Authors: Ankur S. Bhatt, F. M. Becker
Here a correlation to the exact fine-structure constant is found. This derivation suggests that the fine structure constant can be theoretically determined as a Lambert function that utilizes the spectrum range of all the energy modes (radiation modes) that fit inside the observable universe between the particle horizon down to Planck Length. Alternatively, this also could be interpreted as the Lambert function of the particle horizon in natural units. Several methods use hyperbolic geometry to achieve full convergence. A compilation of various convergent equations are found to represent the fine structure constant.
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[v1] 2022-06-23 21:06:56
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