Contents13 sections
  1. Field operators definition
  2. Properties
  3. Rigor
  4. Setup
  5. Equate to find $\mathcal{E}k$
  6. Infinite limit
  7. $E(\omega)$ operator
  8. Positive‑ and negative‑frequency parts (standard decomposition)
  9. Substitute back to the state expansion
  10. The commutation
  11. In 3D
  12. Continuous limit in 3D
  13. Positive- and negative-frequency parts in 3D

Field operators definition§

From the discrete case,

ψ;f=kf(k)a(k)0\ket{\psi;f}=\sum_k f(k) a^\dagger(k)\ket{0}

We can easily see what we need, which is

ψ;f=dωf(ω)E(ω)0\ket{\psi;f}=\int \mathrm{d}\omega\, f(\omega) E^\dagger(\omega)\ket{0}

This is the definition of EE we will take; it is the aa operator in the continuous limit.

Properties§

Since ψ;f\ket{\psi;f} should be normalized, and assuming [E(ω),E(ω)][E(\omega),E^\dagger(\omega')] is a c‑number, the normalization condition forces

[E^(ω),E^(ω)]=δ(ωω).[\hat{E}(\omega), \hat{E}^\dagger(\omega')]=\delta(\omega-\omega').

From the previous chapter, we noted that

[a^k,a^k]=δkk.[\hat{a}_k, \hat{a}_{k'}^\dagger]=\delta_{kk'}.

For a field with continuous modes, the equivalent relation is

[E^(ω),E^(ω)]=δ(ωω).[\hat{E}(\omega), \hat{E}^\dagger(\omega')]=\delta(\omega-\omega').

Rigor§

Although the interpretation makes it obvious why the above should be true, it is worth noting more physical detail via a rigorous derivation.

Setup§

We consider an one‑dimensional cavity of length LL with periodic boundary conditions. The classical electromagnetic field in Coulomb gauge can be expanded in normal modes. Quantization promotes the Fourier amplitudes to operators.

The full free‑field Hamiltonian is

H^=120Ldx(ϵ0E^2(x)+1μ0B^2(x)).\hat{H} = \frac{1}{2}\int_0^L \mathrm{d}x \left( \epsilon_0 \hat{E}^2(x) + \frac{1}{\mu_0}\hat{B}^2(x) \right).

A general expansion of the electric field consistent with the wave equation and the boundary conditions is

E^(x)=ikEk(a^keikxa^keikx),\hat{E}(x) = i\sum_k \mathcal{E}_k \left( \hat{a}_k e^{ikx} - \hat{a}_k^\dagger e^{-ikx} \right),

where k=2πn/Lk = 2\pi n/L with nZn\in\mathbb{Z}, and Ek\mathcal{E}_k is a real normalization constant to be determined (it may depend on k|k|).

The ii and the negative phase on a^\hat{a}^\dagger here is by convention where A^\hat{A} should be a^eikx+a^eikx\propto \hat{a}e^{ikx} + \hat{a}^\dagger e^{-ikx} then E^=tA^\hat{E}=-\partial_t \hat{A} since A^\hat{A} is the canonical variable that have the priority to be quantized.

The corresponding magnetic field for a plane‑polarized wave propagating along xx is

B^(x)=ikkkEkc(a^keikxa^keikx),c=1ϵ0μ0.\hat{B}(x) = i\sum_k \frac{k}{|k|}\frac{\mathcal{E}_k}{c} \left( \hat{a}_k e^{ikx} - \hat{a}_k^\dagger e^{-ikx} \right), \qquad c = \frac{1}{\sqrt{\epsilon_0\mu_0}}.

The bosonic operators satisfy [a^k,a^k]=δk,k[\hat{a}_k,\hat{a}_{k'}^\dagger] = \delta_{k,k'}, [a^k,a^k]=0[\hat{a}_k,\hat{a}_{k'}]=0.

Equate to find Ek\mathcal{E}_k§

Insert the expansions into H^\hat{H} and use the spatial integrals

0Lei(k+k)xdx=Lδk,k,0Lei(kk)xdx=Lδk,k.\int_0^L e^{i(k+k')x}\mathrm{d}x = L\delta_{k,-k'},\qquad \int_0^L e^{i(k-k')x}\mathrm{d}x = L\delta_{k,k'}.

