Quantization of the Maxwell Field: Photons
We will now start to quantize the Maxwell field Aμ(x) = {− Φ(x)∕c, A(x)} similar to the quantization of the Schrödinger field. The fact that electromagnetism has a gauge invariance implies that there are more components than actual dynamical degrees of f
- PDF / 703,484 Bytes
- 60 Pages / 439.36 x 666.15 pts Page_size
- 21 Downloads / 395 Views
		    Quantization of the Maxwell Field: Photons
 
 We will now start to quantize the Maxwell field Aμ (x) = {− (x)/c, A(x)} similar to the quantization of the Schrödinger field. The fact that electromagnetism has a gauge invariance implies that there are more components than actual dynamical degrees of freedom in the Maxwell field. This will make quantization a little more challenging than for the Schrödinger field, but we will overcome those difficulties. Electromagnetic field theory is implicitly relativistic, and quantized Maxwell theory therefore also provides us with a first example of a relativistic quantum field theory. Appendix B provides an introduction to 4-vector and tensor notation in electromagnetic theory.
 
 18.1 Lagrange Density and Mode Expansion for the Maxwell Field The equations of motion for the Maxwell field are the inhomogeneous Maxwell equations,1   ∂μ F μν = ∂μ ∂ μ Aν − ∂ ν Aμ = − μ0 j ν .
 
 (18.1)
 
 These equations can be written as jν +
 
   ∂L ∂L 1 ∂μ ∂ μ Aν − ∂ ν Aμ = − ∂μ =0 μ0 ∂Aν ∂(∂μ Aν )
 
 (18.2)
 
 1 Recall
 
 from electrodynamics that the homogeneous Maxwell equations, viz. Gauss’ law of absence of magnetic monopoles and Faraday’s law of induction, were solved through the introduction of the potentials Aμ .
 
 © The Editor(s) (if applicable) and The Author(s), under exclusive license to Springer Nature Switzerland AG 2020 R. Dick, Advanced Quantum Mechanics, Graduate Texts in Physics, https://doi.org/10.1007/978-3-030-57870-1_18
 
 431
 
 432
 
 18 Quantization of the Maxwell Field: Photons
 
 if we use the Lagrange density L = j ν Aν −
 
 1 0 1 2 Fμν F μν = E 2 − B + j · A − . 4μ0 2 2μ0
 
 (18.3)
 
 This Lagrangian provides us with the canonically conjugate momentum for the vector potential A: ˙ =  0 (A ˙ + ∇) = − 0 E, A = ∂L/∂ A
 
 (18.4)
 
 ˙ =0  = ∂L/∂ 
 
 (18.5)
 
 but
 
 vanishes identically! Therefore we cannot simply impose canonical commutation relations between the four components Aμ of the 4-vector potential and four conjugate momenta ν . To circumvent this problem we revisit the pertinent Maxwell equations (18.1), i.e. Coulomb’s law, ˙ =−  + ∇ · A
 
 1 , 0
 
 (18.6)
 
 and Ampère’s law, ∇(∇ · A) − A +
 
 1 ∂ 1 ∂2 A + 2 ∇ = μ0 j . 2 2 c ∂t c ∂t
 
 (18.7)
 
 One way to solve the problem with  = 0 is to eliminate ∇ · A from the equations of motion through the gauge freedom (x, t) → f (x, t) = (x, t) − f˙(x, t),
 
 (18.8)
 
 A(x, t) → Af (x, t) = A(x, t) + ∇f (x, t),
 
 (18.9)
 
 i.e. we impose the gauge condition ∇ · Af = 0. The equation f (x, t) = − ∇ · A(x, t)
 
 (18.10)
 
 can be solved with the Green’s function G(r) = (4π r)−1 for the Laplace operator, 
 
 1 = − δ(x − x  ), 4π |x − x  |
 
 see Eqs. (11.14) and (11.24) for E = 0. This yields
 
 (18.11)
 
 18.1 Lagrange Density and Mode Expansion for the Maxwell Field
 
 f (x, t) =
 
 1 4π
 
 
 
 d 3x
 
 1 ∇ · A(x  , t). |x − x  |
 
 433
 
 (18.12)
 
 This gauge is denoted as Coulomb gauge. We denote the gauge transformed fields again with  and A, i.e. we have ∇ · A(x, t) = 0.
 
 (18.13)
 
 and  = −
 
 1 , 0
 
 (18.14)
 
 1 ∂2 1 ∂ A − A + 2 ∇ = μ0 j . c2 ∂t 2 c ∂t
 
 (18.15)
 
 W		
Data Loading...
 
	 
	 
	 
	 
	 
	 
	 
	 
	 
	 
	