Lesson 18 Electromagnetic Fields in Matter

Lesson 17 assembled the electromagnetic field in vacuum, with the field strength as a 2-form, the potential as a 1-form, the Lorentz force, the Maxwell equations, the stress-energy tensor, and the variational principle that ties them together. All of that structure lives on Minkowski spacetime and is indifferent to the presence of ordinary matter. Real materials, however, are composed of charges that can be displaced, of currents that can be induced, and of dipoles that can be aligned. The field that acts on a test charge inside such a material is not the microscopic field of the vacuum theory; it is an average field whose sources have been reorganized into polarization and magnetization. The present lesson examines how that reorganization is performed, how the resulting macroscopic fields transform, and how the conservation laws of Lesson 15 survive the averaging.

We begin by recalling the action of the Lorentz group on vectors and tensors. Because every material response must be consistent with special relativity, the transformation properties of the polarization, the magnetization, and the susceptibility tensors are fixed once the vacuum field strength is known. Noether’s theorem, already applied to time translation and to spatial translation, is now applied to Lorentz transformations themselves; the associated conserved charges are the components of the angular-momentum tensor. That tensor is not symmetric. The electromagnetic stress-energy tensor constructed in Lesson 17 is likewise not symmetric. Both defects are removed by the same improvement term, and the improved tensors become the sources of angular momentum carried by the field and by polarized matter.

With the transformation law in hand we turn to the average fields inside matter. The microscopic current is expanded in multipoles about each molecule. The monopole term reproduces the free charge and free current already present in vacuum electrodynamics. The dipole term produces the polarization l18_1.png and the magnetization l18_2.png. Higher multipoles are neglected in the long-wavelength approximation that defines macroscopic electrodynamics. The average field equations then take the familiar form in which l18_3.png and l18_4.png appear as the fields whose divergences and curls are sourced only by the free charges and free currents. The linear response of an isotropic medium is summarized by the electric and magnetic susceptibility matrices; their transformation properties under boosts follow at once from the tensor character of l18_5.png.

Throughout, the geometric language remains that of Lesson 15: configuration space, phase space, Noether charges, and the symplectic structure that guarantees conservation. The new element is the systematic replacement of microscopic sources by their macroscopic averages, performed so that every equation stays covariant and every conserved quantity retains its interpretation as a flux through a three-surface. The result is a complete spacetime account of electromagnetic fields in matter.

Lorentz Transformations

A finite Lorentz transformation acts on the coordinates by a constant matrix Λ,

l18_6.png

(18.1)

that preserves the Minkowski metric,

l18_7.png

(18.2)

In matrix language the same condition reads l18_8.png. Every such matrix that can be reached continuously from the identity may be written as the exponential of a generator A,

l18_9.png

(18.3)

Substitution into the defining relation then shows that the generator itself must be antisymmetric with respect to the metric,

l18_10.png

(18.4)

(The six independent components of an antisymmetric 4 × 4 matrix are precisely the three rotations and the three boosts.)

Because the exponential is the limit of repeated infinitesimal steps,

l18_11.png

(18.5)

it is enough to study the generators. A convenient basis is furnished by the six matrices l18_12.png whose only non-zero entries lie in the αβ and βα positions and satisfy

l18_13.png

(18.6)

Any infinitesimal Lorentz transformation is then a linear combination of these six matrices, and any finite transformation in the connected component of the Lorentz group is the exponential of such a combination.

l18_14.gif

Figure 18.1: The six independent generators of the Lorentz algebra. The three boost generators occupy the time-space slots; the three rotation generators occupy the space-space slots.

The same generators reappear when the action of a Lorentz transformation on tensors is computed. Because every index is transformed by Λ or by l18_15.png, the infinitesimal change of a tensor is obtained by letting each generator act on one index at a time. The resulting formula will be needed both for the transformation law of the electromagnetic field strength and for the Noether charge associated with Lorentz symmetry. Once the generators are in hand, the passage from infinitesimal to finite transformations is purely algebraic, we exponentiate the appropriate linear combination of the l18_16.png. That completes the kinematic preparation required for the dynamical application of Noether’s theorem to Lorentz transformations.

Transforming Vectors and Tensors

A finite Lorentz transformation belonging to the connected component of the Lorentz group is obtained by exponentiating a linear combination of the six generators introduced in the previous subsection,

l18_17.png

(18.7)

where the coefficients l18_18.png are antisymmetric, l18_19.png. Specifying the six independent numbers l18_20.png completely determines the transformation. Three of them parametrize boosts; the other three parametrize rotations.

A contravariant vector transforms by the matrix Λ itself,

l18_21.png

(18.8)

Because each index of a tensor transforms independently, the action on a rank-2 tensor is the tensor product of two copies of Λ. It is convenient to package that action into a single generator acting on the pair of indices. Define

l18_22.png

(18.9)

Then

l18_23.png

(18.10)

The same construction extends immediately to tensors of any rank, where each index contributes one factor of the fundamental generator l18_24.png, and the exponential of the sum generates the finite transformation.

l18_25.gif

Figure 18.2: Action of a Lorentz transformation. A contravariant vector is multiplied by Λ; a rank-2 tensor is transformed by the tensor product of two copies of Λ. Boost generators appear in blue, rotation generators in green.