After straightforward algebra, the Hamiltonian becomes

H^=kϵ0LEk2(2a^ka^k+1+a^ka^k+a^ka^k)k1μ0c2LEk2(a^ka^k+a^ka^k),\begin{aligned} \hat{H} &= \sum_k \epsilon_0 L \mathcal{E}_k^2 \Bigl(2\hat{a}_k^\dagger\hat{a}_k + 1 + \hat{a}_k\hat{a}_{-k} + \hat{a}_k^\dagger\hat{a}_{-k}^\dagger \Bigr) \\ &\qquad - \sum_k \frac{1}{\mu_0 c^2} L \mathcal{E}_k^2 \Bigl( \hat{a}_k\hat{a}_{-k} + \hat{a}_k^\dagger\hat{a}_{-k}^\dagger \Bigr), \end{aligned}

where we used [a^k,a^k]=1[\hat{a}_k,\hat{a}_k^\dagger]=1 and kept only non‑vanishing terms.
Because ϵ0μ0c2=1\epsilon_0\mu_0 c^2 = 1, the coefficients in front of the non‑diagonal terms a^ka^k\hat{a}_k\hat{a}_{-k} and a^ka^k\hat{a}_k^\dagger\hat{a}_{-k}^\dagger cancel exactly. The remaining diagonal part is

H^=k2ϵ0LEk2(a^ka^k+12).\hat{H} = \sum_k 2\epsilon_0 L \mathcal{E}_k^2 \left( \hat{a}_k^\dagger\hat{a}_k + \frac{1}{2} \right).

We demand that this reproduces the known harmonic‑oscillator Hamiltonian H^=kωk(a^ka^k+1/2)\hat{H} = \sum_k \hbar\omega_k (\hat{a}_k^\dagger\hat{a}_k + 1/2). Comparing the two expressions yields

2ϵ0LEk2=ωkEk=ωk2ϵ0L.2\epsilon_0 L \mathcal{E}_k^2 = \hbar\omega_k \quad\Longrightarrow\quad \mathcal{E}_k = \sqrt{\frac{\hbar\omega_k}{2\epsilon_0 L}}.

Thus the electric field operator is

E^(x)=ikωk2ϵ0L(a^keikxa^keikx).\hat{E}(x) = i\sum_k \sqrt{\frac{\hbar\omega_k}{2\epsilon_0 L}} \left( \hat{a}_k e^{ikx} - \hat{a}_k^\dagger e^{-ikx} \right).

Infinite limit§

Let Δk=2πL\Delta k = \frac{2\pi}{L}. In order to make the modes continuous, we take LL\to\infty. Factor as follows:

E^(x)=ik2πLωk4πϵ0(eikxL2πa^keikxL2πa^k)Lidkωk4πϵ0E^(k)eikx+h.c.,\begin{align*} \hat{E}(x) &= i\sum_k \frac{2\pi}{L} \sqrt{\frac{\hbar\omega_k}{4\pi\epsilon_0}} \left( e^{ikx} \sqrt{\frac{L}{2\pi}}\,\hat{a}_k - e^{-ikx} \sqrt{\frac{L}{2\pi}}\,\hat{a}_k^\dagger \right) \\ &\xrightarrow[L\to\infty]{} i\int_{-\infty}^{\infty} \mathrm{d}k \, \sqrt{\frac{\hbar\omega_k}{4\pi\epsilon_0}} \, \hat{E}(k) e^{ikx} + \text{h.c.}, \end{align*}

where we defined the continuum annihilation operator

E^(k)=L2πa^k,[E^(k),E^(k)]=δ(kk).\hat{E}(k) = \sqrt{\frac{L}{2\pi}}\,\hat{a}_k, \qquad [\hat{E}(k),\hat{E}^\dagger(k')] = \delta(k-k').

E(ω)E(\omega) operator§

Because ωk=ck\omega_k = c|k|, we can restrict the integration to positive frequencies. For ω>0\omega>0, set k=ω/ck = \omega/c (positive kk) and dk=dω/c\mathrm{d}k = \mathrm{d}\omega/c. Then

E^(x)=i0dωω4πϵ0cE^(ω)eiωx/c+h.c.,\hat{E}(x) = i\int_{0}^{\infty} \mathrm{d}\omega \, \sqrt{\frac{\hbar\omega}{4\pi\epsilon_0 c}} \, \hat{E}(\omega) e^{i\omega x/c} + \text{h.c.},

where we have absorbed the factor 1/c1/\sqrt{c} from the integration measure into the definition of the continuous frequency operator

E^(ω)1cE^(k ⁣= ⁣ω/c).\hat{E}(\omega) \equiv \frac{1}{\sqrt{c}} \hat{E}(k\!=\!\omega/c).

