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geometrodynamics

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In theoretical physics, geometrodynamics is an attempt to describe spacetime and associated phenomena completely in terms of geometry. Technically, its goal is to unify the fundamental forces and reformulate general relativity as a configuration space of three-metrics, modulo three-dimensional diffeomorphisms. The origin of this idea can be found in an English mathematician William Kingdon Clifford's works. This theory was enthusiastically promoted by John Wheeler in the 1960s, and work on it continues in the 21st century.

~9 min read

Encyclopedic overview

8 sections
Contents
  • Einstein's geometrodynamics
  • Wheeler's geometrodynamics
  • Modern notions of geometrodynamics
  • See also
  • References
  • Works cited
  • General references
  • Further reading

In theoretical physics, geometrodynamics is an attempt to describe spacetime and associated phenomena completely in terms of geometry. Technically, its goal is to unify the fundamental forces and reformulate general relativity as a configuration space of three-metrics, modulo three-dimensional diffeomorphisms. The origin of this idea can be found in an English mathematician William Kingdon Clifford's works. This theory was enthusiastically promoted by John Wheeler in the 1960s, and work on it continues in the 21st century.

==Einstein's geometrodynamics==

Excerpted from Wikipedia’s “geometrodynamics” article, available under the CC BY-SA 4.0 licence.

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