Abstract
We have solved the de Sitter special relativistic ($SR_cR$-)
Dirac equation of hydrogen in the earth-QSO(quasar) framework reference by
means of the adiabatic approach. The aspects of geometry effects of de Sitter
space-time described by Beltrami metric are explored and taken into account. It
is found that the $SR_cR$-Dirac equation of hydrogen is a time
dependent quantum Hamiltonian system. We provide an explicit calculation to
justify the adiabatic approach in dealing with this time-dependent system.
Since the radius of de Sitter sphere $R$ is cosmologically large, the evolution
of the system is very slow so that the adiabatic approximation legitimately
works with high accuracy. We conclude that the electromagnetic fine-structure
constant, the electron mass and the Planck constant are time variations. The
prediction of fine-structure constant is consistent with the presently
available observation data. For confirming it further, experiments/observations
are required.
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