Dielectric


A dielectric or insulator is a material in which all electric charges are bound to a specific atom or molecule and cannot move far from it. There are no free charges.

Behavior under an electric field

Atoms

The simplest possible dielectric is a single atom, with a positively charged atomic nucleus and a negatively charged electron cloud surrounding it. When subject to an electric field, the nucleus and electron cloud move in opposite direction, as one is attracted by the field and the other is repelled. With a strong enough field, the electrons can be ripped from the nucleus, thus ionizing the atom, but for milder fields, a state of equilibrium is reached.

The force keeping the nucleus and cloud together balances the one applied by the external field. In this state, the geometric center of the electron cloud, which acts as a sort of charge equivalent of the Center of mass, does not coincide with the (approximately point-like) nucleus. As such, the positive and negative charges of the atom are not superimposed and this turns the atom into an electric dipole, with a (tiny) electric dipole moment that is typically proportional to the strength of the external field. Such an atom (or molecule) is said to be polarized and the dipole moment is modeled as

p=αE\mathbf{p}=\alpha \mathbf{E}

where E\mathbf{E} is the field and α\alpha is an atom-specific constant called the atomic polarizability.

Molecules

In the case of molecules, the situation is more complicated, as the geometry of a molecule determines whether there are directions in which it is more easily polarized. In the case of a linear molecule, such as CO2\text{CO}_{2}, the polarizability is highest on the molecule's axis. This complicates the induced moment's formula due to having to consider both the components parallel and perpendicular to the axis:

p=αE+αE\mathbf{p}=\alpha_{\perp}\mathbf{E}_{\perp}+\alpha_{\parallel}\mathbf{E}_{\parallel}

This may make the moment not even in the same direction of the field. For completely asymmetrical molecules, the polarizability splits in nine different components, one for every combination of axes. The object containing these components is called the polarizability tensor and is applied to the electric field:

(pxpypz)=(αxxαxyαxzαyxαyyαyzαzxαzyαzz)(ExEyEz)\begin{pmatrix} p_{x} \\ p_{y} \\ p_{z} \end{pmatrix}=\begin{pmatrix} \alpha_{xx} & \alpha_{xy} & \alpha_{xz} \\ \alpha_{yx} & \alpha_{yy} & \alpha_{yz} \\ \alpha_{zx} & \alpha_{zy} & \alpha_{zz} \end{pmatrix}\begin{pmatrix} E_{x} \\ E_{y} \\ E_{z} \end{pmatrix}

Some molecules are permanently polarized due to their geometry. These are called polar molecules. If a uniform field is applied, the force on the positive end of the molecule is F+=qE\mathbf{F}_{+}=q\mathbf{E} and cancels out the force of the negative end F=qE\mathbf{F}_{-}=-q\mathbf{E} exactly. However, a moment of force is applied:

N=(r+×F+)+(r×F)=(d2×qE)+(d2×(qE))=qd×E\mathbf{N}=(\mathbf{r}_{+}\times \mathbf{F}_{+})+(\mathbf{r}_{-}\times \mathbf{F}_{-})=\left( \frac{\mathbf{d}}{2}\times q\mathbf{E} \right)+\left( - \frac{\mathbf{d}}{2}\times (-q\mathbf{E}) \right)=q\mathbf{d}\times \mathbf{E}

where d\mathbf{d} is the distance from the center of the molecule. Clearly then, a dipole p\mathbf{p} in a uniform field experiences a moment of force

N=p×E\mathbf{N}=\mathbf{p}\times \mathbf{E}

Notably, N\mathbf{N} is in such a direction as to make p\mathbf{p} line up parallel to E\mathbf{E}, as for N\mathbf{N} to be zero, and hence stop the rotation, p\mathbf{p} must be parallel to E\mathbf{E}. This means that the dipole will rotate until it points in the direction of the field.

