On the Stueckelberg Like Generalization of General Relativity
Apr, 201116 pages
Published in:
- J.Phys.Conf.Ser. 330 (2011) 012011
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e-Print:
- 1104.2462 [math-ph]
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Abstract: (arXiv)
We first consider the Klein-Gordon equation in the 6-dimensional space with signature and show how it reduces to the Stueckelberg equation in the 4-dimensional spacetime . A field that satisfies the Stueckelberg equation depends not only on the four spacetime coordinates , but also on an extra parameter , the so called evolution time. In our setup, comes from the extra two dimensions. We point out that the space can be identified with a subspace of the 16-dimensional Clifford space, a manifold whose tangent space at any point is the Clifford algebra Cl(1,3). Clifford space is the space of oriented -volumes, , associated with the extended objects living in . We consider the Einstein equations that describe a generic curved space . The metric tensor depends on six coordinates. In the presence of an isometry given by a suitable Killing vector field, the metric tensor depends on five coordinates only, which include . Following the formalism of the canonical classical and quantum gravity, we perform the 4 + 1 decomposition of the 5-dimensional general relativity and arrive, after the quantization, at a generalized Wheeler-DeWitt equation for a wave functional that depends on the 4-metric of spacetime, the matter coordinates, and . Such generalized theory resolves some well known problems of quantum gravity, including "the problem of time".Note:
- 18 pages. Presented at "The 7th Biennial Conference on Classical and Quantum Relativistic Dynamics of Particles and Fields", 30 May - 1 June 2010, National Dong HWa University - Hualien, Taiwan; published version of the paper
- space: Clifford
- vector: Killing
- field theory: vector
- space-time
- general relativity
- quantum gravity
- Wheeler-DeWitt equation
- Klein-Gordon equation
- Einstein equation
- talk
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