Extending superposed harmonic initial data to higher spin

Abstract

Numerical simulations of binary black holes are accompanied by an initial spurious burst of gravitational radiation (called `junk radiation') caused by a failure of the initial data to describe a snapshot of an inspiral that started at an infinite time in the past. A previous study showed that the superposed harmonic (SH) initial data gives rise to significantly smaller junk radiation. However, it is difficult to construct SH initial data for black holes with dimensionless spin $\chi \gtrsim 0.7$. We here provide a class of spatial coordinate transformations that extend SH to higher spin. The new spatial coordinate system, which we refer to as superposed modified harmonic (SMH), is characterized by a continuous parameter -- Kerr-Schild and harmonic spatial coordinates are only two special cases of this new gauge. We compare SMH with the superposed Kerr-Schild (SKS) initial data by evolving several binary black hole systems with $\chi =0.8$ and $0.9$. We find that the new initial data still leads to less junk radiation and only small changes of black hole parameters (e.g. mass and spin). We also find that the volume-weighted constraint violations for the new initial data converge with resolution during the junk stage $(t\lesssim 700M)$, which means there are fewer high-frequency components in waveforms at outer regions.

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Cited by in corpus (4)

• Mini-disk accretion onto spinning black hole binaries: quasi-periodicities and outflows
• The SXS Collaboration's third catalog of binary black hole simulations
• Efficient simulations of high-spin black holes with a new gauge
• Discontinuous Galerkin scheme for elliptic equations on extremely stretched grids