Gauging Potentials: Maxwell, Lorenz, Lorentz and Others on Linking the Electric Scalar and Vector Potentials

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Abstract

The development of tractable relationships for calculating the radiation produced by electric oscillators relied on a particular connection between the scalar potential, whose gradient is determined by charge density, and the vector potential, whose curl determines magnetic induction. Other such connections are permissible in electrodynamic field theory, including one used by Maxwell, but only one among them leads easily to radiation. Forms of electrodynamics other than Maxwell’s, including those by Kirchhoff, Helmholtz, Riemann and others, were not free to choose among such relationships, though none among these theories, with the limiting exception of Helmholtz’s, led to wavelike equations of propagation without assuming propagation a priori. One theory besides Maxwell’s that did was developed by the Danish physicist Lorenz. Although Lorenz derived the link between potentials later deployed for radiation in classical electrodynamics, his theory allowed no other choice. Three decades after Lorenz, the Dutch physicist Lorentz produced the first general understanding that the connection between the potentials can take various forms. Such a link was subsequently denominated a “gauge”, governed by the understanding that a particular choice, called a “gauge transformation”, must leave the measurable quantities of the theory unaltered. What follows traces the ways in which connections between the potentials were deployed in the nineteenth and early twentieth centuries.

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Notes

  1. 1.

    On Maxwell’s field understanding of charge see (Buchwald 1985, 23–34).

  2. 2.

    (Lorentz 1903b, 157). In earlier work Lorentz had instead imposed zero-divergence on the vector potential without discussion (Lorentz 1892, 14).

  3. 3.

    (Jackson and Okun 2001). See (Zangwill 2013) and (Thorne and Blandford 2017) for contemporary presentations of electrodynamics.

  4. 4.

    (Helmholtz 1858).

  5. 5.

    For a demonstration that causality holds in the Coulomb gauge see (Heras 2011) and (Jackson 2002). Both demonstrate that an unretarded term which appears in the Coulomb gauge expression for the vector potential exactly cancels the one in the scalar potential.

  6. 6.

    (Kirchhoff 1882a, 139) and (Kirchhoff 1882b, 159). On Weber see (Archibald 1989b). A modern account is (Assis 1994). See (Jackson and Okun 2001, 9–10) on Kirchhoff et al. Note that the difference in form between the Neumann and Kirchhoff potential functions vanishes for the interaction between closed circuits. The difference also vanishes if the divergence of the potential is zero.

  7. 7.

    Rk results either from Kirchhoff’s form Ak of the vector potential or from the Neumann form AN given the same continuity equation. These two potentials have the same curl.

  8. 8.

    (Kirchhoff 1882a, 140–41).

  9. 9.

    In 1856 Weber and Rudolf Kohlrausch (1809-1858) found the constant c to have the value 4.39 ∗ 108m/s, which implied that the current propagates in such wires at speed 3.1042 ∗ 108m/s, which was close to the extant value for the speed of light.

  10. 10.

    (Maxwell 1873), vol. 2, chap. 9.

  11. 11.

    (Maxwell 1873, sectns. 585-591). Maxwell’s electrokinetic momentum per unit area is ∇ × A, derived from his expression for the circuit’s contribution to the field momentum as ∮A · dl, where A is introduced directly as such. He then asserted that ∇ × A represents “what we are already acquainted with as the magnetic induction” because the variation of this momentum density through the area surrounded by a circuit results in a force, and on “Faraday’s theory, the phenomena of electromagnetic force and induction in a circuit depends on the variation of the number of lines of magnetic induction which pass through the circuit” (sectn. 592).

  12. 12.

    As noted by (Yaghjian 2014, 240).

  13. 13.

    (Maxwell 1873, secs. 783–784). Note that in the Treatise Maxwell’s expression for ∇2 has the opposite sign to the modern one “in order to make our expressions consistent with those in which Quaternions are employed” (sec. 616). I follow modern conventions.

  14. 14.

    (Maxwell 1873 sec. 783).

  15. 15.

    (Yaghjian 2014, 244) points out that since the addition of the gradient of any function of r,t to A leaves B unaltered, it’s possible to add to ψ the term \( \frac{\partial -\int \psi \left(r,{t}^{\prime}\right)d{t}^{\prime }+t\int \left(\rho /\left|\textbf{r}-{\textbf{r}}^{\prime}\right|\right){d}^3{r}^{\prime }}{\partial t} \). The time derivative of the redefined function’s Laplacian then vanishes identically, leaving \( \frac{\partial^2\nabla \cdot \textbf{A}}{\partial {\textrm{t}}^2}=0 \), and so the time derivative of ∇ · A must be independent of time. Consequently, either A itself is independent of time, or else its divergence vanishes. To see the difference between the result that Maxwell drew from zero divergence in comparison to the one later drawn for the Coulomb gauge, it suffices to compare their respective expressions for the vector potential. Maxwell’s reduces to the first term in J, including the displacement current. The Coulomb gauge expression eschews the displacement current but involves the curl of an integral that depends upon the retarded current, itself integrated through the time it takes emission to reach the observation point: see (Jackson 2002), 3.17.

