Loop quantization of spherically symmetric midi-superspaces
arXiv:gr-qc/0703135 · doi:10.1088/0264-9381/24/14/007
Abstract
We quantize the exterior of spherically symmetric vacuum space-times using a midi-superspace reduction within the Ashtekar new variables. Through a partial gauge fixing we eliminate the diffeomorphism constraint and are left with a Hamiltonian constraint that is first class. We complete the quantization in the loop representation. We also use the model to discuss the issues that will arise in more general contexts in the ``uniform discretization'' approach to the dynamics.
18 pages, RevTex, no figures, some typos corrected, published version, for some reason a series of figures were incorrectly added to the previous version
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Cited by in corpus (10)
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- Physical time and other conceptual issues of QG on the example of LQC
- Singularities in loop quantum cosmology
- Emergent diffeomorphism invariance in a discrete loop quantum gravity model
- Holography from loop quantum gravity
- Black holes and Rindler superspace: classical singularity and quantum unitarity