Physics
Scientific paper
Feb 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005tmgm.meet.1041m&link_type=abstract
The Tenth Marcel Grossmann Meeting. Proceedings of the MG10 Meeting held at Brazilian Center for Research in Physics (CBPF), Rio
Physics
Scientific paper
A new solution for the final state of gravitational collapse is proposed. A simple model with a purely vacuum energy de Sitter interior with pv = -ρv, and Schwarzschild exterior of arbitrary total mass M is outlined. These are separated by a thin shell with a small but finite proper thickness ℓ of fluid with eq. of state p = +ρ. This boundary layer is a quantum transition region which replaces the event horizons of the classical de Sitter and Schwarzschild solutions, through which the vacuum energy changes. The new solution has no singularities, no event horizons, and a global time. Its entropy is maximized under small fluctuations and is given by the standard hydrodynamic entropy of the thin shell, which is of order kBℓMc/ħ, instead of the Bekenstein-Hawking entropy formula, SBH = 4πkBGM2/ħc. Unlike black holes, the new solution is thermodynamically stable and has no information paradox.
Mazur Pawel O.
Mottola Emil
No associations
LandOfFree
Dark Energy and Condensate Stars:. a Quantum Alternative to Classical Black Holes 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 Dark Energy and Condensate Stars:. a Quantum Alternative to Classical Black Holes, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Dark Energy and Condensate Stars:. a Quantum Alternative to Classical Black Holes will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-833740