  16. 16.

    Maxwell demonstrates transversality for the vector potential independently of the value of its divergence by combining his equations for E and B in terms of A (Maxwell 1873, vols. 2, sectn. 790).

  17. 17.

    See (Buchwald 1985, 269–76). Oliver Heaviside avoided the use of either the scalar or vector potentials, but he never analyzed the origin of radiation.

  18. 18.

    (Hunt 1991, 117–18).

  19. 19.

    (Buchwald 1993).

  20. 20.

    For a derivation of the Helmholtz condition Rh see (Buchwald 1985, 314).

  21. 21.

    For a succinct demonstration that the Helmholtz system produces the same equations as Maxwell’s if the polarization is infinite see (Darrigol 2000, 417–19). In the limit of infinite polarizability the constant k drops out of consideration.

  22. 22.

    On Lorenz see (Kragh 2018).

  23. 23.

    (Lorenz 1867b), translated as (Lorenz 1867a). On Lorenz see (Kragh 2018).

  24. 24.

    Lorenz used just r to denote |r − r| while integrating over dxdydz.

  25. 25.

    (Lorenz 1867a, 293). Lorenz did not complicate matters by allowing the charge or current sources to move, so that the distances r − r are not themselves dependent on time.

  26. 26.

    Lorenz’s coordinates for the observation point are x,y,z and for the current locus x’,y’,z’, while his expression for the divergence in Rlnz is taken with respect to x,y,z.

  27. 27.

    The speed of propagation would then be 3.1 ∗ 108m/s given Weber’s and Kohlrausch’s value for c. Lorenz remained uncommitted about just what occupied space in order to have “currents”, remarking that “there is scarcely any reason for adhering to the hypothesis of an aether; for it may well be assumed that in the so-called vacuum there is sufficient matter to form an adequate substratum for motion” (Lorenz 1867a, 301).

  28. 28.

    (Heras 2007, 656) provides the correct expression for the divergence under retardation. He notes that operating on functions of r, tcan be misleading because they depend explicitly on source coordinates through r and implicitly through t = t − |r − r|/a.

  29. 29.

    (Heras 2007) demonstrates that starting from a continuity equation (absent the factor ½) between otherwise-unspecified functions ρfml,Cfml, it is possible to define retarded scalar and vector fields that satisfy equations formally similar to the Maxwell four of classical electrodynamics provided that the requisite care is taken in develo** identities with retarded functions.

  30. 30.

    Neumann followed Bernhard Riemann (1826-1866), who had “[in a posthumous publication] presented a (faulty) derivation of the Weber law by assuming a conservative electrodynamics force, and by positing that the potential associated with this force was propagated with constant velocity” (Archibald 1989a, 787). Neumann’s calculation took the distance to be used in computing the potential when it is received at a given point as the distance at that time between the point and a moving emitter, rather than the distance traveled between the two from emission to reception, which was the essence of Clausius’ critique (ibid., 789).

  31. 31.

    (Maxwell 1890a).

  32. 32.

    (Maxwell 1890b, 137–38).

  33. 33.

    (Hertz 1884).

  34. 34.

    (Wiechert 1900).

  35. 35.

    (Wiechert 1900, 557–59).

  36. 36.

    (Lorentz 1903a, b).

  37. 37.

    (Jackson and Okun 2001).

  38. 38.

    On Marconi and Fleming see (Hong 2001). The early development of radio wave transmission is analyzed in (Yeang 2013). For an example of the manner in which the radiation gauge has been used by engineering physicists see, e.g., (Skilling 1942).

  39. 39.

    On Noether see (Rowe 2021).

  40. 40.

    (Wheeler and Feynman 1949). (Lazarovici 2018) argues for the irremediable inconsistency of an electrodynamics grounded on fields.

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Acknowledgments

I thank, Karine Chemla, Anne Kox, Andrew Zangwill, and two anonymous reviewers for their suggestions on drafts of this piece.

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Buchwald, J.Z. (2023). Gauging Potentials: Maxwell, Lorenz, Lorentz and Others on Linking the Electric Scalar and Vector Potentials. In: Chemla, K., Ferreirós, J., Ji, L., Scholz, E., Wang, C. (eds) The Richness of the History of Mathematics. Archimedes, vol 66. Springer, Cham. https://doi.org/10.1007/978-3-031-40855-7_14

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