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| One of the primary objectives of numerical relativity is to acquire a comprehensive understanding of the complex nature of strong dynamical gravitational fields. Another topic studied in this field includes the initial value problem of vacuum relativity. This involves ], discretization techniques for these equations, treatment of black hole spacetimes, and the imposition of boundary conditions. | One of the primary objectives of numerical relativity is to acquire a comprehensive understanding of the complex nature of strong dynamical gravitational fields. Another topic studied in this field includes the initial value problem of vacuum relativity. This involves ], discretization techniques for these equations, treatment of black hole spacetimes, and the imposition of boundary conditions. | ||
| Although many facets are shared with large scale problems in other computational sciences | |||
| like computational fluid dynamics, electromagnetics, and solid mechanics, and will develop with further advancements in these areas of research, numerical relativity offers challenging problems in copututation that have yet to be addressed as it is distinct from classical field theories. | |||
Revision as of 02:56, 26 April 2005
Numerical relativity is a subfield of computational physics that aims to establish numerical solutions to Einstein's field equations in general relativity. Despite promising results, accurate and validated algorithms for Einstein's equations remain elusive. The size and complexity of the equations along with persisting inquiries in fundamental issues of relativity theory are attributed the cause of thus far unsuccessful attempts at resolution. Nonetheless, the field has prodigiously expanded in recent years as engaging research continues.
One of the primary objectives of numerical relativity is to acquire a comprehensive understanding of the complex nature of strong dynamical gravitational fields. Another topic studied in this field includes the initial value problem of vacuum relativity. This involves partial differential equations, discretization techniques for these equations, treatment of black hole spacetimes, and the imposition of boundary conditions.
Although many facets are shared with large scale problems in other computational sciences like computational fluid dynamics, electromagnetics, and solid mechanics, and will develop with further advancements in these areas of research, numerical relativity offers challenging problems in copututation that have yet to be addressed as it is distinct from classical field theories.