Toward a dynamical shift condition for unequal mass black hole binary simulations

Adaptive mesh refinement for hyperbolic partial differential equations

Marsha J. Berger and Joseph Oliger · 1984

Earlier work this paper cites.

New Formalism for Numerical Relativity

C. Bona, J. Massó, E. Seidel, and J. Stela · 1995

Earlier work this paper cites.

Evolution of three-dimensional gravitational waves: Harmonic slicing case

M. Shibata and T. Nakamura · 1995

Earlier work this paper cites.

Coordinate conditions in three-dimensional numerical relativity

J. Balakrishna, G. Daues, E. Seidel, W.-M. Suen, M. Tobias, and E. Wang · 1996

Earlier work this paper cites.

On the Numerical integration of Einstein’s field equations

T. W. Baumgarte and S. L. Shapiro · 1998

Earlier work this paper cites.

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Miguel Alcubierre and Bernd Brügmann · 2001

Earlier work this paper cites.

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Miguel Alcubierre, Bernd Brügmann, Denis Pollney, Edward Seidel, and Ryoji Takahashi · 2001

Earlier work this paper cites.

Gauge conditions for long-term numerical black hole evolutions without excision

Miguel Alcubierre, Bernd Brügmann, Peter Diener, Michael Koppitz, Denis Pollney, Edward Seidel, and Ryoji Takahashi · 2003

Earlier work this paper cites.

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Earlier work this paper cites.

On the well posedness of the Baumgarte-Shapiro- Shibata-Nakamura formulation of Einstein’s field equations

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A single-domain spectral method for black hole puncture data

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Numerical simulation of orbiting black holes

Bernd Brügmann, Wolfgang Tichy, and Nina Jansen · 2004

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Accurate black hole evolutions by fourth-order numerical relativity

Y. Zlochower, J. G. Baker, M. Campanelli, and C. O. Lousto · 2005

Cited alongside, same era.

Accurate evolutions of orbiting black-hole binaries without excision

Manuela Campanelli, Carlos O. Lousto, Pedro Marronetti, and Yosef Zlochower · 2006

Cited alongside, same era.

Gravitational wave extraction from an inspiraling configuration of merging black holes

Geometry and regularity of moving punctures

Mark Hannam, Sascha Husa, Denis Pollney, Bernd Brügmann, and Niall Ó Murchadha · 2007

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Calibration of moving puncture simulations

Bernd Brügmann, José A. González, Mark Hannam, Sascha Husa, Ulrich Sperhake, and Wolfgang Tichy · 2008

Later among the works it cites.

Reducing phase error in long numerical binary black hole evolutions with sixth order finite differencing

Sascha Husa, José A. González, Mark Hannam, Bernd Brügmann, and Ulrich Sperhake · 2008

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Accurate effective-one-body waveforms of inspiralling and coalescing black-hole binaries

Thibault Damour, Alessandro Nagar, Mark Hannam, Sascha Husa, and Bernd Brügmann · 2008

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Black-hole binary simulations: the mass ratio 10:1

José A. González, Ulrich Sperhake, and Bernd Brügmann · 2009

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Schwarzschild black hole as moving puncture in isotropic coordinates