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| − | == Chandrasekhar (ET_2010_11) ==
| + | This page has been combined with [[Detailed Release Announcement]]. |
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| − | In preparation.
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| − | == Bohr (ET_2010_06) ==
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| − | We are pleased to announce the first release (code name "Bohr") of the
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| − | Einstein Toolkit, an open, community developed software infrastructure
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| − | for relativistic astrophysics. The Einstein Toolkit is a collection
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| − | of over 130 software components and tools for simulating and analyzing
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| − | general relativistic astrophysical systems that builds on numerous
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| − | software efforts in the numerical relativity community including
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| − | CactusEinstein, the Whisky hydrodynamics code, and the Carpet AMR
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| − | infrastructure. The Cactus Framework is used as the underlying
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| − | computational infrastructure providing large-scale parallelization,
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| − | general computational components, and a model for collaborative,
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| − | portable code development. The toolkit includes modules to build
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| − | complete codes for simulating black hole spacetimes as well as systems
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| − | governed by relativistic hydrodynamics. Current development in the
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| − | consortium is targeted at providing additional infrastructure for
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| − | general relativistic magnetohydrodynamics.
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| − | The Einstein Toolkit uses a distributed software model and its
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| − | different modules are developed, distributed, and supported either by
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| − | the core team of Einstein Toolkit Maintainers, or by individual
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| − | groups. Where modules are provided by external groups, the Einstein
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| − | Toolkit Maintainers provide quality control for modules for inclusion
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| − | in the toolkit and help coordinate support. The Einstein Toolkit
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| − | Maintainers currently involve postdocs and faculty from five different
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| − | institutions, and hold weekly meetings that are open for anyone to
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| − | join in.
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| − | Guiding principles for the design and implementation of the toolkit
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| − | include:
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| − | 1: Open, community-driven software development that encourages the
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| − | sharing of code across the community, prevents code duplication, and
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| − | leads to sustainable support and development of essential code.
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| − | 2: Well thought out and stable interfaces between components that
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| − | enable multiple implementations of physics capabilities, and allow
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| − | groups or individuals to concentrate on their areas of interest.
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| − | 3: Separation of physics software from computational science
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| − | infrastructure so that new technologies for large scale computing,
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| − | processor accelerators, or parallel I/O can be easily integrated with
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| − | science codes.
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| − | 4: The provision of complete working production codes to provide:
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| − | prototypes, standard benchmarks, and testcases; codes that are
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| − | available for and usable by the general astrophysics community; tools
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| − | for new researchers and groups to enter this field; training and
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| − | education for a new generation of researchers.
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| − | For more information about using or contributing to the Einstein
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| − | Toolkit, or to join the Einstein Toolkit Consortium, please visit our
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| − | web pages at <http://einsteintoolkit.org>.
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| − | We thank the numerous people who contributed to this software over the
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| − | past many years; there are too many to be listed here. We also
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| − | gratefully acknowledge those who helped in the past months to make
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| − | this release happen. The Einstein Toolkit is primarily supported by
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| − | NSF 0903973/0903782/0904015 (CIGR), and also by NSF 0701566/0855892
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| − | (XiRel), 0721915 (Alpaca), and 0905046/0941653 (PetaCactus).
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| − | The "Bohr" Release Team on behalf of the Einstein Toolkit Consortium
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| − | (2010-06-17)
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