The Problem of the Cosmological Constant
Tom Ostoma, Mike Trushyk
Abstract
ElectroMagnetic Quantum Gravity (EMQG) is applied to the problem of the Cosmological Constant. EMQG is a quantum gravity theory (ref. 1) in which the virtual particles of the quantum vacuum play a very important role in all gravitational interactions, and also in accelerated motion. According to EMQG theory (and quantum field theory in general), empty space is populated by vast numbers of virtual particles, consisting of virtual fermion and virtual anti-fermion particles, which posses mass, and also virtual boson particles of all the various force particle species. Therefore the problem of the cosmological constant is essentially equivalent to a determination of the mass contributed by all the virtual particles of the vacuum to the overall curvature and dynamics of the entire universe. Our original analysis was based on the assumption of perfect symmetry in the creation and destruction of virtual fermion and virtual anti-fermion particle pairs in the quantum vacuum, which is in accordance with the existing laws of conservation of both electric charge, and also of the new law of conservation of gravitational 'mass charge'. We now believe that this may not be necessarily true, and that EMQG can allow the possibility of a very tiny value for the cosmological constant. Furthermore, it turns out that this question can only be resolved when a solution to the problem of baryon asymmetry in the universe is resolved. In other words an answer must be found as to why our universe seems to contain only real matter, and very little, if any anti-matter.
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