If the field is nonuniform, F+\mathbf{F}_{+} does not balance F\mathbf{F}_{-} and there will be a net force on the molecule (on top of the moment of force). This is uncommon, as since molecules are tiny, the variation of the field needs to be very important such that we can't ignore the variation even in the space of a molecule. That said, the formula is

F=ΔF±=q(E+E)=qΔE\mathbf{F}=\Delta \mathbf{F}_{\pm}=q(\mathbf{E}_{+}-\mathbf{E}_{-})=q\Delta \mathbf{E}

If the dipole is tiny, we can approximate this for each axis as

ΔEi(Ei)d\Delta E_{i}\equiv(\nabla E_{i})\cdot \mathbf{d}

where i=x,y,zi=x,y,z. In vector terms

ΔE=(d)E\Delta \mathbf{E}=(\mathbf{d}\cdot \nabla)\mathbf{E}

and therefore

F=(p)E\mathbf{F}=(\mathbf{p}\cdot \nabla)\mathbf{E}

and the moment of force therefore sums to the previous one to get

N=p×E+r×F\mathbf{N}=\mathbf{p}\times \mathbf{E}+\mathbf{r}\times \mathbf{F}

Linear dielectrics

At a macroscopic level, we can estimate the behavior of materials by their behavior at a microscopic level. From the study of dielectric polarization, we know that it comes from the alignment of atoms and molecules around the electric field. We also know that the intensity of their dipole moment is dependent on the strength of the field, so long it's not large enough to break the molecules. Thus, we can (qualitatively) assume that the polarization of a dielectric is dependent on the electric field that is applied onto it. In fact, many material not only exhibit this dependence, but specifically a linear dependence:

P=ε0χeE\mathbf{P}=\varepsilon_{0}\chi_{e}\mathbf{E}

where ε0\varepsilon_{0} is the vacuum permittivity and χe\chi_{e} is the electric susceptibility, whose value depends on the microscopic structure of the material and external factors like temperature. E\mathbf{E} is the total field, including the one caused by polarization itself. Materials that obey this relation are known as linear dielectrics.

The dependence on the total field, as opposed to the external field, can cause problems: say you apply a field to a dielectric. It gets polarized and starts producing a field of its own, which adds on top of the external one, which in turn causes a variation in the polarization, which changes the material's field, which changes the total field, which changes the polarization, which— you get the point. Logically, it goes on to infinity, though it eventually comes to rest. Breaking out of the infinite loop can be done, for instance, by examining the electric displacement instead:

D=ε0E+P=ε0E+ε0χeE=ε0(1+χe)E\mathbf{D}=\varepsilon_{0}\mathbf{E}+\mathbf{P}=\varepsilon_{0}\mathbf{E}+\varepsilon_{0}\chi_{e}\mathbf{E}=\varepsilon_{0}(1+\chi_{e})\mathbf{E}

We can define the permittivity of a material as

ε=ε0(1+χe)\varepsilon=\varepsilon_{0}(1+\chi_{e})

and thus the displacement is

D=εE\boxed{\mathbf{D}=\varepsilon \mathbf{E}}

Despite the displacement being entirely dependent on E\mathbf{E}, the Curl of D\mathbf{D} is still not guaranteed to be zero. This is because for it to be zero, the line integral across the boundary between materials needs to be zero, but it isn't zero as the electric susceptibility changes when switching material. In fact, this discontinuity in χe\chi_{e} not only causes the curl to be nonzero, it makes it blow up to infinity in those points. Mathematically, the cause is that the curl of P\mathbf{P} in linear dielectrics is

×P=ε0×(χeE)=ε0E×(χe)\nabla\times\mathbf{P}=\varepsilon_{0}\nabla\times\mathbf{(\chi_{e}\mathbf{E})}=-\varepsilon_{0}\mathbf{E}\times(\nabla \chi_{e})

and is dependent on the Gradient of χe\chi_{e}. The only way this can be zero is if χe\chi_{e} is spatially constant. In other words, all space1 needs to have the same susceptibility, in which case χe=0\nabla \chi_{e}=0 and the curl of P\mathbf{P} (and therefore D\mathbf{D}) is zero everywhere. A material in which the susceptibility is constant is said to be homogeneous. In this scenario, the displacement is very much analogous to the electric field and similar laws apply to it:

