Astronomy and Astrophysics – Astrophysics – General Relativity and Quantum Cosmology
Scientific paper
2001-05-21
Astronomy and Astrophysics
Astrophysics
General Relativity and Quantum Cosmology
7 figures, 173 pages, PhD thesis TU-Vienna (advisor: Wolfgang Kummer), v2: shortened abstract, corrected typos, added referenc
Scientific paper
In this thesis special emphasis is put on the quantization of the spherically reduced Einstein-massless-Klein-Gordon model using a first order approach for geometric quantities, because phenomenologically it is probably the most relevant of all dilaton models with matter. After a Hamiltonian BRST analysis path integral quantization is performed using temporal gauge for the Cartan variables. Retrospectively, the simpler Faddeev-Popov approach turns out to be sufficient. It is possible to eliminate all unphysical and geometric quantities establishing a non-local and non-polynomial action depending solely on the scalar field and on some integration constants, fixed by suitable boundary conditions on the asymptotic effective line element. Then, attention is turned to the evaluation of the (two) lowest order tree vertices, explicitly assuming a perturbative expansion in the scalar field being valid. Each of them diverges, but unexpected cancellations yield a finite S-matrix element when both contributions are summed. The phenomenon of a "virtual black hole" -- already encountered in the simpler case of minimally coupled scalars in two dimensions -- occurs, as the study of the (matter dependent) metric reveals. A discussion of the scattering amplitude leads to the prediction of gravitational decay of spherical waves, a novel physical phenomenon. Several possible extensions conclude this dissertation.
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