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Lorenz fields convey energy as Nadelstrahlung

H. C. Potter
Abstract.

Gauge transformations leave unchanged only specific Maxwell fields. To reveal more, I develop Lorenz field equations for superposed, sourced and unsourced, wave function potentials. In this Maxwell form system, the Lorenz condition is charge conservation. This allows me to define three transformation classes that screen for Lorenz relevance. Nongauge, sans gauge function, Lorentz conditions add polarization fields. These enable emergent, light-like radiation. That from Lissajous potentials is Nadelstrahlung. It conveys energy localized like particles at charge conserving, progressive phase points. Such rays escape discovery in modern Maxwell fields where gauge transformations suppress the polarizations.

1. Introduction

In 1867, during the time when J. C. Maxwell (1831-79) was publishing his electromagnetic theory, L. V. Lorenz (1829-91) published his theory equating light vibrations with electric currents [1]. This work is translated to modern vector notation and critiqued in [2]. Lorenz starts with Kirchhoff’s Ohm’s law expression. For scalar potentials with a finite propagation speed, he obtains delayed potentials. These potentials satisfy inhomogeneous wave equations and, when charge is conserved, the eponic Lorenz condition [3, pp. 268-9]. They are nonlocal. All their derivatives also must be inhomogeneous wave function solutions for correspondingly differentiated remote sources. Since the potentials satisfy wave equations they can be augmented with homogeneous wave equation solutions. These sourceless augmentations are local. Their derivatives depend only on proximate values. The composite potentials still satisfy wave equations and the Lorenz condition with one and the same propagation speed. But they are no longer strictly delayed. Their differential character is mixed, local and nonlocal.

In his 1867 paper, Lorenz never develops first order field equations from his potentials. In fact, until now, this has been ignored. With magnetic induction as the vector potential curl, I obtain Lorenz field equations with Maxwell form. This allows Lorenz delay to be fully probed. For nonlocal potentials, the fields in these equations are nonlocal also. The desirable locality can be restored as a far field approximation for systems that satisfy specific size constraints [4, p. 222]. For the augmented potentials, the Lorenz field equations incorporate fields for electric displacement and magnetic field strength by adding polarization fields. This development is presented formally in Sec. 2. It shows that wave function potentials satisfying the Lorenz condition assure charge conservation. Thus, the form invariant Lorenz condition is charge conservation. This limits potentials transformation. Polarization radiation is described in Sec. 3. It should aid light mechanism study. Transformation and radiation aspects are discussed in Sec. 4.

2. Lorenz fields

The electromagnetic Lorenz potentials satisfy differential wave equations with charge, ρ\rho, and current, 𝐉\mathbf{J}, density sources and, when charge is conserved, the Lorenz condition

a𝐀=Ωt.-a\boldsymbol{\nabla}\bullet\mathbf{A}=\frac{\partial\Omega}{\partial t}. (1)

For sources distributed throughout all space, the potentials are given by

The wave equation operator for wave speed aa, a\square_{a}, is defined in Sec. 4.1. When the potentials are augmented by solutions to the homogeneous wave equation, aΩ0=a𝐀0=0\square_{a}\Omega_{0}=\square_{a}\mathbf{A}_{0}=0, the Lorenz condition takes the modified form

a(𝐀+𝐀0)=(Ω+Ω0)t.-a\boldsymbol{\nabla}\bullet(\mathbf{A}+\mathbf{A}_{0})=\frac{\partial(\Omega+\Omega_{0})}{\partial t}. (3)

The augmentations could be set to zero by implicit scalar strengths. For

and 𝐁=×𝐀,\mathbf{\mathbf{B}}=\mathbf{\boldsymbol{\nabla}}\times\mathbf{A}, (4b)

we also have the fields 𝐃=𝐄+𝐏\mathbf{D}=\mathbf{E}+\mathbf{P} and 𝐇=𝐁𝐌\mathbf{H}=\mathbf{B}-\mathbf{M}. The polarization fields are

and 𝐌=×𝐀0.\mathbf{M}=-\boldsymbol{\nabla}\times\mathbf{A}_{0}. (5b)

The ring denotes temporal partial differentiation. Constants for units adjustment are set to unit value. All fields satisfy wave equations with propagation speed aa. These definitions pass the augmentation strengths to the polarizations. Without strengths, the polarizations vanish when the augmentations are derived from a gauge function, i.e. when 𝐀0=χ\mathbf{A}_{0}=\boldsymbol{\nabla}\chi and Ω0=χ̊/a\Omega_{0}=-\mathring{\chi}/a. The fields satisfy Maxwell form equations:

a×𝐄=𝐁/t,a\mathbf{\boldsymbol{\nabla}}\times\mathbf{E}=-\partial\mathbf{\mathbf{B}}/\partial t, (6c)
a×𝐇=𝐃/t+4π𝐉.a\mathbf{\boldsymbol{\nabla}}\times\mathbf{H}=\partial\mathbf{D}/\partial t+4\pi\mathbf{J}. (6d)

Together Eqs. (6b) and (6d) give the condition for charge conservation

𝐉+ρt=0.\boldsymbol{\nabla}\bullet\mathbf{J}+\frac{\partial\rho}{\partial t}=0. (7)

The Eq. (3) Lorenz condition too gives this when acted on by the wave equation operator a\square_{a}.

