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Towards standard testbeds for numerical relativity

Towards standard testbeds for numerical relativity
Towards standard testbeds for numerical relativity
In recent years, many different numerical evolution schemes for Einstein's equations have been proposed to address stability and accuracy problems that have plagued the numerical relativity community for decades. Some of these approaches have been tested on different spacetimes, and conclusions have been drawn based on these tests. However, differences in results originate from many sources, including not only formulations of the equations, but also gauges, boundary conditions, numerical methods and so on. We propose to build up a suite of standardized testbeds for comparing approaches to the numerical evolution of Einstein's equations that are designed to both probe their strengths and weaknesses and to separate out different effects, and their causes, seen in the results. We discuss general design principles of suitable testbeds, and we present an initial round of simple tests with periodic boundary conditions. This is a pivotal first step towards building a suite of testbeds to serve the numerical relativists and researchers from related fields who wish to assess the capabilities of numerical relativity codes. We present some examples of how these tests can be quite effective in revealing various limitations of different approaches, and illustrating their differences. The tests are presently limited to vacuum spacetimes, can be run on modest computational resources and can be used with many different approaches used in the relativity community.
0264-9381
589-613
Alcubierre, Miguel
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Allen, Gabrielle
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Bona, Carles
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Fiske, David
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Goodale, Tom
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Guzmán, F. Siddhartha
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Hawke, Ian
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Hawley, Scott H.
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Husa, Sascha
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Koppitz, Michael
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Lechner, Christiane
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Pollney, Denis
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Rideout, David
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Salgado, Marcelo
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Schnetter, Erik
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Seidel, Edward
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Shinkai, Hisa-aki
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Shoemaker, Deidre
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Szilágyi, Béla
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Takahashi, Ryoji
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Winicour, Jeff
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Alcubierre, Miguel
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Allen, Gabrielle
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Bona, Carles
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Fiske, David
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Goodale, Tom
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Guzmán, F. Siddhartha
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Hawke, Ian
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Hawley, Scott H.
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Husa, Sascha
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Koppitz, Michael
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Lechner, Christiane
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Pollney, Denis
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Rideout, David
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Salgado, Marcelo
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Schnetter, Erik
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Seidel, Edward
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Shinkai, Hisa-aki
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Shoemaker, Deidre
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Szilágyi, Béla
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Takahashi, Ryoji
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Winicour, Jeff
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Alcubierre, Miguel, Allen, Gabrielle, Bona, Carles, Fiske, David, Goodale, Tom, Guzmán, F. Siddhartha, Hawke, Ian, Hawley, Scott H., Husa, Sascha, Koppitz, Michael, Lechner, Christiane, Pollney, Denis, Rideout, David, Salgado, Marcelo, Schnetter, Erik, Seidel, Edward, Shinkai, Hisa-aki, Shoemaker, Deidre, Szilágyi, Béla, Takahashi, Ryoji and Winicour, Jeff (2004) Towards standard testbeds for numerical relativity. Classical and Quantum Gravity, 21 (2), 589-613. (doi:10.1088/0264-9381/21/2/019).

Record type: Article

Abstract

In recent years, many different numerical evolution schemes for Einstein's equations have been proposed to address stability and accuracy problems that have plagued the numerical relativity community for decades. Some of these approaches have been tested on different spacetimes, and conclusions have been drawn based on these tests. However, differences in results originate from many sources, including not only formulations of the equations, but also gauges, boundary conditions, numerical methods and so on. We propose to build up a suite of standardized testbeds for comparing approaches to the numerical evolution of Einstein's equations that are designed to both probe their strengths and weaknesses and to separate out different effects, and their causes, seen in the results. We discuss general design principles of suitable testbeds, and we present an initial round of simple tests with periodic boundary conditions. This is a pivotal first step towards building a suite of testbeds to serve the numerical relativists and researchers from related fields who wish to assess the capabilities of numerical relativity codes. We present some examples of how these tests can be quite effective in revealing various limitations of different approaches, and illustrating their differences. The tests are presently limited to vacuum spacetimes, can be run on modest computational resources and can be used with many different approaches used in the relativity community.

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Published date: 2004

Identifiers

Local EPrints ID: 29315
URI: http://eprints.soton.ac.uk/id/eprint/29315
ISSN: 0264-9381
PURE UUID: 0b952192-63e4-40c6-8fb9-225bb463969c

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Date deposited: 11 May 2006
Last modified: 15 Mar 2024 07:30

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Contributors

Author: Miguel Alcubierre
Author: Gabrielle Allen
Author: Carles Bona
Author: David Fiske
Author: Tom Goodale
Author: F. Siddhartha Guzmán
Author: Ian Hawke
Author: Scott H. Hawley
Author: Sascha Husa
Author: Michael Koppitz
Author: Christiane Lechner
Author: Denis Pollney
Author: David Rideout
Author: Marcelo Salgado
Author: Erik Schnetter
Author: Edward Seidel
Author: Hisa-aki Shinkai
Author: Deidre Shoemaker
Author: Béla Szilágyi
Author: Ryoji Takahashi
Author: Jeff Winicour

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