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* {{cite journal | author= ] | title= Geometrodynamics and the Issue of the Final State, in "Relativity Groups and Topology" | publisher= Les Houches Lecture Notes 1963, Gordon and Breach | year=1965 }} * {{cite journal | author= ] | title= Geometrodynamics and the Issue of the Final State, in "Relativity Groups and Topology" | publisher= Les Houches Lecture Notes 1963, Gordon and Breach | year=1965 }}
* {{cite book | author=Misner, Charles W. Thorne, Kip S. & Wheeler, John Archibald | title=Gravitation | publisher=San Francisco: W. H. Freeman | year =1973 | isbn=0-7167-0344-0}} See ''chapter 42''. * {{cite book | author=Misner, Charles W. Thorne, Kip S. & Wheeler, John Archibald | title=Gravitation | publisher=San Francisco: W. H. Freeman | year =1973 | isbn=0-7167-0344-0}} See ''chapter 42''.
* {{ cite journal | author = G. Ponzano and Tullio E. Regge (1968) | title= Semiclassical limit of Racah coefficients in Spectroscopic and group theoretical methods in physics | pages=1-58 | publisher = North-Holland }}
* {{cite book | author= Herbert W. Hamber | title= Quantum Gravitation - The Feynman Path Integral Approach | publisher = Springer Publishing | year=2009 | doi=10.1007/978-3-540-85293-3 | isbn=978-3-540-85292-6}} See ch. 4 and 6. * {{cite book | author= Herbert W. Hamber | title= Quantum Gravitation - The Feynman Path Integral Approach | publisher = Springer Publishing | year=2009 | doi=10.1007/978-3-540-85293-3 | isbn=978-3-540-85292-6}} See ch. 4 and 6.
* {{cite journal | author= James B. Hartle | title= Simplicial MiniSuperSpace I. General Discussion | journal=Jour. Math. Physics | year=1985 | volume=26 | pages=804-812 | doi=10.1063/1.526571}} * {{cite journal | author= James B. Hartle | title= Simplicial MiniSuperSpace I. General Discussion | journal=Jour. Math. Physics | year=1985 | volume=26 | pages=804-812 | doi=10.1063/1.526571}}

Revision as of 03:31, 30 October 2014

In general relativity, Regge calculus is a formalism for producing simplicial approximations of spacetimes that are solutions to the Einstein field equation. The calculus was introduced by the Italian theoretician Tullio Regge in the early 1960s.

The starting point for Regge's work is the fact that every Lorentzian manifold admits a triangulation into simplices. Furthermore, the spacetime curvature can be expressed in terms of deficit angles associated with 2-faces where arrangements of 4-simplices meet. These 2-faces play the same role as the vertices where arrangements of triangles meet in a triangulation of a 2-manifold, which is easier to visualize. Here a vertex with a positive angular deficit represents a concentration of positive Gaussian curvature, whereas a vertex with a negative angular deficit represents a concentration of negative Gaussian curvature.

The deficit angles can be computed directly from the various edge lengths in the triangulation, which is equivalent to saying that the Riemann curvature tensor can be computed from the metric tensor of a Lorentzian manifold. Regge showed that the vacuum field equations can be reformulated as a restriction on these deficit angles. He then showed how this can be applied to evolve an initial spacelike hyperslice according to the vacuum field equation.

The result is that, starting with a triangulation of some spacelike hyperslice (which must itself satisfy a certain constraint equation), one can eventually obtain a simplicial approximation to a vacuum solution. This can be applied to difficult problems in numerical relativity such as simulating the collision of two black holes.

The elegant idea behind Regge calculus has motivated the construction of further generalizations of this idea. In particular, Regge calculus has been adapted to study quantum gravity.

See also

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