Fields derived from the delayed potentials can not be proportional to those derived from the potential augmentations. This means coupling normally provided by the constitutive relations, 𝐃=ϵ𝐄\mathbf{D}=\epsilon\mathbf{E} and 𝐁=μ𝐇\mathbf{B}=\mu\mathbf{H}, is not primal. There are three choices. First, take the relations as valid in very small space-time volumes where boundary conditions are set. Second, further augment the potentials with proportional delayed potentials. Then, wave function speed can be adjusted for dielectric constant ϵ\epsilon and magnetic permeability μ\mu by measurement. Third, couple the fields by local and nonlocal fluxes. To see this, notice that the relation 𝐇(×𝐃)𝐃(×𝐇)=(𝐃×𝐇)\mathbf{H}\bullet(\boldsymbol{\nabla}\times\mathbf{D})-\mathbf{D}\bullet(\boldsymbol{\nabla}\times\mathbf{H})=\boldsymbol{\nabla}\bullet(\mathbf{D}\times\mathbf{H}) allows two energy continuity expressions to be obtained from Eqs. (6c) and (6d). When 𝐄\mathbf{E} and 𝐁\mathbf{B} are replaced by 𝐏\mathbf{P} and 𝐌\mathbf{M} using the expressions for 𝐃\mathbf{D} and 𝐇\mathbf{H},

a(𝐇×𝐃)=[𝐇𝐇t+𝐃𝐃t]+4π𝐃𝐉.a\boldsymbol{\nabla}\bullet(\mathbf{H}\times\mathbf{\mathbf{D}})=\left[\mathbf{H}\bullet\frac{\partial\mathbf{H}}{\partial t}+\mathbf{D}\bullet\frac{\partial\mathbf{D}}{\partial t}\right]+4\pi\mathbf{\mathbf{D}}\bullet\mathbf{\mathbf{J}}. (8a)
More directly,
a(𝐇×𝐄)=[𝐇𝐁t+𝐄𝐃t]+4π𝐄𝐉.a\boldsymbol{\nabla}\bullet(\mathbf{H}\times\mathbf{\mathbf{E}})=\left[\mathbf{H}\bullet\frac{\partial\mathbf{B}}{\partial t}+\mathbf{E}\bullet\frac{\partial\mathbf{D}}{\partial t}\right]+4\pi\mathbf{E}\bullet\mathbf{\mathbf{J}}. (8b)

Both exist when the polarizations vanish. But when 𝐄\mathbf{E} and 𝐁\mathbf{B} vanish, the latter vanishes and the former carries the entire flux. This coupling allows local polarization waves to emerge from a nonlocal electromagnetic field. The Hertz dipole radiation solution discussed in Sec. 4.2 is the only extant example which exhibits this emergence.

3. Polarization radiation

As sources go to zero the potentials become possible augmentations. So, the potential augmentations can conserve charge. These augmentations are then restrained by the Lorenz condition. Potentials in matter free space have not been so restrained previously. With this restraint, the potentials describe waves that can be considered to propagate by progressively conserving charge. Features are given in Sec. 3.1. There I show the polarizations will describe rays without the longitudinal fields that plague other formulations [5]. An example with Lissajous vector potential is presented in Sec. 3.2. In this instance rays are real space paths determined by linearly independent potential vector component phases. With neither wave packet dispersion [6] nor quantum mechanical nonlocality, these rays provide localization that has long eluded discovery. Localization to rays is relaxed for linearly dependent component phases.

