Astronomy and Astrophysics – Astrophysics – General Relativity and Quantum Cosmology
Scientific paper
2001-03-16
Astronomy and Astrophysics
Astrophysics
General Relativity and Quantum Cosmology
latex, 21 pages
Scientific paper
A family of spacetimes suitable for describing the matter conditions of a static, spherically symmetric quantum vacuum is studied, as well as its reliability for describing a regular model for the interior of a semiclassical, static black hole ---without ever invoking a mass shell for the final object. In paper I, this condition was seen to limit the search to only one, distinguished family, that was investigated in detail. Here it will be proven that, aside from being mathematically generic (in its uniqueness), this family exhibits beautiful physical properties, that one would reasonably demand from a collapse process, including the remarkable result that isotropization may take place conveniently far from the (unavoidable) regularization scale. The analysis is also extended in order to include the possibility of a stringy core, always within the limits imposed by the semiclassical approach to gravitation. This constitutes a first approximation to the final goal of trying to characterize a regular, self-gravitating, stringy black hole.
Elizalde Emilio
Hildebrandt Sergi R.
No associations
LandOfFree
A family of quantum interiors for ordinary and stringy black holes II: Geometric considerations and global properties does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with A family of quantum interiors for ordinary and stringy black holes II: Geometric considerations and global properties, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A family of quantum interiors for ordinary and stringy black holes II: Geometric considerations and global properties will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-638721