Mart Gibson
The Quantum Inertial Field as a Function of Cosmic Acceleration
The quantum inertial field generated by the action of cosmic expansion on
the waveform of a quantum half spin particle is investigated. The
spacetime/vacuum of general relativity/quantum field theory is held to be a
continuum or matrix demonstrating the property of inertia. Cosmic expansion
produces a tension or potential across the cosmic field, resulting in a
local change in the linear inertial density of the matrix which is evidenced
as a differential pressure on the surface of a half spin waveform. This
pressure differential or gradient does work on the surface of the rotational
oscillation generating quantum spin and quantum gravity. The nature of a
free half spin waveform with no translational motion is analyzed and the
field equations of the interaction of that waveform and the pressure
gradient are derived and presented as a quantum solution to the field
equation of general relativity. Finally the equations are evaluated using
observed quantum measurements with respect to gravitational, electroweak and
strong interactions.
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