Testing the correctness of the Poynting vector E× B as the momentum density of gauge fields
Abstract
Following our recent finding that the renowned formula x× ( E× B) is not the correct density for the electromagnetic angular momentum, here we examine the validity of the Poynting vector E × B as the electromagnetic momentum density (or energy flux). The competitor is the gauge-invariant canonical momentum Ei ∇ Ai. It often gives the same result as E× B, but we propose that a delicate measurement (of the azimuthal energy flow in polarized atomic radiations) can make a discrimination. By clarifying the profound difference between two kinds of energy-momentum tensors: the canonical (or mechanical) one and the symmetric (or gravitational) one, we predict that it is Ei ∇ Ai that would pass the delicate experimental test. Our observations have far-reaching implications for understanding the source of gravity, and the nucleon momentum as well.
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