The infinitesimal form is often the most useful for calculations. Expanding the exponential to first order shows that the change in a vector is

l18_26.png

(18.11)

while the change in a tensor is the sum of the generator acting on each index separately. These variations are exactly the ones that enter the Noether procedure when the symmetry under consideration is a Lorentz transformation. Once the finite transformation law and its infinitesimal generator are both in hand, the construction of the associated conserved charges can proceed exactly as it did for translations.

Lorentz Invariance

A Lorentz transformation acts simultaneously on the coordinates and on the components of any field that lives on spacetime. If the coordinates transform by

l18_27.png

(18.12)

then a field l18_28.png with several components transforms by the corresponding representation of the same generators,

l18_29.png

(18.13)

The matrices l18_30.png are block-diagonal. Consequently the only non-vanishing entries of l18_31.png connect components that belong to one and the same irreducible multiplet—scalar, vector, or tensor. Components belonging to different fields do not mix under a Lorentz transformation.

This block-diagonal structure is the precise statement of Lorentz invariance for a multi-component field, where each irreducible piece transforms into itself, and the Lagrangian density, being a scalar, is unchanged when every field is replaced by its transformed counterpart and the coordinates are simultaneously transformed. The same property guarantees that the Euler–Lagrange equations retain their form in every inertial frame.

l18_32.gif

Figure 18.3: Block-diagonal action of a Lorentz transformation. A scalar, a vector, and a tensor each transform among their own components; components belonging to different fields do not mix.

Because the generators never mix distinct irreducible representations, the classification of fields by their Lorentz transformation properties is unambiguous. A scalar field has a single component and M'=0; a vector field transforms with the fundamental generators l18_33.png; a rank-2 tensor transforms with the tensor-product generators constructed in the previous subsection. These transformation laws will be used both to verify the covariance of the Maxwell equations and to construct the Noether charges associated with Lorentz symmetry.

Applying Noether’s Theorem to Lorentz Transformations

When the Lagrangian density is a Lorentz scalar, Noether’s theorem supplies one conserved current for each independent parameter of a Lorentz transformation. Because those parameters are the six independent components of the antisymmetric matrix l18_34.png, there exist six conserved currents l18_35.png, themselves antisymmetric in the pair αβ,

l18_36.png

(18.14)

Their divergences vanish on shell, and the associated charges are the components of the angular-momentum tensor.

The general Noether formula for a current associated with an infinitesimal variation generated by a parameter ε reads

l18_37.png

(18.15)

For a pure Lorentz transformation we set l18_38.png (and all other parameters to zero). The coordinate variation and the field variation are then given by the corresponding generators,

l18_39.png

(18.16)

and

l18_40.png

(18.17)

Substitution yields the explicit current

l18_41.gif

(18.18)

The terms that multiply the coordinates l18_42.png and l18_43.png are precisely the components of the canonical stress-energy tensor l18_44.png already obtained from translational invariance. The remaining term is the spin contribution arising from the transformation of the field components themselves. Consequently the conserved current may be written compactly as

l18_45.png

(18.19)

l18_46.gif

Figure 18.4: The Lorentz Noether current. The orbital contribution (blue) is built from the canonical stress-energy tensor; the spin contribution (green) arises from the action of the generators on the field components. Their sum is divergenceless on shell.

The six currents l18_47.png are the relativistic generalization of angular-momentum density. Their spatial integrals yield the total angular momentum of the system, including both the orbital part associated with the motion of the energy-momentum distribution and the intrinsic spin carried by the fields. Because the canonical stress-energy tensor is not symmetric, the orbital piece alone is not conserved; the spin piece is required to cancel the antisymmetric part of l18_48.png and to restore conservation. The same cancellation will reappear when the electromagnetic stress-energy tensor is improved by the Belinfante procedure, confirming that the Noether charge obtained here is identical to the angular momentum constructed from the symmetrized tensor.

Scalar Fields

For a theory containing only scalar fields the spin generators l18_49.png vanish identically. The Lorentz Noether current therefore reduces to its orbital part,

l18_50.png

(18.20)

where l18_51.png is the canonical stress-energy tensor already obtained from translational invariance.

Consider first the spatial component l18_52.png. The corresponding finite transformation is a rotation about the l18_53.png-axis,

l18_54.png

(18.21)

Invariance of the action under this rotation implies conservation of l18_55.png. Its charge density is

l18_56.png

(18.22)

Recognizing l18_57.png as the momentum density, one sees that the spatial integral of l18_58.png is precisely the third component of l18_59.png. Defining the three-vector

l18_60.png

(18.23)

then yields the familiar expression

l18_61.png

(18.24)

Conservation of the projection l18_62.png follows from invariance under rotations about the axis l18_63.png.

The mixed components l18_64.png arise from boosts. For a boost in the l18_65.png-direction one has

l18_66.png

(18.25)

The associated charge is

l18_67.png

(18.26)

The integral of l18_68.png is the total momentum l18_69.png and the integral of l18_70.png is the total energy E. Writing l18_71.png for the center-of-energy coordinate then gives

l18_72.png

(18.27)

Differentiating with respect to time produces

l18_73.png

(18.28)

The velocity of the center of energy is the constant l18_74.png, so the derivative vanishes and l18_75.png is conserved.