D=ρf,×D=0\nabla\cdot\mathbf{D}=\rho_{f},\qquad \nabla\times\mathbf{D}=0

and the displacement can be calculated as if the dielectric was not there in the first place:

D=ε0Evac\mathbf{D}=\varepsilon_{0}\mathbf{E}_\text{vac}

where Evac\mathbf{E}_\text{vac} is the field that would be produced by the same free charge distribution if the dielectric was not there. It is related to the actual field by a constant:

E=1εD=1εrEvac\mathbf{E}=\frac{1}{\varepsilon}\mathbf{D}=\frac{1}{\varepsilon_{r}}\mathbf{E}_\text{vac}
Boundary values

Under the assumption that the linear dielectric is both homogeneous and isotropic, the bound charge density ρb\rho_{b} is proportional to the free charge density ρf\rho_{f}:

ρb=P=(ε0χeεD)=(χe1+χe)ρf\boxed{\rho_{b}=-\nabla\cdot\mathbf{P}=-\nabla \cdot\left( \varepsilon_{0} \frac{\chi_{e}}{\varepsilon}\mathbf{D} \right)=-\left( \frac{\chi_{e}}{1+\chi_{e}} \right)\rho_{f}}

In particular, unless free charge is embedded in the material, the bound charge density must be zero. Thus, all the charge must reside on the surface. This way, the potential obeys Laplace's equation and it can be used to find it.

The conditions can also be rewritten to explicitly only reference the free charge too. Starting from the displacement boundary conditions we have

DaboveDbelow=εaboveEaboveεbelowEbelow=σfD_\text{above}^{\perp}-D_\text{below}^{\perp}=\varepsilon _\text{above}E_\text{above}^{\perp}-\varepsilon _\text{below}E_\text{below}^{\perp}=\sigma_{f}

and in terms of potential

εaboveVabovenεbelowVbelown=σf\varepsilon _\text{above}\frac{ \partial V_\text{above} }{ \partial n } -\varepsilon _\text{below}\frac{ \partial V_\text{below} }{ \partial n } =-\sigma_{f}

Energy

In capacitors

From the fact that a Capacitor filled with dielectric has a higher capacitance, and from the formula

W=12CV2W=\frac{1}{2}CV^{2}

we can recognize that it must take more work to charge a dielectric-filled capacitor than a vacuum one. The reason here is because part of the field is cancelled out by the bound charges that occur in a material, thus it takes more free charge to achieve the same potential.

In linear dielectrics

For a linear dielectric, the displacement is D=εE\mathbf{D}=\varepsilon \mathbf{E}. We can modify the formula for the electrostatic energy stored in a system to take this into account:

W=ε02εrE2 dτ=12DE dτW=\frac{\varepsilon_{0}}{2}\int \varepsilon_{r}E^{2}\ d\tau=\frac{1}{2}\int \mathbf{D}\cdot \mathbf{E}\ d\tau

To prove this is true, suppose some (not necessarily linear) dielectric is fixed and we move a free charge closer. Since the distribution ρf\rho_{f} is increased by an amount of Δρf\Delta \rho_{f} each time the charge moves a little bit closer, the polarization will change and with it, the bound charge distribution. We're only interested about the incremental work done on the free charge itself:

ΔW=(Δρf)V dτ\Delta W=\int(\Delta \rho_{f})V\ d\tau

Since D=ρf\nabla\cdot\mathbf{D}=\rho_{f}, Δρf=(ΔD)\Delta \rho_{f}=\nabla \cdot(\Delta \mathbf{D}), where ΔD\Delta \mathbf{D} is the change in displacement due to moving the free charge closer. So