With this definition, [E^(ω),E^(ω)]=δ(ωω)[\hat{E}(\omega),\hat{E}^\dagger(\omega')] = \delta(\omega-\omega') because

[E^(ω),E^(ω)]=1c[E^(ω/c),E^(ω/c)]=1cδ ⁣(ωωc)=δ(ωω).[\hat{E}(\omega),\hat{E}^\dagger(\omega')] = \frac{1}{c} [\hat{E}(\omega/c),\hat{E}^\dagger(\omega'/c)] = \frac{1}{c} \delta\!\left(\frac{\omega-\omega'}{c}\right) = \delta(\omega-\omega').

Positive‑ and negative‑frequency parts (standard decomposition)§

We define the positive‑frequency part of the electric field operator as

E^(+)(x)i0dωω4πϵ0cE^(ω)eiωx/c,\hat{E}^{(+)}(x) \equiv i\int_{0}^{\infty}\mathrm{d}\omega\, \sqrt{\frac{\hbar\omega}{4\pi\epsilon_0 c}}\,\hat{E}(\omega) e^{i\omega x/c},

and the negative‑frequency part as its Hermitian conjugate:

E^()(x)[E^(+)(x)]=i0dωω4πϵ0cE^(ω)eiωx/c.\hat{E}^{(-)}(x) \equiv \left[\hat{E}^{(+)}(x)\right]^\dagger = -i\int_{0}^{\infty}\mathrm{d}\omega\, \sqrt{\frac{\hbar\omega}{4\pi\epsilon_0 c}}\,\hat{E}^\dagger(\omega) e^{-i\omega x/c}.

Then the full (Hermitian) field operator is simply

E^(x)=E^(+)(x)+E^()(x).\hat{E}(x) = \hat{E}^{(+)}(x) + \hat{E}^{(-)}(x).

This decomposition is standard in quantum optics because E^(+)(x)\hat{E}^{(+)}(x) annihilates the vacuum and E^()(x)\hat{E}^{(-)}(x) creates excitations.

Substitute back to the state expansion§

The state ψ;f|\psi;f\rangle transforms accordingly. Up to a re-scaling of ff,

ψ;f=dkL2πf(k)E^(k)0=dkf~(k)E^(k)0=dωf(ω)E(ω)0.\begin{align*} \ket{\psi;f} &= \int\mathrm{d}k\,\sqrt{\frac{L}{2\pi}}f(k)\,\hat{E}^\dagger(k)\ket{0} \\ &= \int\mathrm{d}k\,\tilde{f}(k)\,\hat{E}^\dagger(k)\ket{0} \\ &= \int\mathrm{d}\omega\,f(\omega)E^\dagger(\omega)\ket{0}. \end{align*}

The commutation§

From the definition E^(k)=L/(2π)a^k\hat{E}(k)=\sqrt{L/(2\pi)}\,\hat{a}_k and [a^k,a^k]=δkk[\hat{a}_k,\hat{a}_{k'}^\dagger]=\delta_{kk'}, we have

[E^(k),E^(k)]=L2πδkk  L  δ(kk).[\hat{E}(k),\hat{E}^\dagger(k')] = \frac{L}{2\pi}\delta_{kk'} \;\xrightarrow[L\to\infty]{}\; \delta(k-k').

In terms of frequency,

[E(ω),E(ω)]=δ(ωω),[E(\omega),E^\dagger(\omega')] = \delta(\omega-\omega'),

which matches the result obtained from normalization.

In 3D§

It is anyway a phase convention, we will drop the ii from here. Then, in 3D

E^(r)=k,λEk(a^k,λe^k,λeikr+a^k,λe^k,λeikr)\hat{\mathbf{E}}(\mathbf{r})=\sum_{\mathbf{k},\lambda}\mathcal{E}_k\left(\hat{a}_{\mathbf{k},\lambda}\,\hat{\mathbf{e}}_{\mathbf{k},\lambda}\,e^{i\mathbf{k}\cdot\mathbf{r}}+\hat{a}^\dagger_{\mathbf{k},\lambda}\,\hat{\mathbf{e}}^*_{\mathbf{k},\lambda}\,e^{-i\mathbf{k}\cdot\mathbf{r}}\right)

where

Ek=ωk2ϵ0V\mathcal{E}_k=\sqrt{\frac{\hbar \omega_k}{2\epsilon_0 V}}

The sum is over all wavevectors k=2πL(nx,ny,nz)\mathbf{k} = \frac{2\pi}{L}(n_x, n_y, n_z) with niZn_i \in \mathbb{Z}, and over two transverse polarizations λ=1,2\lambda = 1,2 satisfying e^k,λk\hat{\mathbf{e}}_{\mathbf{k},\lambda} \perp \mathbf{k}.