Finally, the divergence of the current itself implies a symmetry property of the stress-energy tensor. On shell one has

l18_76.png

(18.29)

[Explain on shell]

l18_77.gif

Figure 18.5: Conserved charges for scalar fields. Rotations (blue) produce the orbital angular momentum l18_78.png; boosts (green) produce the center-of-energy relation -t P+E X.

Thus, for a theory of scalar fields, conservation of angular momentum forces the stress-energy tensor to be symmetric. For fields that carry intrinsic spin the same argument no longer holds; an additional spin term appears in the current and the canonical tensor need not be symmetric. That case is examined next.

Vector and Tensor Fields

For theories that contain vector or tensor fields the Lorentz generators l18_79.png no longer vanish. The Noether current associated with a Lorentz transformation therefore acquires an additional piece,

l18_80.png

(18.30)

where the spin current is

l18_81.png

(18.31)

The first two terms continue to represent the orbital angular momentum carried by the momentum density of the fields. The new term l18_82.png is the intrinsic angular momentum, or spin, that resides in the tensorial character of the fields themselves.

Because the generators l18_83.png act on the field indices, the spin current is nonzero whenever the fields transform nontrivially under the Lorentz group. For a vector field the generators are the fundamental matrices l18_84.png; for a rank-2 tensor they are the tensor-product generators constructed earlier. In either case the spin contribution is local—it depends on the field values and their first derivatives at a single point—and does not involve the coordinate factors l18_85.png that appear in the orbital piece.

Conservation of the total current l18_86.png still holds on shell. The orbital piece alone, however, is no longer divergenceless, because the canonical stress-energy tensor of a spinning field is not symmetric. The divergence of the orbital contribution is precisely cancelled by the divergence of the spin current, so that only their sum is conserved. This cancellation is the relativistic statement that the total angular momentum—orbital plus spin—is the quantity protected by Lorentz invariance.

l18_87.gif

Figure 18.6: Angular momentum for fields with spin. The orbital contribution (blue) is built from the canonical stress-energy tensor; the spin contribution (green) arises from the Lorentz generators acting on the field indices. Only their sum is divergenceless.

The same decomposition will reappear when the electromagnetic field is examined. The photon carries spin 1, and the spin current constructed from the field strength supplies the term needed to symmetrize the Maxwell stress-energy tensor. The pattern established here—orbital piece from the coordinates, spin piece from the generators—therefore governs every relativistic field theory.

Electrodynamics

The general decomposition of angular momentum into orbital and spin pieces becomes concrete once it is applied to the electromagnetic field. The question is whether the field itself carries intrinsic angular momentum. To answer it one begins with the Lagrangian that couples the electromagnetic potential to charged matter,

l18_88.png

(18.32)

The matter fields l18_89.png are scalars under Lorentz transformations, while the potential l18_90.png transforms as a vector. Consequently the only non-vanishing generators in the spin current are those that act on the vector index of l18_91.png.

The finite transformation that mixes the components may be written

l18_92.png

(18.33)

where the generators are block-diagonal,

l18_93.png

(18.34)

Substitution into the general expression for the spin current then yields

l18_94.png

(18.35)

The spatial components of this current define a spin density

l18_95.png

(18.36)

In terms of the electric field and the vector potential one finds the compact relation

l18_96.png

(18.37)

To see that the spin density is nonzero for a realistic field configuration, consider a circularly polarized plane wave propagating in the l18_97.png-direction. A suitable potential is

l18_98.png

(18.38)

The upper (lower) sign corresponds to right (left) circular polarization. The associated electric field is simply

l18_99.png

(18.39)

and the spin density reduces to

l18_100.png

(18.40)

Thus a circularly polarized electromagnetic wave carries a nonzero spin angular momentum density directed along its direction of propagation. The magnitude is proportional to the energy density of the wave, and the sign is fixed by the sense of polarization. This is the concrete realization, within classical electrodynamics, of the spin term that appears in the general Noether current for Lorentz transformations.

l18_101.gif

Figure 18.7: Spin density of a circularly polarized wave. The rotating electric field (blue) produces a spin density l18_102.png (green) aligned with the direction of propagation; the sign reverses with the sense of polarization.

The same spin current that yields l18_103.png is precisely the term required to cancel the antisymmetric part of the canonical electromagnetic stress-energy tensor. Once that cancellation is performed, the improved tensor becomes symmetric and the total angular momentum—orbital plus spin—is conserved. In this way the abstract decomposition introduced for general vector fields acquires a direct physical interpretation inside Maxwell theory.

The Electric Field in Matter

Charged matter produces an electromagnetic field and, when accelerated, radiates. When the same matter is placed in an external field it experiences forces; if the material has internal structure, those forces act between its constituent parts as well. In the present treatment irreversible currents inside the matter are set aside; only the reversible response associated with bound charge is retained.

In the local rest frame of a material element the charge density is the product of the charge per atom l18_104.png and the number density of atoms. The four-current of charge is therefore

l18_105.png

(18.41)

where l18_106.png is the particle-number current already introduced for the material. Because the charge is bound to the atoms, the spatial components of l18_107.png vanish in the local rest frame. The relation is covariant, so it holds in every frame. Conservation of particle number together with the fact that the material coordinates are constant along the flow then imply

l18_108.png

(18.42)

In the absence of interaction the total Lagrangian would be the sum of a pure-matter piece and a pure-field piece,

l18_109.png

(18.43)

with

l18_110.png

(18.44)

and

l18_111.png

(18.45)

with the coupling introduced by the interaction term

l18_112.png

(18.46)

Variation with respect to the potential immediately yields the inhomogeneous Maxwell equation

l18_113.png

(18.47)

and this is the form required once the charge current of the material is taken as the source.

