Statistics – Applications
Scientific paper
Jan 2002
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aipc..608..633m&link_type=abstract
SPACE TECHNOLOGY AND APPLICATIONS INTERNATIONAL FORUM- STAIF 2002. Conference on Thermophyiscs in Microgravity; Conference on In
Statistics
Applications
Spaceborne And Space Research Instruments, Apparatus, And Components, Einstein-Maxwell Spacetimes, Spacetimes With Fluids, Radiation Or Classical Fields
Scientific paper
Here it is conjectured that the part of the universe that we see that is expanding is in fact a solution to the Dirac Equation itself, an electron. Recall previous attempts to associate fractalness with a spin 0 boson in lets say the Wheeler De Witt Equation (Tufts U. Seminar, 1990, ``Wave function of the Universe''). A spin 1/2 particle is allowed because the spin would be nearly unnoticable due to inertial frame dragging. And of course we know that bosons themselves are composed of spin 1/2 particles so to make the fractalness universal we need a spin 1/2 fractal seed particle that the universe is selfsimilar to. The universe could then have an expansion stage (recall electron zitterbwegung motions) and would rotate (spin), but the rotation would be nearly unobservable for an INside observor due to inertial frame dragging. That makes the derivations easy since it means that we can then solve the Einstein equations for a spherical symmetry (getting the old Schwarzchild metric result) with the rotation (involving the Kerr metric) and oscillation (involving the Birkhoff theorem) as mere perturbations. The results are very interesting. Among them is the fact that the universe couldn't have expanded from a point (as in the inflationary scenario), but from a region just large enough to contain the baryons (it could fit within Mercury's orbit). And we also find a generally covariant Dirac equation that has for E=dt/ds√(g)00. Recall the (Dirac equation) zitterbewegung oscillation for an observor OUTside the horizon. But the Hamiltonian H (which is ω=
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