3.1. Polarization waves

As representative Lorenz potential augmentations consider

When ff, gg and hh are functionally dependent only on phase factors ωt𝐤𝐫\omega t-\mathbf{k}\bullet\mathbf{r} where 𝐤=(kx,ky,kz)\mathbf{k}=(k_{x},k_{y},k_{z}) and a2k2=ω2a^{2}k^{2}=\omega^{2}, these potentials satisfy the homogeneous wave equation and the Lorenz condition. Since Ω0=Ω̊0𝐤/ω\boldsymbol{\nabla}\Omega_{0}=-\mathring{\Omega}_{0}\mathbf{k}/\omega and 𝐤×(𝐤×𝐀̊0)=𝐤(𝐤𝐀̊0)k2𝐀̊0\mathbf{k}\times(\mathbf{k}\times\mathring{\mathbf{A}}_{0})=\mathbf{k}(\mathbf{k}\bullet\mathring{\mathbf{A}}_{0})-k^{2}\mathring{\mathbf{A}}_{0},


When the vector potential components are periodic functions they can be considered to be plane waves. Unlike Lorenz fields defined by nonlocal potentials, the polarizations are local functions. They are orthogonal, 𝐏𝐌=0\mathbf{P}\bullet\mathbf{M}=0, and have no longitudinal components, 𝐤𝐏=𝐤𝐌=0\mathbf{k}\bullet\mathbf{P}=\mathbf{k}\bullet\mathbf{M}=0; they carry a flux 𝐌×𝐏=ω2(𝐤×𝐀̊0)2𝐤/k\mathbf{M}\times\mathbf{P}=\omega^{-2}(\mathbf{k}\times\mathring{\mathbf{A}}_{0})^{2}\mathbf{k}/k equal to 𝐃×𝐇\mathbf{D}\times\mathbf{H} when 𝐄=𝐁=0\mathbf{E}=\mathbf{B}=0 and travel indefinitely in a ray direction 𝐤\mathbf{k} at speed aa without driving sources.

3.2. Polarization flux localization

Polarization waves provide, at least, a classical solution to the [7, 8, 9, 21] duality. To see how, consider a vector potential with Lissajous phases ϕ1=ω1t𝐤1𝐫\phi_{1}=\omega_{1}t-\mathbf{k}_{1}\bullet\mathbf{r}, ϕ2=ω2t𝐤2𝐫\phi_{2}=\omega_{2}t-\mathbf{k}_{2}\bullet\mathbf{r} and ϕ3=ω3t𝐤3𝐫\phi_{3}=\omega_{3}t-\mathbf{k}_{3}\bullet\mathbf{r} where 𝐤1=(k1x,k1y,0)\mathbf{k}_{1}=(k_{1x},k_{1y},0), 𝐤2=(k2x,k2y,0)\mathbf{k}_{2}=(k_{2x},k_{2y},0) and 𝐤3=(0,0,k3z)\mathbf{k}_{3}=(0,0,k_{3z}). Though periodic components are not essential, added insight is provided by the simple form

𝐀0=(sinϕ1,sinϕ2,sinϕ3).\mathbf{A}_{0}=\left(\sin\phi_{1},\sin\phi_{2},\sin\phi_{3}\right). (11a)
When a2kI2=ωI2a^{2}k_{I}^{2}=\omega_{I}^{2} for I=1,2 or 3I=1,2\textrm{ or }3, a𝐀0=0\square_{a}\mathbf{A}_{0}=0. The Lorenz condition gives
Ω0=(k1x/k1)sinϕ1+(k2y/k2)sinϕ2+sinϕ3.\Omega_{0}=(k_{1x}/k_{1})\sin\phi_{1}+(k_{2y}/k_{2})\sin\phi_{2}+\sin\phi_{3}. (11b)

This also satisfies the homogeneous wave equation aΩ0=0\square_{a}\Omega_{0}=0. So these potentials can be taken to define the Eqs. (5) Lorenz polarizations and flux given in the Appendix.

When ϕ1=ϕ2=ϕ\phi_{1}=\phi_{2}=\phi for 𝐤1𝐤2\mathbf{k}_{1}\neq\mathbf{k}_{2} the phase moves on the parametric line

X(t)=[k2y(ω1tϕ)k1y(ω2tϕ)]/(k1xk2yk2xk1y),X(t)=[k_{2y}(\omega_{1}t-\phi)-k_{1y}(\omega_{2}t-\phi)]/(k_{1x}k_{2y}-k_{2x}k_{1y}), (12a)
Y(t)=[k2x(ω1tϕ)+k1x(ω2tϕ)]/(k1xk2yk2xk1y)Y(t)=[-k_{2x}(\omega_{1}t-\phi)+k_{1x}(\omega_{2}t-\phi)]/(k_{1x}k_{2y}-k_{2x}k_{1y}) (12b)

with velocity

𝐕=(k2yω1k1yω2,k1xω2k2xω1,0)/(k1xk2yk2xk1y)\mathbf{V}=(k_{2y}\omega_{1}-k_{1y}\omega_{2},k_{1x}\omega_{2}-k_{2x}\omega_{1},0)/(k_{1x}k_{2y}-k_{2x}k_{1y}) (13)

giving V2=2a2k1k2[k1k2(k1xk2x+k1yk2y)]/(k1xk2yk2xk1y)2V^{2}=2a^{2}k_{1}k_{2}[k_{1}k_{2}-(k_{1x}k_{2x}+k_{1y}k_{2y})]/(k_{1x}k_{2y}-k_{2x}k_{1y})^{2}. If the flux vector were to have a component perpendicular to the phase velocity the ray would dissipate. So the vector product components must vanish or, for the Eqs. (17c) and (13) flux and velocity,