The stress-energy tensor likewise splits into three contributions,

l18_114.png

(18.48)

The matter piece is the one already obtained for a continuous medium,

l18_115.png

(18.49)

The electromagnetic piece is the canonical tensor constructed from the field strength,

l18_116.png

(18.50)

while the interaction piece is

l18_117.png

(18.51)

Four-momentum balance for the material then reads

l18_118.png

(18.52)

The right-hand side is precisely the Lorentz force density exerted by the field on the charges bound in the matter. Thus the same variational principle that produces Maxwell’s equations also produces the force law that governs the motion of the charged continuum.

l18_119.gif

Figure 18.8: Charged continuum in an external field. The bound four-current l18_120.png (blue) sources the field; the field exerts the Lorentz force density l18_121.png (red) that appears on the right-hand side of the material momentum balance.

The construction just given still treats the microscopic charges as structureless. When the charges inside each molecule are allowed to separate under the influence of the local field, polarization appears and the macroscopic Maxwell equations acquire the familiar form involving l18_122.png and l18_123.png. That refinement is the subject of the following subsections.

Symmetrizing the Stress-Energy Tensor

Whenever a field theory possesses a nonzero spin current l18_124.png, the canonical stress-energy tensor l18_125.png fails to be symmetric. The asymmetry is not an obstacle to the conservation of four-momentum, but it is inconvenient for the electromagnetic canonical tensor, for example, is not gauge-invariant. A symmetric improvement l18_126.png can be constructed that yields the same total four-momentum, is divergenceless on shell, and, in the electromagnetic case, is gauge-invariant.

The spin current is antisymmetric in its first pair of indices. From it one builds an auxiliary tensor that is antisymmetric in its last pair,

l18_127.png

(18.53)

The improved stress-energy tensor is then defined by

l18_128.png

(18.54)

Because l18_129.png is antisymmetric in νλ, the divergence of the added term vanishes identically,

l18_130.png

(18.55)

Thus l18_131.png is conserved whenever l18_132.png is conserved.

The two tensors also give the same total four-momentum. Integrating the difference over a spacelike slice and using the antisymmetry of G produces only surface terms that vanish at infinity,

l18_133.png

(18.56)

Hence the integrated charges coincide.

It remains only to verify symmetry. A short calculation that again employs the conservation of the angular-momentum current yields

l18_134.png

(18.57)

The right-hand side is precisely the divergence of l18_135.png, and that vanishes on the shell. What does, :on the shell” mean? It means that the system is governed by a classical equation of motion. Therefore

l18_136.png

(18.58)

The improved tensor is symmetric, conserved, and equivalent to the canonical tensor for all global charges. In electrodynamics it is, in addition, gauge-invariant, removing the last practical defect of the canonical expression.

l18_137.gif

Figure 18.9: Belinfante symmetrization. The canonical tensor l18_138.png (blue) is improved by the divergence of l18_139.png constructed from the spin current (green). The result l18_140.png is symmetric, conserved, and yields the same total four-momentum.

The same improvement will be applied to the electromagnetic field in a later subsection, where the explicit form of l18_141.png reduces to the familiar Maxwell stress-energy tensor written entirely in terms of l18_142.png.

More About Angular Momentum

Once a symmetric, conserved stress-energy tensor l18_143.png is available, an angular-momentum current can be written that contains only an orbital piece,

l18_144.png

(18.59)

No explicit spin term appears. Because l18_145.png is both symmetric and divergenceless, the current l18_146.png is itself conserved. Its spatial integral therefore supplies a conserved angular-momentum charge built solely from the improved tensor.

To see that this charge coincides with the one obtained from the original Noether current, substitute the definition of Θ,

l18_147.gif

(18.60)

The combination of G terms that is free of derivatives is precisely the spin current,

l18_148.png

(18.61)

Hence

l18_149.png

(18.62)

When the difference is integrated over a spacelike slice, the divergence term becomes a pure surface integral. Antisymmetry of G in its last pair of indices forces that surface integral to vanish, so

l18_150.png

(18.63)

The two currents therefore generate identical total angular momenta. One may use l18_151.png in place of the original Noether current whenever only the integrated charges are required. The advantage is that every contribution is now expressed through the single symmetric tensor l18_152.png

l18_153.gif

Figure 18.10: Equivalence of angular-momentum currents. The original Noether current l18_154.png (blue) contains both orbital and spin contributions; the improved current l18_155.png (green) is built solely from the symmetric tensor l18_156.png. Their spatial integrals coincide.

The same construction will be applied to the electromagnetic field, where l18_157.png reduces to the familiar Maxwell tensor written entirely in terms of l18_158.png. The resulting angular-momentum density then automatically includes the spin carried by the field.

