Holography and non-locality in a closed vacuum-dominated universe

Details Holography and non-locality in a closed vacuum-dominated universe Holography and non-locality in a closed vacuum-dominated universe

2006-09-28

arxiv.org/abs/gr-qc/0609128v2

Int.J.Theor.Phys.46:399-404,2007

Astronomy and Astrophysics

Astrophysics

General Relativity and Quantum Cosmology

4 pages, no figures, to be published in Int. J. Theor. Phys, references corrected

Scientific paper

10.1007/s10773-006-9241-x

A closed vacuum-dominated Friedmann universe is asymptotic to a de Sitter space with a cosmological event horizon for any observer. The holographic principle says the area of the horizon in Planck units determines the number of bits of information about the universe that will ever be available to any observer. The wavefunction describing the probability distribution of mass quanta associated with bits of information on the horizon is the boundary condition for the wavefunction specifying the probability distribution of mass quanta throughout the universe. Local interactions between mass quanta in the universe cause quantum transitions in the wavefunction specifying the distribution of mass throughout the universe, with instantaneous non-local effects throughout the universe.

Affiliated with

Also associated with

No associations

Rating

Holography and non-locality in a closed vacuum-dominated universe 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 Holography and non-locality in a closed vacuum-dominated universe, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Holography and non-locality in a closed vacuum-dominated universe will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-531607