Mundim, Christian D. Ott,
Erik Schnetter, Gabrielle Allen, Manuela Campanelli, and Pablo
Laguna. The Einstein Toolkit: A Community Computational Infrastructure
for Relativistic Astrophysics. Classical and Quantum Gravity,
29(11):115001, 2012. (doi:10.1088/0264-9381/29/11/115001)
[3] Denis Pollney, Christian Reisswig, Erik Schnetter, Nils Dorband, Peter
Diener. High accuracy binary black hole simulations with an extended
wave zone. Phys.Rev. D83 (2011)
044045. (doi:10.1103/PhysRevD.83.044045)
[4] Erik Schnetter, Scott H. Hawley, and Ian Hawke. Evolutions in 3-D
numerical relativity using fixed mesh refinement. Class. Quantum
Grav., 21:1465–1488, 2004. (doi:10.1088/0264-9381/21/6/014)
[5] Jonathan Thornburg. A Fast Apparent-Horizon Finder for 3-Dimensional
Cartesian Grids in Numerical Relativity. Class. Quantum Grav.,
21:743–766, 2004. (doi:10.1088/0264-9381/21/2/026)
[6] Marcus Ansorg, Bernd Brügmann, and Wolfgang Tichy. A single-domain
spectral method for black hole puncture data. Phys. Rev. D, 70:064011,
2004. (doi:10.1103/PhysRevD.70.064011)
[7] Olaf Dreyer, Badri Krishnan, Deirdre Shoemaker, and Erik
Schnetter. Introduction to isolated horizons in numerical
relativity. Phys. Rev. D, 67:024018,
2003. (doi:10.1103/PhysRevD.67.024018)
[8] Tom Goodale, Gabrielle Allen, Gerd Lanfermann, Joan Massó, Thomas
Radke, Edward Seidel, and John Shalf. The Cactus framework and
toolkit: Design and applications. In Vector and Parallel Processing –
VECPAR'2002, 5th International Conference, Lecture Notes in Computer
Science, Berlin, 2003. Springer.
[9] J. David Brown, Peter Diener, Olivier Sarbach, Erik Schnetter, and
Manuel Tiglio. Turduckening black holes: an analytical and
computational study. Phys. Rev. D, 79:044023,
2009. (doi:10.1103/PhysRevD.79.044023)
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