ΔW=[(ΔD)]V dτ\Delta W=\int[\nabla \cdot(\Delta \mathbf{D})]V\ d\tau

Now

[(ΔD)V]=[(ΔD)]V+ΔD(V)\nabla \cdot[(\Delta \mathbf{D})V]=[\nabla \cdot(\Delta \mathbf{D})]V+\Delta \mathbf{D}\cdot(\nabla V)

and using integration by parts we get

ΔW=[(ΔD)V] dτ+(ΔD)E dτ\Delta W=\int \nabla \cdot[(\Delta \mathbf{D})V]\ d\tau+\int(\Delta \mathbf{D})\cdot \mathbf{E}\ d\tau

The divergence theorem turns the first integral into a surface integral, which vanishes if we integrate over all space. Thus, only the second term remains

ΔW=(ΔD)E dτ\Delta W=\int(\Delta \mathbf{D})\cdot \mathbf{E}\ d\tau

This is universal and applies to all dielectrics. Now suppose it is linear. We can substitute the displacement like

(ΔD)E=ε(ΔE)E=12Δ(εE2)=12Δ(DE)(\Delta \mathbf{D})\cdot \mathbf{E}=\varepsilon(\Delta \mathbf{E})\cdot \mathbf{E}=\frac{1}{2}\Delta(\varepsilon E^{2})=\frac{1}{2}\Delta(\mathbf{D}\cdot \mathbf{E})

(for infinitesimal increments). Thus

ΔW=Δ(12DE dτ)\Delta W=\Delta\left( \frac{1}{2}\int \mathbf{D}\cdot \mathbf{E}\ d\tau \right)

The total work done to build up the charge all the way from zero to the end result, then, is

W=12DE dτ\boxed{W=\frac{1}{2}\int \mathbf{D}\cdot \mathbf{E}\ d\tau}

This formula ends up differing from the original one, but not because either are wrong, they just represent different energies. The general one dependent on the square of the field represents the energy required to assemble all charges in the system, both free and bound, by moving each one independently from infinity (or whatever point of reference). This does not, however, include the energy spent when rotating and stretching the molecules and atoms of the dielectric to actually get the charges into their expected geometry, as you are moving the charges one by one. The second formula, dependent on the displacement, instead represents the energy required to move only the free charge, but does include the elastic "spring" energy contained in the atoms and molecules due to, well, their displacement. The difference here is that the first energy is about moving charges as if they were independent, while the second involves moving only the free ones and figuring out how bound charges respond. The latter is always higher (as it also includes the elastic energy) and generally the one you want, as free charges are usually artificially controlled, but bound ones are not.

Electromagnetic wave dispersion

Dispersion is the frequency dependence of a wave's phase velocity. It is a known phenomenon in optics, where light scattering from a piece of glass disperses into a rainbow. This section attempts to explain why an electromagnetic wave disperses in a dielectric.

A correct model of dispersion requires a quantum mechanical model of electronic structure, but a qualitative model can be developed even with classical physics alone. Our end goal is to explain why the permittivity ε\varepsilon of a dielectric is dependent on the angular frequency ω\omega of an electromagnetic wave. We will do so through a simplified model of electrons in matter.

Each electron in a dielectric is, generally speaking, bound to a specific molecule. We'll say that there is a binding force FbindingF_{\text{binding}} keeping the electron attached to the molecule against the displacement of imposed by the wave (which we assume to be propagating on the xx axis and polarized on the yy axis as usual) and we'll say that this force is elastic and described by Hooke's law:

Fbinding=kx=mω02yF_\text{binding}=-kx=-m\omega_{0}^{2}y

where k=mω02k=m\omega_{0}^{2} is the spring constant, mm is the mass of the electron and ω0=k/m\omega_{0}=\sqrt{ k/m } is the natural oscillation frequency. We claim this is a valid approximation since any Potential (and thus force) can be approximated by the harmonic oscillator for small enough displacements around an equilibrium point, which the electron's stable orbit around the molecule is.

