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Phys. Rev. D 71, 081501(R) (2005) [5 pages]

Spherically symmetric quantum horizons

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Martin Bojowald*
Max-Planck-Institut für Gravitationsphysik, Albert-Einstein-Institut, Am Mühlenberg 1, D-14476 Potsdam, Germany

Rafal Swiderski
Max-Planck-Institut für Gravitationsphysik, Albert-Einstein-Institut, Am Mühlenberg 1, D-14476 Potsdam, Germany

Received 12 October 2004; revised 15 December 2004; published 8 April 2005

Isolated horizon conditions specialized to spherical symmetry can be imposed directly at the quantum level. This answers several questions concerning horizon degrees of freedom, which are seen to be related to orientation, and its fluctuations at the kinematical as well as dynamical level. In particular, in the absence of scalar or fermionic matter the horizon area is an approximate quantum observable. Including different kinds of matter fields allows to probe several aspects of the Hamiltonian constraint of quantum geometry that are important in inhomogeneous situations.

© 2005 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevD.71.081501
DOI:
10.1103/PhysRevD.71.081501
PACS:
04.70.Dy, 04.60.Pp

*Electronic address: mabo@aei.mpg.de

Electronic address: swiderski@aei.mpg.de