(k2yω1k1yω2)(k2xk2yk2k1y2k1)(k1xω2k2xω1)(k1xk1yk1+k2x2k2)=0.(k_{2y}\omega_{1}-k_{1y}\omega_{2})(\frac{k_{2x}k_{2y}}{k_{2}}-\frac{k_{1y}^{2}}{k_{1}})-(k_{1x}\omega_{2}-k_{2x}\omega_{1})(-\frac{k_{1x}k_{1y}}{k_{1}}+\frac{k_{2x}^{2}}{k_{2}})=0. (14)

This reduces to (k1y+k2x)[k1k2(k1xk2x+k2yk1y)]=0(k_{1y}+k_{2x})[k_{1}k_{2}-(k_{1x}k_{2x}+k_{2y}k_{1y})]=0. So, 𝐤1\mathbf{k}_{1} and 𝐤2\mathbf{k}_{2} can satisfy two alternative conditions for flux and phase velocity directions to be aligned. The phase ϕ\phi is a parameter that gives simple harmonic polarizations. But ϕ\phi is not a wave phase factor unless ω1=ω2\omega_{1}=\omega_{2}, because it is confined to the line defined by Eqs. (12). As 𝐤1𝐤2\mathbf{k}_{1}\to\mathbf{k}_{2}, the ray-like character persists.

Although the case for 𝐤1𝐤2\mathbf{k}_{1}\neq\mathbf{k}_{2}would appear to have physical relevance in describing light-like waves, the more general case in which ϕ1ϕ2\phi_{1}\neq\phi_{2} may provide a particle description for light. In this case, the phase point (ϕ1,ϕ2)(\phi_{1},\phi_{2}) moves on a path defined by Eqs. (12) with ϕ\phi replaced by ϕ1\phi_{1} or ϕ2\phi_{2}. Now, the flux has the Eq. (16c) form. To prevent ray dissipation by flux components normal to the phase path, restraints must again be applied to 𝐤1\mathbf{k}_{1} and 𝐤2\mathbf{k}_{2}. These will depend on ϕ1\phi_{1} and ϕ2\phi_{2}. This means the flux is carried by phase points. This case is illustrated in Fig. 1 for select wave vector values that give 𝐕=(a,0,0)\mathbf{V}=(a,0,0). Construction details are given in the caption. Significantly, Fig. 1 shows that VV can equal aa even when 𝐕\mathbf{V} and 𝐌×𝐏\mathbf{M}\times\mathbf{P} are not aligned. The concentrated energy bearers can be marshaled into ensembles.

Refer to caption
Figure 1. This figure depicts a phase and flux directions non-alignment instance. Polarizations are defined by text Eqs. (11) Lissajous potentials with vector potential component wave vectors 𝐤1=([(2653)/16]12,3/8,0)\mathbf{k}_{1}=([(\sqrt{265}-3)/16]^{\frac{1}{2}},-\sqrt{3/8},0) and 𝐤2=(1/2,3/2,0)\mathbf{k}_{2}=(1/\sqrt{2},\sqrt{3/2},0). For these potentials the text Eq. (13) phase velocity, 𝐕\mathbf{V}, equals (a,0,0)(a,0,0). The hatching represents constant vector potential x- and y-component values at phases ϕ1=7.60+2πn\phi_{1}=-7.60+2\pi n and ϕ2=2.55+2πm\phi_{2}=2.55+2\pi m. These travel with wave speed aa in their respective wave vector directions. The Lissajous periodicities have the relative value (ω1/ω2)2=(k1/k2)2=(265+3)/320.60.(\omega_{1}/\omega_{2})^{2}=(k_{1}/k_{2})^{2}=(\sqrt{265}+3)/32\approx 0.60. The text Eq. (16a) electric polarization 𝐏\mathbf{P} at (ϕ1,ϕ2)(\phi_{1},\phi_{2}) has components 𝐏1\mathbf{P}_{1} normal to 𝐤1\mathbf{k}_{1} and 𝐏2\mathbf{P}_{2} normal to 𝐤2\mathbf{k}_{2}. These components depend independently on the 𝐤\mathbf{k}’s, ϕ\phi’s and vector potential component magnitudes to give a composite polarization 𝐏\mathbf{P} and flux 𝐌×𝐏\mathbf{M}\times\mathbf{P}. Both 𝐕\mathbf{V} and 𝐌×𝐏\mathbf{M}\times\mathbf{P} change magnitude and direction as the 𝐤\mathbf{k}’s are independently changed. But 𝐌×𝐏\mathbf{M}\times\mathbf{P} can be brought into alignment with fixed 𝐕\mathbf{V} by changing the vector potential component relative magnitudes and, equivalently for the Eqs. (11) potentials, the ϕ\phi’s. This alignment is required to keep a ray from dissipating.

