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The constant h is elevated to a dynamical field, coupling to other fields,and itself, through the Lagrangian density derivative terms. The spatial andtemporal dependence of h falls directly out of the field equations themselves.Three solutions are found: a free field with a tadpole term; a standing-wavenon-propagating mode; a non-oscillating non-propagating mode. The first two arequantizable, and the third is not. The third corresponds to a zero-momentumclassical field that naturally decays spatially to a constant with no ad-hocterms added to the Lagrangian. An attempt is made to calibrate the constants inthe third solution based on experimental data. The three fields are referred toas actons. It is tentatively concluded that the acton origin coincides with amassive body, or point of infinite density, though is not mass dependent. Anexpression for the positional dependence of Planck's constant is derived from afield theory in this work that matches in functional form that of one derivedfrom considerations of Local Position Invariance violation in GR in anotherpaper by this author. Astrophysical and Cosmological interpretations areprovided. A treatment of variable Planck's constant in a path integral isappended.

Planck's Constant as a Dynamical Field & Path Integral