The Symmetrized Electromagnetic Stress-Energy Tensor

The general Belinfante procedure is now applied to the coupled system of charged matter and the electromagnetic field. The Lagrangian is the one already introduced,

l18_159.png

The associated spin current is

l18_160.png

(18.64)

From it one constructs the improvement tensor

l18_161.png

(18.65)

Adding the divergence of G to the canonical stress-energy tensor produces the improved tensor

l18_162.png

(18.66)

The field equations set the last parenthesis to zero, so the interaction term drops out. The improved tensor therefore splits cleanly into a matter piece and a pure-field piece,

l18_163.png

(18.67)

where

l18_164.png

(18.68)

and

l18_165.png

(18.69)

The electromagnetic contribution is symmetric by inspection and is built solely from the gauge-invariant field strength; it is therefore itself gauge-invariant.

In an inertial frame the components of l18_166.png recover the familiar expressions. The energy density is

l18_167.png

(18.70)

The mixed components are the Poynting flux,

l18_168.png

(18.71)

while the spatial block is the Maxwell stress tensor,

l18_169.png

(18.72)

Four-momentum balance between the two subsystems now reads

l18_170.png

(18.73)

The Lorentz force density appears as the rate at which four-momentum is transferred from the field to the matter; no residual interaction term remains in the stress-energy tensor itself.

l18_171.gif

Figure 18.11: The symmetrized electromagnetic stress-energy tensor. All components are written in terms of the gauge-invariant field strength l18_172.png: energy density (blue), Poynting flux (green), and Maxwell stresses (red).

Because l18_173.png is both symmetric and conserved (when the matter current vanishes), the angular-momentum current constructed from it in the previous subsection automatically includes the spin carried by the field. The canonical tensor, the spin current, and the Belinfante improvement have thereby been reduced to a single, gauge-invariant object that governs the energy, momentum, and angular momentum of the electromagnetic field.

Angular Momentum in Electromagnetic Fields

With the symmetrized electromagnetic stress-energy tensor l18_174.png in hand, the angular-momentum current is given entirely by the orbital expression constructed in the preceding subsection,

l18_175.png

(18.74)

No separate spin term need be written; the spin carried by the field is already incorporated through the improvement that produced l18_176.png.

Consider a left-circularly polarized plane wave propagating in the l18_177.png-direction. The spin density obtained earlier from the canonical current is

l18_178.png

(18.75)

[Explain this a bit better]

so the wave carries a nonzero intrinsic angular momentum density parallel to its direction of propagation. When the same configuration is examined with the improved current one finds

l18_179.png

(18.76)

The vanishing is immediate once the momentum density is inspected where l18_180.png is proportional to l18_181.pngand therefore points strictly along l18_182.png. The vector product with the transverse coordinates l18_183.png and l18_184.png is identically zero. The orbital contribution measured by l18_185.png therefore vanishes, while the total angular momentum of the wave remains equal to the spin obtained from the original Noether current. The two descriptions differ only by a spatial divergence; their integrated charges coincide.

The same pattern holds for any free electromagnetic field. The improved tensor l18_186.png automatically accounts for both the orbital motion of the energy-momentum distribution and the intrinsic spin associated with the polarization. Consequently the single current l18_187.png furnishes a complete, gauge-invariant account of the angular momentum carried by the field.

l18_188.gif

Figure 18.12: Angular momentum of a circularly polarized wave. The Poynting vector (green) lies along the propagation direction, so the orbital contribution built from l18_189.png vanishes; the total angular momentum is pure spin.

The construction just completed shows that every conserved quantity associated with the Poincaré group—energy, momentum, and angular momentum—can be expressed through the single symmetric, gauge-invariant tensor l18_190.png. The same tensor will serve as the source of the gravitational field once the Einstein equations are introduced.

Polarized Materials

Many of the distinctive electromagnetic properties of bulk matter arise from the partial alignment of the electric and magnetic dipole moments of its constituent volume elements. That alignment is called polarization. The present section develops the continuum description of polarized media; the same framework will later be applied to plasmas.

The starting point is a dipole-moment tensor constructed directly from the microscopic currents that circulate inside each material element. Once that tensor is in hand, the microscopic Maxwell equations can be averaged to produce a closed set of macroscopic field equations. The averaging replaces the rapidly varying microscopic sources by a polarization and a magnetization; the macroscopic fields then satisfy equations whose sources are only the free charges and free currents. The same averaging procedure yields a macroscopic Lagrangian whose Euler–Lagrange equations are precisely the macroscopic Maxwell system.

l18_191.gif

Figure 18.13: Polarization of a material. Microscopic dipoles that are randomly oriented (blue) produce no net moment; partial alignment (green) yields a macroscopic polarization l18_192.png.

The construction that follows therefore accomplishes three things at once: it supplies the dipole-moment tensor in terms of the underlying currents, it produces the macroscopic Maxwell equations that govern the averaged fields, and it furnishes the Lagrangian from which those equations are derived. With those elements in place the response of polarized matter—and later of plasmas—can be examined within the same geometric framework already used for the vacuum field.