This electron is likely also subject to a damping force FdampingF_\text{damping}, which we'll assume to be a generic dissipative force

Fdamping=mγdydtF_\text{damping}=-m\gamma \frac{dy}{dt}

for some damping coefficient γ>0\gamma>0. As for why this is here, that's beyond the scope of this model. There are reasons, such as radiation damping, but they aren't relevant here.

Finally, when the wave passes by, it will enact a driving force FdrivingF_\text{driving} on the electron as per the electric field EE:

Fdriving=qE=qE0cos(ωt)F_\text{driving}=qE=qE_{0}\cos (\omega t)

where qq is the elementary charge and E0E_{0} is the amplitude of the electric part of the wave at the coordinates of the electron. Of course, the full force would be a Lorentz force including the magnetic field, but magnetic forces are tiny compared to electric ones in the vacuum, so we can ignore without loss of much generality.

Combine all of these with Newton's second law and you get

Ftot=md2ydt2=Fbinding+Fdamping+FdrivingF_\text{tot}=m \frac{d^{2}y}{dt^{2}}=F_\text{binding}+F_\text{damping}+F_\text{driving}

so

md2ydt2+mγdydt+mω02y=qE0cos(ωt)m \frac{d^{2}y}{dt^{2}}+m\gamma \frac{dy}{dt}+m\omega_{0}^{2}y=qE_{0}\cos (\omega t)

This is an inhomogeneous second-order linear Ordinary differential equation in xx, representing a damped harmonic oscillator driven at frequency ω\omega. This becomes easier to handle if we regard it as the real part of a complex differential equation in x~\tilde{x}:

d2y~dt2+γdy~dt+ω02y~=qmE0eiωt\frac{d^{2}\tilde{y}}{dt^{2}}+\gamma \frac{d\tilde{y}}{dt}+\omega_{0}^{2}\tilde{y}=\frac{q}{m}E_{0}e^{-i\omega t}

where we used Euler's formula to see the cosine as the real part of a complex exponential. In a steady state, the system oscillates at the driving frequency

x~(t)=x~0eiωt\tilde{x}(t)=\tilde{x}_{0}e^{-i\omega t}

Plugging this into the ODE and solving for x~0\tilde{x}_{0} gives

x~0=qm1ω02ω2iγωE0\tilde{x}_{0}=\frac{q}{m}\frac{1}{\omega_{0}^{2}-\omega ^{2}-i\gamma \omega}E_{0}

An oscillating charge act as an electric dipole of electric dipole moment

p~(t)=qx~(t)=q2m1ω02ω2iγωE0eiωt\tilde{p}(t)=q\tilde{x}(t)=\frac{q^{2}}{m}\frac{1}{\omega_{0}^{2}-\omega ^{2}-i\gamma \omega}E_{0}e^{-i\omega t}

Note the presence of an imaginary term iγωi\gamma \omega at the denominator. This causes a phase shift in pp compared to EE, leaving it arctan(γm/(ω02ω2))\arctan(\gamma m/(\omega_{0}^{2}-\omega ^{2})) behind. This angle is tiny when ωω0\omega\ll \omega_{0} and grows asymptotically to π\pi when ωω0\omega\gg \omega_{0}.

The exact values for ω\omega, ω0\omega_{0} and γ\gamma depend on the position of electron in the molecule and its orbit in the system. Suppose there are fjf_{j} electrons with natural frequency ωj\omega_{j} and damping coefficient γj\gamma_{j}. If there are NN molecules per unit volume, the dielectric polarization P\mathbf{P} is the real part of

P~=Nq2m(jfjωj2ω2iγjω)E~\tilde{\mathbf{P}}=\frac{Nq^{2}}{m}\left( \sum_{j} \frac{f_{j}}{\omega_{j}^{2}-\omega ^{2}-i\gamma_{j}\omega} \right)\tilde{\mathbf{E}}