4. Discussion

Above, I have shown the Lorenz condition can select light-like rays from electromagnetic fields. This permits light mechanism study. Also, its equivalence to charge conservation limits potentials transformation. These aspects are discussed below.

4.1. Potentials transformation

Early last century, H. A. Lorentz (1853-1928) made two comments on Maxwell field potentials. First, the Eqs. (4) electric field strength and magnetic induction are unchanged in form for any gauge function, χ\chi, that gives new potentials defined by

and Ω=Ω1+χ̊/a.\Omega=\Omega_{1}+\mathring{\chi}/a. (15b)

Gauge restraints are now widely accepted [10]. Some gauges do not even specify a gauge function. For these, a gauge function further restrains the potentials. The second comment was that Eq. (1), dubbed the Lorentz condition, causes the Maxwell field potentials to satisfy the Eqs. (2) wave equations. This is shown in [11]. Lorentz did not relate these comments. So, the Lorentz condition has been treated as a gauge that can be freely changed. This freedom and wave function potential nonlocality have caused potential reality to be denied. When Eq. (1) is charge conservation, as I have shown above that it is, these comments are coupled. As charge conservation, Eq. (1) is a basic law. With this, in Sec. 2 I have shown the Eqs. (2) wave function potentials give the Eq. (6) field equations with Maxwell form. This is the second comment converse. Thus, Maxwell fields must always have wave function potentials. The potentials can be local, nonlocal or mixed. Further, as a basic law, Eq. (1) can not be freely changed.

When the original potentials are sourced wave functions Eqs. (15) resolve to three Lorenz classes that need not have the gauge function form. First, the new potentials are not wave functions. Second, the new potentials are wave functions with changed source values. Third, the new potentials are wave functions with unchanged source values. In the first case the Lorentz condition will not apply. Then, charge will not be conserved and the potentials will not propagate with a wave speed. Both must be spurned. The latter, because tests in [12, 13, 14, 15] show longitudinal electric fields to propagate with finite speed. The last two cases will conserve charge if the Lorentz condition persists. This persistence will assure Lorenz field equations in which charge and current density are deemed observables that produce potentials and fields yielding emergent light-like waves. These conserve charge progressively as described in Sec. 3.1. Further, localized energy is conveyed on ray forming phase points as described in Sec. 3.2. For gauge transformations, persistence requires the Lorenz gauge, aχχχ/a2=0\square_{a}\chi\equiv\boldsymbol{\nabla}\bullet\boldsymbol{\nabla}\chi-\overset{\circ\circ}{\chi}/a^{2}=0. It suppresses the polarizations and, thus, their dependent, emergent rays.

4.2. Light mechanization

In the late eighteen hundreds, H. von Helmholtz (1821-94) tried to unite electromagnetic theories [16]. To this end he based his concept on electric and magnetic polarization. From this he obtained wave equations for a homogeneous medium. His transverse waves have speed c/ϵμc/\sqrt{\epsilon\mu}. Here cc is the vacuum light speed. Only difficult, precision measurements could complete the theory, because his longitudinal wave speed has any value greater than or equal to zero. Unlike Helmholtz waves, Lorenz waves are simply transverse, because Eq. (6b) gives 𝐏=0\boldsymbol{\nabla}\bullet\mathbf{P}=0.

To promote his concept, Helmholtz issued a challenge to measure a coupling between electromagnetism and dielectric polarization. His former student, H. Hertz (1857-94), later claimed the prize. He then went on to observe dipole radiation reflection and interference. Based on this Hertz concluded that polarization propagation is like vacuum light [17, pp. 19 and 122-3] and [18]. Hertz’s dipole field [4, 17, 18] has radial, transverse wave emergence in the far field. At intermediate distances the waves have greater than light speed that approaches light speed in the far field. These waves change from longitudinal to transverse as the radial direction changes from dipole length to dipole equator. Hertz reconciled these properties in the equatorial plane by observing strobed interference between free air and straight wire waves [17, pp. 150-5]. His and recent [19] reports suggest light structure may be open to study. Antiphased fields in [19] may represent an Eq. (6d) Ampere law based, magnetoinductive internal structure [2].