The Average Electromagnetic Field in Matter

Until now the electromagnetic field inside a material has been treated as though it varied smoothly on every scale. A classical atomic model shows that this cannot be literally true, where the microscopic field l18_193.png can fluctuate violently on atomic distances. The macroscopic field that appears in the continuum theory is therefore defined as a local average of the microscopic field about an observation event l18_194.png,

l18_195.png

(18.77)

The weighting function Δ is appreciable only inside a spacetime region whose spatial radius Λ is large compared with atomic dimensions yet small compared with any macroscopic length of interest, and whose temporal width Λ’ is long compared with atomic periods yet short compared with macroscopic times. Typical values are l18_196.png m and l18_197.png sec. An explicit normalized choice is the Gaussian

l18_198.png

(18.78)

which satisfies

l18_199.png

(18.79)

So long as every macroscopic length greatly exceeds atomic lengths, the precise values of Λ, Λ’ and the detailed shape of Δ drop out of the averaged field. To see why, consider the Fourier transform of a microscopic electric field,

l18_200.png

(18.80)

The macroscopic field is the convolution

l18_201.png

(18.81)

whose transform is simply

l18_202.png

(18.82)

The Fourier transform of the averaging kernel is itself a Gaussian that equals unity for all wave-numbers small compared with 1/Λ and falls to zero for wave-numbers large compared with 1/Λ. Consequently every Fourier component that varies on macroscopic scales is transmitted unchanged, while the atomic-scale fluctuations are suppressed. The macroscopic field defined by the average is therefore independent of the precise choice of averaging parameters once those parameters lie in the intermediate range described above.

l18_203.gif

Figure 18.14: Spatial averaging. The microscopic field (red) fluctuates on atomic scales; convolution with the kernel Δ of width Λ produces the smooth macroscopic field (blue)..

The same averaging may be applied to every component of the field strength and to the microscopic current. The resulting macroscopic quantities satisfy a closed set of equations whose sources are only the free charges and the polarization and magnetization of the medium. Those equations, and the Lagrangian from which they follow, are constructed in the following subsections.

The Multipole Expansion of the Average Current

The macroscopic field is the average of the microscopic field; the same averaging applied to the microscopic current produces the macroscopic source. Because the microscopic Maxwell equation identifies the source with the divergence of the field strength, the averaged current

l18_204.png

(18.83)

is precisely the source that appears on the right-hand side of the macroscopic inhomogeneous equation.

The material is regarded as a collection of N small elements. The microscopic current is the sum of the contributions of each element,

l18_205.png

(18.84)

A representative world-line l18_206.png is assigned to the nth element, with the time component chosen so that l18_207.png. Each element is spatially localized where l18_208.png vanishes outside a region of diameter l18_209.png m about l18_210.png. Since d≪Λ, the weighting function may be expanded about the representative point,

l18_211.png

(18.85)

Each successive term is smaller than the preceding one by a factor of order d/Λ.

Charge conservation supplies two integral identities that allow the expansion to be rearranged. After those identities are used, the macroscopic current takes the form

l18_212.png

(18.86)

The first term is the free current carried by the motion of the elements themselves,

l18_213.png

(18.87)

The second term is the divergence of the dipole-moment tensor

l18_214.png

(18.88)

These are the first two terms in the multipole expansion of the averaged current. The monopole piece describes the free charges and currents; the dipole piece describes the polarization and magnetization of the material. Higher multipoles are suppressed by additional powers of d/Λ and may be neglected for ordinary macroscopic applications.

l18_215.gif

Figure 18.15: Multipole expansion. Each material element (size d≪Λ contributes a free current along its world-line (blue) and a dipole moment arising from internal currents (red). The macroscopic source is the free current plus the divergence of the dipole tensor l18_216.png.

The dipole tensor l18_217.png will be decomposed into its electric and magnetic parts in the following subsections; those parts become the polarization and magnetization that enter the macroscopic Maxwell equations.

Monopole Terms

The free part of the macroscopic current admits a simple interpretation once the spatial integral of the charge density of each element is performed. That integral is the total charge l18_218.png carried by the nth element, so

l18_219.png

(18.89)

The combination l18_220.png, is precisely the infinitesimal displacement l18_221.png along the world-line of the element. The expression therefore collapses to a sum of line integrals,

l18_222.png

(18.90)

Each term is the contribution of a point charge l18_223.png that travels along the representative world-line l18_224.png. In other words, the monopole piece of the averaged current is exactly the current that would be produced by a collection of structureless charged particles located at the centers of the material elements.

l18_225.gif

Figure 18.16: Monopole current. Each material element contributes as a point charge l18_226.png moving along its representative world-line; the macroscopic free current is the sum of these contributions, smoothed by the averaging kernel.

Higher multipoles arise only from the internal structure of the elements and are deferred to the next subsection. For many purposes the monopole term alone already supplies the free charge and free current that appear as sources in the macroscopic Maxwell equations.

The Dipole Term

The dipole contribution to the macroscopic current is completely determined by the antisymmetric tensor

l18_227.png

(18.91)

where the dipole moment of the nth element is

l18_228.png

(18.92)

In the instantaneous rest frame of the element, where l18_229.png, the components simplify. The mixed components become the electric dipole moment,

l18_230.png

(18.93)

while the purely spatial components become the magnetic moment,

l18_231.png

(18.94)

Thus the single relativistic tensor l18_232.png unifies the electric polarization and the magnetization of each material element. When these microscopic moments are smoothed by the averaging kernel they produce the macroscopic polarization and magnetization that source the macroscopic Maxwell equations.

l18_233.gif

Figure 18.17: Dipole moments of a material element. In the rest frame the mixed components l18_234.png are the electric dipole (blue) and the spatial components l18_235.png are the magnetic moment (green).

The same tensor will be decomposed into its irreducible pieces under the rotation group in the next subsection, making the identification with the conventional polarization l18_236.png and magnetization l18_237.png completely explicit.

