Planck's Constant as a Dynamical Field & Path Integral
Rand Dannenberg

TL;DR
This paper models Planck's constant as a dynamic field with solutions that include standing waves and decay modes, linking its variability to astrophysical phenomena and incorporating it into path integral formulations.
Contribution
It introduces a novel field-theoretic approach to treat Planck's constant as a dynamical entity with specific solutions and explores its implications in astrophysics and cosmology.
Findings
Derived a positional dependence of Planck's constant matching previous theoretical models
Identified three solutions for the acton field with distinct physical properties
Connected the variability of Planck's constant to astrophysical and cosmological contexts
Abstract
The constant h is elevated to a dynamical field, coupling to other fields, and itself, through the Lagrangian density derivative terms. The spatial and temporal dependence of h falls directly out of the field equations themselves. Three solutions are found: a free field with a tadpole term; a standing-wave non-propagating mode; a non-oscillating non-propagating mode. The first two are quantizable, and the third is not. The third corresponds to a zero-momentum classical field that naturally decays spatially to a constant with no ad-hoc terms added to the Lagrangian. An attempt is made to calibrate the constants in the third solution based on experimental data. The three fields are referred to as actons. It is tentatively concluded that the acton origin coincides with a massive body, or point of infinite density, though is not mass dependent. An expression for the positional dependence of…
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Taxonomy
TopicsAdvanced Thermodynamics and Statistical Mechanics · Experimental and Theoretical Physics Studies · Quantum Mechanics and Applications
