Astronomy and Astrophysics – Astrophysics – General Relativity and Quantum Cosmology
Scientific paper
2010-04-08
Phys.Rev.D82:024005,2010
Astronomy and Astrophysics
Astrophysics
General Relativity and Quantum Cosmology
Published in PRD
Scientific paper
10.1103/PhysRevD.82.024005
We present numerical evolutions of three equal-mass black holes using the moving puncture approach. We calculate puncture initial data for three black holes solving the constraint equations by means of a high-order multigrid elliptic solver. Using these initial data, we show the results for three black hole evolutions with sixth-order waveform convergence. We compare results obtained with the BAM and AMSS-NCKU codes with previous results. The approximate analytic solution to the Hamiltonian constraint used in previous simulations of three black holes leads to different dynamics and waveforms. We present some numerical experiments showing the evolution of four black holes and the resulting gravitational waveform.
Bruegmann Bernd
Cao Zhoujian
Galaviz Pablo
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