Continuous limit in 3D§

The discrete sum becomes an integral via the replacement

kV(2π)3d3k\sum_\mathbf{k} \longrightarrow \frac{V}{(2\pi)^3}\int \mathrm{d}^3k

which follows from the fact that each mode occupies a volume (2π/L)3=(2π)3/V(2\pi/L)^3 = (2\pi)^3/V in k\mathbf{k}-space. Define the continuum operators

a^k,λV(2π)3a^(k,λ),[a^(k,λ),a^(k,λ)]=δ(3)(kk)δλλ\hat{a}_{\mathbf{k},\lambda} \longrightarrow \sqrt{\frac{V}{(2\pi)^3}}\,\hat{a}(\mathbf{k},\lambda), \qquad [\hat{a}(\mathbf{k},\lambda),\hat{a}^\dagger(\mathbf{k}',\lambda')] = \delta^{(3)}(\mathbf{k}-\mathbf{k}')\delta_{\lambda\lambda'}

so that the commutation relation becomes a Dirac delta instead of a Kronecker delta. Note the same 1/V1/\sqrt{V} cancellation as in 1D: Ek1/V\mathcal{E}_k \propto 1/\sqrt{V} while the mode density grows as VV, so all physical observables are VV-independent.

Substituting:

E^(r)=λd3k(2π)3ωk2ϵ0(a^(k,λ)e^k,λeikr+a^(k,λ)e^k,λeikr)\hat{\mathbf{E}}(\mathbf{r}) = \sum_\lambda \int \frac{\mathrm{d}^3k}{(2\pi)^3} \sqrt{\frac{\hbar\omega_k}{2\epsilon_0}} \left( \hat{a}(\mathbf{k},\lambda)\,\hat{\mathbf{e}}_{\mathbf{k},\lambda}\,e^{i\mathbf{k}\cdot\mathbf{r}} + \hat{a}^\dagger(\mathbf{k},\lambda)\,\hat{\mathbf{e}}^*_{\mathbf{k},\lambda}\,e^{-i\mathbf{k}\cdot\mathbf{r}} \right)

Switching to spherical coordinates in k\mathbf{k}-space with k=kk = |\mathbf{k}|, ωk=ck\omega_k = ck, and d3k=k2dkdΩ\mathrm{d}^3k = k^2\,\mathrm{d}k\,\mathrm{d}\Omega:

E^(r)=λ0dω(2π)3c3dΩω2ω2ϵ0(a^(ω,k^,λ)e^k^,λeiωk^r/c+h.c.)\hat{\mathbf{E}}(\mathbf{r}) = \sum_\lambda \int_0^\infty \frac{\mathrm{d}\omega}{(2\pi)^3 c^3} \int \mathrm{d}\Omega\, \omega^2 \sqrt{\frac{\hbar\omega}{2\epsilon_0}} \left( \hat{a}(\omega,\hat{k},\lambda)\,\hat{\mathbf{e}}_{\hat{k},\lambda}\,e^{i\omega\hat{k}\cdot\mathbf{r}/c} + \text{h.c.} \right)

For an atom at the origin (dipole approximation, eikratom1e^{i\mathbf{k}\cdot\mathbf{r}_\text{atom}} \approx 1) or when only the frequency content matters, one typically integrates out the angular and polarization degrees of freedom. This yields the spectral density of the field, which is the physically relevant quantity for decay rates and is manifestly VV-independent.

Positive- and negative-frequency parts in 3D§

As in 1D, we split

E^(r)=E^(+)(r)+E^()(r)\hat{\mathbf{E}}(\mathbf{r}) = \hat{\mathbf{E}}^{(+)}(\mathbf{r}) + \hat{\mathbf{E}}^{(-)}(\mathbf{r})

where

E^(+)(r)=k,λEka^k,λe^k,λeikr\hat{\mathbf{E}}^{(+)}(\mathbf{r}) = \sum_{\mathbf{k},\lambda} \mathcal{E}_k\, \hat{a}_{\mathbf{k},\lambda}\,\hat{\mathbf{e}}_{\mathbf{k},\lambda}\,e^{i\mathbf{k}\cdot\mathbf{r}}

contains only annihilation operators (positive frequency, annihilates vacuum), and E^()=[E^(+)]\hat{\mathbf{E}}^{(-)} = \left[\hat{\mathbf{E}}^{(+)}\right]^\dagger contains only creation operators. This decomposition is used throughout quantum optics: photodetection theory, the optical Bloch equations, and the input-output formalism all rely on it.

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