For vacuum polarization waves Eq. (8a) takes a simple form. By the Gauss theorem, it represents an equality between the temporal energy change in a volume and the energy flux through its surface. For monochromatic waves, 𝐌×𝐏\mathbf{M}\times\mathbf{P} can be written using the Hertz analogy as hν𝐟h\nu\mathbf{f} where hνh\nu is photon energy and 𝐟\mathbf{f} is photon flux with coherence length inversely related to monochromaticity departure [20]. This dependence means that the photon power density must approach zero as the coherence length becomes very large for monochromatic photons. The compact, quantum particle photon concept is untenable in this limit. The concept is further threaten by confounding photon size with wavelength. This problem is revealed by the Table 1 benchmarks. There the lowest energy photons have a wavelength greater than the Earth orbit radius. These conflicts are homologized in [21] by setting a hypothetical photon energy density equal to a flux magnitude divided by the energy transfer speed.

Table 1. Some Vacuum Photon Properties
Energy Frequency Wavelength Energy Frequency Wavelength
   hνh\nu    ν\nu Hz    λ\lambda cm    hνh\nu    ν\nu Hz    λ\lambda cm
1 GeV 0.241E24 12.4E-14 1 μ\mueV [17] 0.241E9 12.4E1
1 MeV 0.241E21 12.4E-11 1 neV 0.241E6 12.4E4
1 keV 0.241E18 12.4E-8 1 peV 0.241E3 12.4E7
1 eV 0.241E15 12.4E-5 1 feV 0.241 12.4E10
1 meV 0.241E12 12.4E-2 1 aeV [19] 0.241E-3 12.4E13

For energy, hh is Planck’s constant. Electron rest mass equals 0.5 MeV, visible light at 5000 Å\mathring{\textrm{A}} equals 2.48 eV and cosmic microwave background radiation at 3 K equals 0.26 meV. Atomic nucleus radii are about E-12 cm, atomic radii are about E-8 cm, Earth radius is 6.38E8 cm and Earth orbit radius is 1.5E13 cm. Solar radiant energy flux at Earth is 8.58E21 eV/(s m2) with an energy distribution that should be appropriate for the 5780 K effective sun temperature. The H. Hertz, Electric Waves, D. E. Jones, trans. (Dover Pubs., Inc., NY, 1962) and P. J. Chi and C. T. Russell, “Phase skipping and Poynting flux of continuous pulsations,” J. Geophys. Res. 𝟏𝟎𝟑\mathbf{103}:A12, 29479-29491(1998) citations attempt internal structure study.

When phase point motion and wave flux are not aligned, flux normal to the phase point motion would force ray dissipation. This is like saying that all light rays are electromagnetic, but not all electromagnetic waves are light rays. Failure to recognize this has prevented light-like rays from being found in electromagnetic fields to help describe light behavior in optics and photography [7, 8, 9]. Synchrotron light emitted as rays by high speed electrons in a circular orbit supports this. These rays are attributed to the radial acceleration not the periodic linear acceleration required to maintain the electron energy. Their presence in the electric field has not been shown [22, 23, 24]. However, one unconfirmed report [25] finds them to be electrically polarized in the electron orbit plane like the Sec. 3.2 phase directed polarization waves.

Although phase independence is compelling, its nonexistence would support treating rays as having the closely bound potentials described in Sec. 3.1 above. In this limit energy should still be borne progressively by charge conserving phase points. Even so, phase independence is a hidden variable whose consequence is unintuitive. Whether electromagnetic energy localization to phase points is consistent with quantum statistics should be examined elsewhere, because it has special features to help model the standard quantum oscillators. The points are defined by Lissajous potentials. They bear a fixed flux at constant speed. They vanish where either charge cannot be conserved or flux and phase are not aligned. Individually, they do not bear oscillations. But they can be marshaled into Eq. (20), Piekara bead-chain, flux magnitude beads. These features provide a new means to help describe light generation. If flux and phase alignment were required for light generation, its low intrinsic likelihood would predict a small efficiency. One challenge is light from atoms. Its study could help increase laser output when atoms are aligned by shell structure.

5. Conclusion

I have shown that if Lorenz had published field equations electromagnetism as we know it today would have a solid, delay based etiology. We would have Lorenz condition equivalence to charge conservation, light-like ray emergence from fields and energy conveyance by field phase points. Based on this I propose that the terms “Lorenz condition" and “Lorentz condition" be retained. The Lorentz condition would be only a potentials transformation. The Lorenz condition would express charge conservation in a form left unchanged by potentials transformation, Lorenz covariance. Further, the light-like rays that convey localized energy in Lorenz fields escape discovery in modern Maxwell fields. So, they may aid photon mechanization.