Now, P\mathbf{P} (the real part) is not currently linearly proportional to E\mathbf{E} since there is a phase difference between (all due to that pesky iγjωi\gamma_{j}\omega at the denominator), so technically this is not a linear medium. However, the complex P~\tilde{\mathbf{P}} is linearly proportional to the complex E~\tilde{\mathbf{E}}, so in an odd way, we can see this as a linear medium with complex electric susceptibility χ~e\tilde{\chi}_{e} such that

P~=ε0χ~eE~\tilde{\mathbf{P}}=\varepsilon_{0}\tilde{\chi}_{e}\tilde{\mathbf{E}}

Similarly, we can define a complex permittivity ε~\tilde{\varepsilon} and a complex relative permittivity

ε~r=ε~ε0=1+Nq2mε0jfjωj2ω2iγjω(1)\tilde{\varepsilon}_{r}=\frac{\tilde{\varepsilon}}{\varepsilon_{0}}=1+ \frac{Nq^{2}}{m\varepsilon_{0}}\sum_{j} \frac{f_{j}}{\omega_{j}^{2}-\omega ^{2}-i\gamma_{j}\omega}\tag{1}

Now, in most cases the imaginary term is negligible, stamped out by ωj2ω2\omega ^{2}_{j}-\omega ^{2}. However, when ω\omega gets closer to ωj\omega_{j}, that difference approaches zero and the imaginary term is the only thing that is left. This has some major consequences, though before we examine them, let's discuss what we ended up with.

In a dispersive medium, the wave equation now reads

2E~=ε~μ02E~t2\nabla ^{2}\tilde{\mathbf{E}}=\tilde{\varepsilon}\mu_{0}\frac{ \partial ^{2}\tilde{\mathbf{E}} }{ \partial t^{2} }

of plane wave solution

E~(x,t)=E~0ei(k~xωt)\tilde{\mathbf{E}}(x,t)=\tilde{\mathbf{E}}_{0}e^{i(\tilde{k}x-\omega t)}

and complex wavenumber k~=ε~μ0 ω\tilde{k}=\sqrt{ \tilde{\varepsilon}\mu_{0} }\ \omega. We can split this in real and imaginary parts k~=k+iκ\tilde{k}=k+i\kappa to write

E~(x,t)=E~0eκxei(kxωt)\tilde{\mathbf{E}}(x,t)=\tilde{\mathbf{E}}_{0}e^{-\kappa x}e^{i(kx-\omega t)}

which is an attenuated wave. This is a logical consequence of us adding a damping force. The irradiance of the wave is proportional to the square of the electric field, IE2I\propto E^{2}, so it is attenuated like Ie2κxI\propto e^{-2\kappa x}. Because of this, we call α2κ\alpha\equiv2\kappa the absorption coefficient. It's reciprocal, 1/α1/\alpha, is called the penetration depth of the wave. It is a characteristic length for the suppression of the wave, similar to skin depth, but for irradiance. The phase velocity is vp=ω/kv_{p}=\omega/k and the refractive index is n=ck/ωn=ck/\omega. This is all quite similar to what happens to a wave incident on a perfect conductor, although the interpretation of the coefficients is different since the dampening here is due to some arbitrary force instead of rearrangement of free charge.

For most materials, there's not much else we can say without diving deeper into the nature of electronic structure. However, for gases the second term in (1)(1) is small; not enough to delete it completely, but enough to justify approximating the square root in k~=ε~μ0 ω=ε0ε~rμ0 ω\tilde{k}=\sqrt{ \tilde{\varepsilon}\mu_{0} }\ \omega=\sqrt{ \varepsilon_{0}\tilde{\varepsilon}_{r}\mu_{0} }\ \omega with the first couple of terms in its binomial expansion:

1+x1+x2\sqrt{ 1+x }\simeq1+ \frac{x}{2}

This means, since μ0=1/ε0c2\mu_{0}=1/\varepsilon_{0}c^{2},

k~=ε~ε0c2 ω=ωcε~rωc[1+Nq22mε0jfjωj2ω2iγjω]\tilde{k}=\sqrt{ \frac{\tilde{\varepsilon}}{\varepsilon_{0}c^{2}} }\ \omega=\frac{\omega}{c}\sqrt{ \tilde{\varepsilon}_{r} }\simeq \frac{\omega}{c}\left[ 1+ \frac{Nq^{2}}{2m\varepsilon_{0}}\sum_{j} \frac{f_{j}}{\omega_{j}^{2}-\omega ^{2}-i\gamma_{j}\omega} \right]

and so

n=ckω1+Nq22mε0jfj(ωj2ω2)(ωj2ω2)2+γj2ω2n=\frac{ck}{\omega}\simeq 1+ \frac{Nq^{2}}{2m\varepsilon_{0}}\sum_{j} \frac{f_{j}(\omega ^{2}_{j}-\omega ^{2})}{(\omega_{j}^{2}-\omega ^{2})^{2}+\gamma ^{2}_{j}\omega ^{2}}

and

α=2κNq2ω2mε0cjfjγj(ωj2ω2)2+γj2ω2\alpha=2\kappa \simeq \frac{Nq^{2}\omega ^{2}}{m\varepsilon_{0}c}\sum_{j} \frac{f_{j}\gamma_{j}}{(\omega_{j}^{2}-\omega ^{2})^{2}+\gamma ^{2}_{j}\omega ^{2}}

These quantities, nn and α\alpha, generally behave pretty nicely, with nn increasing monotonically with frequency. However, as we've hinted at before, ωj2ω2\omega_{j}^{2}-\omega ^{2} cancels out when ωjω\omega_{j}\simeq \omega, leaving only the damping term. When oscillations frequencies of different sources match, we get a resonance, which in general causes some weird behavior to crop up. This is the case here also, as when these two frequencies match, the refractive index crashes down immediately to the point it goes below 1. Simultaneously, the absorption coefficients spikes up, as you can see in the figure.

This resonant behavior is called anomalous dispersion. When light is shining on a material at precisely resonant frequency, it will almost entirely be absorbed, as seen by the high α\alpha value. This is a consequence of how a driven oscillator works, where the "efficiency" is maximized when the driving frequency is equal to the damping frequency. In this case, the maximum amount of energy is dissipated, as seen by the peak of α\alpha in ωj=ω\omega_{j}=\omega. Also, the fact that nn falls below one in this range implies that the phase speed of the wave vp=c/nv_{p}=c/n is greater than lightspeed. At first glance, this is unacceptable. The speed of light is one of the few untouchable tenets of physics alongside the conservation of energy. However, it's not actually a problem. The reason is the the "speed" of a wave isn't really a speed. Or rather, it is, but the definition is largely invented. There's nothing actually physical moving at the phase speed, since the very concept of speed for something like a wave doesn't even make that much sense. What is moving anyway? Waves are delocalized, spread out over a large region of space and without a clear center or "core". All concepts of "speed" on a wave are fundamentally just a suggestion, because they don't relate to any real physical object. As such, it's not really a problem for the phase speed to the exceed lightspeed. The root cause is that the actual physical object, the energy transported by the wave, does not move at phase speed2.

Outside of resonances, behavior is pretty typical. We can ignore the damping term to get

n=1+Nq22mε0jfjωj2ω2n=1+ \frac{Nq^{2}}{2m\varepsilon_{0}}\sum_{j} \frac{f_{j}}{\omega_{j}^{2}-\omega ^{2}}

Resonance frequencies are therefore "landmines" in the field of the electromagnetic spectrum. These appear pretty randomly throughout the spectrum, as the logic behind them is not at all easy to understand. For most transparent materials, the resonant frequency nearest to the visible spectrum is in the ultraviolet.

Footnotes

  1. Actually, only the space where the field is nonzero needs to be like this. We don't really care about whether the susceptibility is constant or not if there is no field at all. If the field is created within the dielectric and becomes negligible before coming out of the surface, we might as well call all space homogeneous.

  2. You might assume that group velocity must be the "correct one", then. You'd also be wrong, though, as group velocity can also exceed the speed of light near a resonance.