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    The Superposition Principle of Waves Not Fulfilled under M. W. Evans' O(3) Hypothesis

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    In 1992 M.W. Evans proposed a so-called O(3) symmetry of electromagnetic fields by adding a constant longitudinal "ghost field" to the well-known transversal plane em waves. He considered this symmetry as a new law of electromagnetics. Later on, since 2002, this O(3) symmetry became the center of his Generally Covariant Unified Field Theory which he recently renamed as ECE Theory. One of the best-checked laws of electrodynamics is the principle of linear superposition of electromagnetic waves, manifesting itself in interference phenomena. Its mathematical equivalent is the representation of electric and magnetic fields as vectors. By considering the superposition of two phase-shifted waves we show that the superposition principle is incompatible with M.W. Evans' O(3) hypothesis.Comment: 5 pages, no figure

    On the virial theorem for the relativistic operator of Brown and Ravenhall, and the absence of embedded eigenvalues

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    A virial theorem is established for the operator proposed by Brown and Ravenhall as a model for relativistic one-electron atoms. As a consequence, it is proved that the operator has no eigenvalues greater than max(mc2,2αZ12)\max(m c^2, 2 \alpha Z - \frac{1}{2}), where α\alpha is the fine structure constant, for all values of the nuclear charge ZZ below the critical value ZcZ_c: in particular there are no eigenvalues embedded in the essential spectrum when Z3/4αZ \leq 3/4 \alpha. Implications for the operators in the partial wave decomposition are also described.Comment: To appear in Letters in Math. Physic

    Hamiltonians of Spherically Symmetric, Scale-Free Galaxies in Action-Angle Coordinates

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    We present a simple formula for the Hamiltonian in terms of the actions for spherically symmetric, scale-free potentials. The Hamiltonian is a power-law or logarithmic function of a linear combination of the actions. Our expression reduces to the well-known results for the familiar cases of the harmonic oscillator and the Kepler potential. For other power-laws, as well as for the singular isothermal sphere, it is exact for the radial and circular orbits, and very accurate for general orbits. Numerical tests show that the errors are always small, with mean errors across a grid of actions always less than 1 % and maximum errors less than 2.5 %. Simple first-order corrections can reduce mean errors to less than 0.6 % and maximum errors to less than 1 %. We use our new result to show that :[1] the misalignment angle between debris in a stream and a progenitor is always very nearly zero in spherical scale-free potentials, demonstrating that streams can be sometimes well approximated by orbits, [2] the effects of an adiabatic change in the stellar density profile in the inner regions of a galaxy weaken any existing 1/r density cusp, which is reduced to 1/r1/31/r^{1/3}. More generally, we derive the full range of adiabatic cusp transformations and show how to relate the starting cusp index to the final cusp index. It follows that adiabatic transformations can never erase a dark matter cusp.Comment: 6 pages, MNRAS, in pres

    Dirac-Sobolev inequalities and estimates for the zero modes of massless Dirac operators

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    The paper analyses the decay of any zero modes that might exist for a massless Dirac operator H:= \ba \cdot (1/i) \bgrad + Q, where QQ is 4×44 \times 4-matrix-valued and of order O(|\x|^{-1}) at infinity. The approach is based on inversion with respect to the unit sphere in R3\R^3 and establishing embedding theorems for Dirac-Sobolev spaces of spinors ff which are such that ff and HfHf lie in (Lp(R3))4,1p<.(L^p(\R^3))^4, 1\le p<\infty.Comment: 11 page
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