Appendix

For the Eqs. (11) potentials, Eqs. (5) gives

𝐏\displaystyle\mathbf{P} =(k2xk2yk2cosϕ2k1y2k1cosϕ1,k1xk1yk1cosϕ1k2x2k2cosϕ2,0),\displaystyle=(\frac{k_{2x}k_{2y}}{k_{2}}\cos\phi_{2}-\frac{k_{1y}^{2}}{k_{1}}\cos\phi_{1},\frac{k_{1x}k_{1y}}{k_{1}}\cos\phi_{1}-\frac{k_{2x}^{2}}{k_{2}}\cos\phi_{2},0), (16a)
𝐌\displaystyle\mathbf{M} =(0,0,k2xcosϕ2k1ycosϕ1)and\displaystyle=(0,0,k_{2x}\cos\phi_{2}-k_{1y}\cos\phi_{1})\quad\textrm{and} (16b)
𝐌×𝐏=(k2xcosϕ2k1ycosϕ1)××(k1xk1yk1cosϕ1+k2x2k2cosϕ2,k2xk2yk2cosϕ2k1y2k1cosϕ1,0).\begin{split}\mathbf{M}\times\mathbf{P}&=(k_{2x}\cos\phi_{2}-k_{1y}\cos\phi_{1})\times\\ &\times(-\frac{k_{1x}k_{1y}}{k_{1}}\cos\phi_{1}+\frac{k_{2x}^{2}}{k_{2}}\cos\phi_{2},\frac{k_{2x}k_{2y}}{k_{2}}\cos\phi_{2}-\frac{k_{1y}^{2}}{k_{1}}\cos\phi_{1},0).\end{split} (16c)

Taking ϕ1=ϕ2=ϕ\phi_{1}=\phi_{2}=\phi gives the simple harmonic polarizations and flux

𝐏\displaystyle\mathbf{P} =cosϕ(k2xk2yk2k1y2k1,k1xk1yk1k2x2k2,0),\displaystyle=\cos\phi(\frac{k_{2x}k_{2y}}{k_{2}}-\frac{k_{1y}^{2}}{k_{1}},\frac{k_{1x}k_{1y}}{k_{1}}-\frac{k_{2x}^{2}}{k_{2}},0), (17a)
𝐌\displaystyle\mathbf{M} =cosϕ(0,0,k2xk1y)and\displaystyle=\cos\phi(0,0,k_{2x}-k_{1y})\quad\textrm{and} (17b)
𝐌×𝐏\displaystyle\mathbf{M}\times\mathbf{P} =(k2xk1y)cos2ϕ(k1xk1yk1+k2x2k2,k2xk2yk2k1y2k1,0)\displaystyle=(k_{2x}-k_{1y})\cos^{2}\phi(-\frac{k_{1x}k_{1y}}{k_{1}}+\frac{k_{2x}^{2}}{k_{2}},\frac{k_{2x}k_{2y}}{k_{2}}-\frac{k_{1y}^{2}}{k_{1}},0) (17c)

having bead-chain [21] flux squared magnitude

|𝐌×𝐏|2=(k2xk1y)2[k2x22k2xk1yk1k2(k2xk1x+k2yk1y)+k1y2]cos4ϕ.\left|\mathbf{M}\times\mathbf{P}\right|^{2}=(k_{2x}-k_{1y})^{2}[k_{2x}^{2}-2\frac{k_{2x}k_{1y}}{k_{1}k_{2}}(k_{2x}k_{1x}+k_{2y}k_{1y})+k_{1y}^{2}]\cos^{4}\phi. (18)

When 𝐤1=𝐤2=𝐤=(kx,ky,0)\mathbf{k}_{1}=\mathbf{k}_{2}=\mathbf{k}=(k_{x},k_{y},0), the polarizations further simplify to

k𝐏\displaystyle k\mathbf{P} =(kxky)cosϕ(ky,kx,0)and\displaystyle=(k_{x}-k_{y})\cos\phi(k_{y},-k_{x},0)\quad\textrm{and} (19a)
𝐌\displaystyle\mathbf{M} =cosϕ(0,0,kxky)\displaystyle=\cos\phi(0,0,k_{x}-k_{y}) (19b)

with the flux having direction 𝐤\mathbf{k} and magnitude

|𝐌×𝐏|=(kxky)2cos2ϕ.\left|\mathbf{M}\times\mathbf{P}\right|=(k_{x}-k_{y})^{2}\cos^{2}\phi. (20)

This flux is highly anisotropic with maximum values for kx=kyk_{x}=-k_{y} and null values for kx=kyk_{x}=k_{y}.