Frame Dependence

The dipole tensor written in the preceding subsection refers to a preferred frame in which the time axis is fixed by a one-form l18_238.png. The question is whether that choice affects the tensor itself.

A world-line may be parametrized by any monotonic parameter l18_239.png. The map l18_240.png is independent of l18_241.png. When the four-velocity is written with respect to this parameter, l18_242.png plays the role of a proper-time coordinate that is constant on the planes of constant l18_243.png. The level-set condition

l18_244.png

(18.95)

then determines the parameter, and the chain rule supplies the identity

l18_245.png

(18.96)

Substitution of this identity into the definition of l18_246.png produces an expression that still appears to depend on l18_247.png.

An infinitesimal change l18_248.png induces a variation l18_249.png of the parameter. After the resulting variation of l18_250.png is integrated by parts, every term that survives is proportional to a derivative of the averaging kernel. Because that kernel varies only on the scale Λ, while the support of each microscopic current is of size d, the variation satisfies

l18_251.png

(18.97)

The dipole tensor therefore changes only by a quantity of relative order d/Λ when the preferred time axis is altered. To the accuracy already adopted in the multipole expansion, l18_252.png is independent of the choice of frame.

l18_253.gif

Figure 18.18: Frame independence. Changing the preferred time axis (blue to green) alters the dipole tensor only by a relative amount of order d/Λ, which is already neglected in the multipole expansion.

The same conclusion applies to the macroscopic polarization and magnetization constructed from l18_254.png. They may be computed in any convenient frame; the result, to the order retained here, is unique.

The Field-Dipole Moment Interaction

Once the averaged current has been decomposed into free and dipole pieces, Maxwell’s equations take the form

l18_255.png

(18.98)

The dipole tensor therefore acts as an additional source. The corresponding interaction energy density is the scalar contraction

l18_256.png

(18.98)

Adding this term to the free-field and free-current contributions produces the macroscopic Lagrangian

l18_257.png

(18.100)

In the rest frame of the material the contraction reduces to the familiar expression

l18_258.png

(18.101)

where l18_259.png and l18_260.png are the electric polarization and the magnetization constructed from the mixed and spatial components of l18_261.png. The same scalar appears as the interaction energy of a dipole with an external field, confirming that the relativistic coupling introduced above is the correct continuum generalization of the elementary dipole interaction.

l18_262.gif

Figure 18.19: Field-dipole interaction. The contraction l18_263.png reduces in the rest frame to l18_264.png, the energy density of polarized matter in an external field.

The Matter Dipole-Moment Interaction

Polarizing a material requires energy. The simplest continuum description of that energy is a quadratic form in the electric and magnetic dipole densities,

l18_265.png

(18.102)

The coefficients κ and χ function as spring constants; they are material-dependent and may vary from point to point.

To obtain a Lorentz-covariant expression one replaces the rest-frame squares by the appropriate contractions with the four-velocity l18_266.png of the material,

l18_267.png

(18.103)

The complete Lagrangian of matter, field, and polarization is then

l18_268.png

(18.104)

Variation with respect to the potential recovers Maxwell’s equations. Variation with respect to the dipole tensor itself yields the linear constitutive relations. In the local rest frame they reduce to

l18_269.png

(18.105)

and

l18_270.png

(18.106)

The covariant statement of the same stationarity condition is

l18_271.png

(18.107)


The dimensionless coefficient κ is the electric susceptibility; for ordinary materials it ranges from l18_272.png to l18_273.png. The magnetic susceptibility χ is typically far smaller: negative for diamagnetic substances and positive for paramagnetic ones.

l18_274.gif

Figure 18.20: Linear response. In the rest frame the polarization is proportional to the electric field and the magnetization is proportional to the magnetic field; the constants of proportionality are the electric and magnetic susceptibilities.

Other Choices of Polarization Fields

The components of the dipole tensor l18_275.png have so far been treated as the fundamental fields that describe polarization. Polarization, however, is a property of the matter itself. It is therefore natural to introduce fields that live on the material manifold and are dragged along with the flow.

Define the Lagrangian-frame polarization and magnetization by

l18_276.png

(18.108)

In the rest frame the inverse relations are simply

l18_277.png

(18.109)

The same relations, written covariantly, reconstruct the spacetime dipole tensor from the material fields and the particle current,

l18_278.png

(18.110)

When these expressions are substituted into the earlier Lagrangian one obtains

l18_279.png

(18.111)

The polarization fields l18_280.png and l18_281.png are now the independent variables that characterize the material response; the spacetime tensor l18_282.png is a derived object. Variation with respect to l18_283.png and l18_284.png again yields the linear constitutive relations, but the underlying variational principle is expressed entirely in terms of quantities that transform as scalars under changes of the material coordinates.

l18_285.gif

Figure 18.21: Material-frame polarization. The fieldsl18_286.png and l18_287.png are defined on the body manifold; the spacetime dipole tensor l18_288.png is obtained from them by the flow of the material.

