Evolving a puncture black hole with fixed mesh refinement

Imbiriba, B.; Baker, John G.; Choi, Dae-Il; Centrella, Joan; Fiske, David R.; Brown, J. David; Meter, James R. van; Olson, K.

doi:10.1103/physrevd.70.124025

Cited by 55 publications

(74 citation statements)

References 24 publications

(45 reference statements)

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“…where u 0 is the value of the function u at the puncture and m is the mass parameter in (20). Figure 10 shows the maximum radiation content of a number of single black-hole initial-data sets, and a comparison with similar cases for Bowen-York puncture black holes.…”

Section: A Single Boosted Ctsp Black Holementioning

confidence: 99%

“…We will focus on the momentum constraint, which takes the form Laguna considered if we choose u = v = 0 (or u = v = 1 in Laguna's notation). The conformal factor and lapse splittings (20) and (21) are then…”

Section: A Single Black Hole With Linear Momentummentioning

confidence: 99%

“…Without the need for complex inner boundary conditions, the puncture approach is potentially easier to implement than excision. CTS-puncture binary black-hole initial data would provide a useful comparison with excision data results, and also allow evolution codes that employ punctures [18,19,20] to take advantage of CTS data.…”

Section: Introductionmentioning

confidence: 99%

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Conformal thin-sandwich puncture initial data for boosted black holes

Hannam¹,

Cook

2005

Phys. Rev. D

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We apply the puncture approach to conformal thin-sandwich black-hole initial data. We solve numerically the conformal thin-sandwich puncture (CTSP) equations for a single black hole with non-zero linear momentum. We show that conformally flat solutions for a boosted black hole have the same maximum gravitational radiation content as the corresponding Bowen-York solution in the conformal transverse-traceless decomposition. We find that the physical properties of these data are independent of the free slicing parameter.

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Section: A Single Boosted Ctsp Black Holementioning

confidence: 99%

Section: A Single Black Hole With Linear Momentummentioning

confidence: 99%

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Conformal thin-sandwich puncture initial data for boosted black holes

Hannam¹,

Cook

2005

Phys. Rev. D

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“…The equal-mass runs were carried out with our Hahndol evolution code [32] using the Paramesh meshrefinement infrastructure [33]. The new X4 00 data, however, uses Hahndol paired with the Einstein Toolkit [34] release of the Cactus Computational Toolkit [35] and the Carpet mesh-refinement driver [36].…”

Section: Simulationsmentioning

confidence: 99%

Mergers of black-hole binaries with aligned spins: Waveform characteristics

et al. 2011

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We conduct a descriptive analysis of the multipolar structure of gravitational-radiation waveforms from equal-mass aligned-spin mergers, following an approach first presented in the complementary context of nonspinning black holes of varying mass ratio [1]. We find that, as with the nonspinning mergers, the dominant waveform mode phases evolve together in lock-step through inspiral and merger, supporting the previous waveform description in terms of an adiabatically rigid rotator driving gravitational-wave emission -an implicit rotating source (IRS). We further apply the latetime merger-ringdown model for the rotational frequency introduced in [1], along with an improved amplitude model appropriate for the dominant (2, ±2) modes. This provides a quantitative description of the merger-ringdown waveforms, and suggests that the major features of these waveforms can be described with reference only to the intrinsic parameters associated with the state of the final black hole formed in the merger. We provide an explicit model for the merger-ringdown radiation, and demonstrate that this model agrees to fitting factors better than 95% with the original numerical waveforms for system masses above ∼ 150M⊙. This model may be directly applicable to gravitational-wave detection of intermediate-mass black hole mergers.

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“…Refs. [9,[11][12][13][14][15][16][17][18][19]). This technology allows groups to push their computational boundaries to very large coordinate distances, reducing the effects of incoming radiation and constraint violating modes introduced by applying boundary conditions at a finite distance.…”

Section: Introductionmentioning

confidence: 99%

Excising das All: Evolving Maxwell waves beyond scri

2006

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We study the numerical propagation of waves through future null infinity in a conformally compactified spacetime. We introduce an artificial cosmological constant, which allows us some control over the causal structure near null infinity. We exploit this freedom to ensure that all light cones are tilted outward in a region near null infinity, which allows us to impose excision-style boundary conditions in our finitedifference code. In this preliminary study we consider electromagnetic waves propagating in a static, conformally compactified spacetime.

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Evolving a puncture black hole with fixed mesh refinement

Cited by 55 publications

References 24 publications

Conformal thin-sandwich puncture initial data for boosted black holes

Conformal thin-sandwich puncture initial data for boosted black holes

Mergers of black-hole binaries with aligned spins: Waveform characteristics

Excising das All: Evolving Maxwell waves beyond scri

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