References and links

  • [1] Lorenz L. On the Identity of the Vibrations of Light with Electrical Currents. The London, Edinburgh and Dublin Philosophical Magazine and Journal of Science Series 4 1867; 34: 287-301.
  • [2] Potter HC. Lorenz on Light: A Precocious Photon Paradigm. November 2008: Available from: http://arXiv.org/abs/0811.2123
  • [3] Whittaker ET. A history of the theories of aether & electricity. Dover: New York; 1989.
  • [4] Marion JB. Classical Electromagnetic Radiation. Academic Press: New York; 1965.
  • [5] Keller O. On the theory of spatial localization of photons Phys. Rep. 2005; 𝟒𝟏𝟏\mathbf{411}: 1-232.
  • [6] Darwin CG. The Uncertainty Principle Science 1931; 𝟕𝟑\mathbf{73}: 653-660.
  • [7] Dimitrova TL, Weis A., The wave-particle duality of light: A demonstration experiment. Am. J. Phys. 2008; 𝟕𝟔\mathbf{76}: 137-42.
  • [8] Kaloyerou PN. The GRA beam-splitter experiments and particle-wave duality of light. J. Phys. A: Math. Gen. 2006; 𝟑𝟗\mathbf{39}: 11541-11566.
  • [9] Alonso MA. Focus Issue: Rays in Wave Theory. Opt. Express 2002; 𝟏𝟎\mathbf{10}: 715: Available from: http://www.opticsexpress.org/abstract.cfm?URI=OPEX-10-16-715
  • [10] Jackson JD, Okun LB. Historical roots of gauge invariance. Rev. Mod. Phys. 2001; 73: 663-680.
  • [11] Heras JA. How the potentials in different gauges yield the same retarded electric and magnetic fields. Am. J. Phys. 2007; 𝟕𝟓\mathbf{75}: 176-183.
  • [12] Monstein C, Wesley JP. Observation of scalar longitudinal electrodynamic waves. Europhys. Lett. 2002; 𝟓𝟗\mathbf{59}: 514-20.
  • [13] Tsontchev RI, Chubykalo AE, Rivera-Juarez JM. Coulomb Interaction Does Not Spread Instantaneously. Hadronic Journal 2000; 𝟐𝟑\mathbf{23}: 401-24.
  • [14] Tsontchev RI, Chubykalo AE, Rivera-Juarez JM. Addendum to ‘Coulomb Interaction Does Not Spread Instantaneously’. Hadronic Journal 2001; 𝟐𝟒\mathbf{24}: 253-61.
  • [15] Ignatiev GF, Leus VA. On a superluminal transmission at the phase velocities. In: Chubykalo AE, Pope V, Smirnov-Rueda R, Eds. Instantaneous Action at a Distance in Modern Physics: “Pro” and “Contra”, Nova Science, New York, 1999: pp. 203-7.
  • [16] Woodruff AE. The Contributions of Herman von Helmholtz to Electrodynamics. ISIS 1968; 𝟓𝟗\mathbf{59}: 300-11.
  • [17] Hertz H. Electric Waves. Jones DE, Trans. Dover: New York; 1962.
  • [18] Smirnov-Rueda R. Were Hertz’s ‘crucial’ experiments on propagation of electromagnetic interaction conclusive? In: Chubykalo AE, Pope V, Smirnov-Rueda R, Eds. Instantaneous Action at a Distance in Modern Physics: “Pro” and “Contra”, Nova Science, New York, 1999: pp. 57-73.
  • [19] Chi PJ, Russell CT. Phase skipping and Poynting flux of continuous pulsations. J. Geophys. Res. 1998; 𝟏𝟎𝟑\mathbf{103}: 29479-29491.
  • [20] Mandel L, Wolf E. Optical coherence and quantum optics. Cambridge U. Press: New York; 1995.
  • [21] Piekara AH. Self-trapping light waves and quanta: Towards an explanation of wave-photon duality. Opt. Laser Technol. 1982; 𝟏𝟒\mathbf{14}: 207-212.
  • [22] Hannay JH, Jeffrey MR. The electric field of synchrotron radiation. Proc. Roy. Soc. A 2005; 𝟒𝟔𝟏\mathbf{461}: 3599-3610.
  • [23] Bohn CL. Coherent Synchrotron Radiation: Theory and Experiments. AIP Conf. Proc. 2002; 𝟔𝟒𝟕\mathbf{647}: 81-95.
  • [24] Murnaghan FD. The Lines of Electric Force Due to a Moving Electron. Am. J. Math. 1917; 𝟑𝟗\mathbf{39}: 147-162.
  • [25] Elder FR, Gurewitsch AM, Langmuir RM, Pollock HC. Radiation from Electrons in a Synchrotron. Phys. Rev. 1947; 𝟕𝟏\mathbf{71}: 829-30.
  • [26] I thank P. A. Martin for directing me to the Murnaghan paper referenced above.