The Electric Susceptibility Matrix

The electric contribution to the polarization energy may be generalized by replacing the deformation tensor with an arbitrary symmetric matrix l18_289.png. With n the number of particles per Lagrangian volume element the term becomes

l18_290.png

(18.112)

Variation with respect to the material polarization then yields the linear relation

l18_291.png

(18.113)

where the Lagrangian-frame electric field is the pull-back

l18_292.png

(18.114)

In the special case of an undeformed, stationary element this reduces to the familiar laboratory expression

l18_293.png

(18.115)

For a deformed element observed in its local rest frame the same relation acquires the Jacobian factors of the deformation,

l18_294.png

(18.116)

The field equations remain unchanged if the susceptibility matrix is allowed to depend on the material coordinates; such dependence simply describes an inhomogeneous medium.

When the strain is small the susceptibility may be expanded to first order,

l18_295.png

(18.117)

The unstrained matrix l18_296.png is symmetric and therefore possesses six independent components. The tensor l18_297.png is symmetric in each pair i j and k l, giving thirty-six independent components in the most general anisotropic solid.

Isotropy imposes a strong restriction. For every rotation matrix A one must have

l18_298.png

(18.118)

The only tensors compatible with this requirement are

l18_299.png

(18.119)

and

l18_300.png

(18.120)

The two scalars l18_301.png and l18_302.png measure the change in susceptibility under pure compression and under pure shear, respectively. For a dielectric fluid the susceptibility is isotropic in the current configuration and takes the still simpler form

l18_303.png

(18.121)

l18_304.gif

Figure 18.22: Strain dependence of the susceptibility. In an isotropic solid the unstrained response is a pure multiple of the identity (blue); small strain adds independent compression and shear corrections (green).

The Magnetic Susceptibility Matrix

The magnetic contribution to the polarization energy is treated in exact analogy with the electric term. The simplest covariant expression is

l18_305.png

(18.122)

Replacing the deformation tensor by a general symmetric matrix l18_306.png and introducing the particle density n yields the more flexible form

l18_307.png

(18.123)

Variation with respect to the material magnetization then produces

l18_308.png

(18.124)

where the Lagrangian-frame magnetic field is the pull-back of the dual field strength,

l18_309.png

(18.125)

In the local rest frame the same relation becomes

l18_310.png

(18.126)

As in the electric case, the susceptibility matrix may depend on the material coordinates, thereby describing a magnetically inhomogeneous medium, and may be expanded in powers of the strain when the deformation is small. Isotropy again reduces the independent coefficients to a pair of scalars that govern the response to compression and to shear.

l18_311.gif

Figure 18.23: Magnetic response. The magnetization is obtained from the magnetic field by contraction with the susceptibility matrix l18_312.png; deformation of the material mixes the laboratory components through the deformation gradients.

Another Look at the Stress-Energy Tensor

The complete Lagrangian of the coupled system is the sum of seven contributions,

l18_313.png

(18.127)

The pure-field and free-current pieces are the familiar expressions

l18_314.png

(18.128)

and

l18_315.png

(18.129)

while the field-dipole couplings are

l18_316.png

(18.130)

The remaining terms are the quadratic polarization energies and the matter internal energy already introduced.

The canonical stress-energy tensor is constructed in the usual way,

l18_317.png

(18.131)

Its associated spin current is

l18_318.png

(18.132)

After the Belinfante improvement that employs Maxwell’s equations, the symmetric tensor splits into the same seven pieces,

l18_319.png

(18.133)

The pure electromagnetic contribution recovers the vacuum Maxwell tensor,

l18_320.png

(18.134)

the free-current piece vanishes identically, and the remaining pieces are the interaction and material terms listed in the original calculation.

In the material rest frame the energy density, momentum density, and stresses reduce to

l18_321.png

(18.135)

and

l18_322.png

(18.136)

together with the corresponding spatial stresses. Introducing the auxiliary fields

l18_323.png

(18.137)

and

l18_324.png

(18.138)

rewrites the energy density and the Poynting flux in the compact forms

l18_325.png

(18.139)

and

l18_326.png

(18.140)

When the susceptibilities themselves depend on strain, additional stress contributions appear. To first order in the strain one has

l18_327.png

(18.141)

and

l18_328.png

(18.142)

The polarization-matter and magnetization-matter stresses then become

l18_329.png

(18.143)

and

l18_330.png

(18.144)

where the barred coefficients absorb the deformation gradients. The complete electromagnetic stress in a solid is therefore

l18_331.gif

(18.145)

The electric and magnetic sectors enter symmetrically.

For a polarizable fluid the susceptibilities are isotropic in the current configuration,

l18_332.png

(18.146)

and

l18_333.png

(18.147)

The interaction stresses simplify to

l18_334.png

(18.148)

and

l18_335.png

(18.149)

Collecting terms yields the electromagnetic stress of a fluid,

l18_336.png

(18.150)

All contributions are now expressed through the macroscopic fields l18_337.png, l18_338.png and the derivatives of the susceptibilities with respect to specific volume.

l18_339.gif

Figure 18.24: Electromagnetic contributions to the stress-energy tensor in matter. Energy density (blue), energy flux l18_340.png (green), and the stresses built from l18_341.png and l18_342.png (red), together with the strain corrections that arise when the susceptibilities depend on deformation.

Further Reading

Kip S. Thorne, Roger D. Blandford, (2017), Modern Classical Physics, Princeton University Press

Charles W. Misner, Kip S. Thorne, John Archibald Wheeler, (1973), Gravitation, W. H. Freeman and Company.

George E. Hrabovsky, (2020), Relativistic Viscous Fluids, Midwest Relativity Meeting, University of Notre Dame, IN

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