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Originally Posted by Fraser
In the first few moments of the Universe, enormous amounts of both matter and antimatter were created, and then moments later combined and annihilated generating the energy that drove the expansion of the Universe. But for some reason, there was an infinitesimal amount more matter than antimatter. Everything that we see today was that tiny [...]
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Fraser. I would like to see a plot of the B/anti-B decay rates' discrepancies vs the 24 hour diurnal variation seen in the SNO solar neutrino results...which runs ~ 14%. A variation matching that oscillation would suggest that the rates might be closer/farther at aphelion and perihelion too. B meson decays, like any particle decay, are weak interactions, sensitive to ambient magnetic fields, and changing fluxes. pete