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Towards a covariant formulation of electromagnetic wave polarization

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2.2. GENERALIZED STOKES PARAMETERS 11<br />

2.2 Generalized Stokes parameters<br />

In this Section we give the definitions <strong>of</strong> the two-dimensional Stokes parameters<br />

and the generalized <strong>polarization</strong> parameters introduced by T. Carozzi, R. Karlsson<br />

and J. Bergman [6]. These <strong>polarization</strong> parameters are a generalization <strong>of</strong><br />

the Stokes parameters into three-dimensions. A similar set <strong>of</strong> parameters were<br />

introduced by Brosseau [5]. The Poynting vector and the Maxwell stress tensor<br />

are introduced and defined. Storey and Lefeuvre’s [23] six dimensional <strong>electromagnetic</strong><br />

quasi-vector and their representation <strong>of</strong> the quadratic quantities <strong>of</strong> an<br />

<strong>electromagnetic</strong> field are also discussed.<br />

2.2.1 Spectral density matrix<br />

Consider an arbitrary vector field, ⃗ f(⃗r, t). The field is a superposition <strong>of</strong> all<br />

<strong>wave</strong>s and stationary fields at the point ⃗r. The spectral components <strong>of</strong> the field<br />

⃗f(⃗r, t), one obtains by taking the Fourier transform, ⃗ F (⃗r, ω), <strong>of</strong> the field, defined<br />

as<br />

⃗F (⃗r, ω) =<br />

∫ ∞<br />

−∞<br />

⃗f(⃗r, t)e iωt dt. (2.46)<br />

The vector, ⃗ F , represents a complex valued vector field which can be separated<br />

into three complex amplitudes (the x, y, z components), or into three real<br />

amplitudes (F 1 , F 2 , F 3 ) and their real phases (δ 1 , δ 2 , δ 3 ), in the following way<br />

⎛<br />

⃗F (⃗r, ω) = ⎝ F ⎞ ⎛<br />

⎞<br />

x(⃗r, ω) F 1 (⃗r, ω)e δ1(⃗r,ω)<br />

F y (⃗r, ω) ⎠ = ⎝F 2 (⃗r, ω)e δ2(⃗r,ω) ⎠ . (2.47)<br />

F z (⃗r, ω) F 3 (⃗r, ω)e δ3(⃗r,ω)<br />

The spectral density matrix, S d (⃗r, ω), is constructed by taking the tensor product<br />

between F ⃗ = F ⃗ (⃗r, ω), and its Hermitian conjugate, F ⃗ † = F ⃗ † (⃗r, ω). This<br />

gives<br />

⎛<br />

⎞<br />

S d (⃗r, ω) = F ⃗ ⊗ F ⃗ F x F † x ∗ F x Fy ∗ F x Fz<br />

∗<br />

= ⎝F y Fx ∗ F y Fy ∗ F y Fz<br />

∗ ⎠ , (2.48)<br />

F z Fx ∗ F z Fy ∗ F z Fz<br />

∗<br />

where F ∗ denotes complex conjugate. We will assume (⃗r, ω)-dependence and<br />

the notation S d = S d (⃗r, ω) will be used in the following.<br />

2.2.2 Instantaneous Stokes’ parameters<br />

Stokes’ parameters describe the <strong>polarization</strong> state <strong>of</strong> a transverse <strong>electromagnetic</strong><br />

<strong>wave</strong> in the <strong>polarization</strong> plane. One usually assumes that the <strong>wave</strong> propagates<br />

in the z-direction and the <strong>polarization</strong> ellipse lies in the xy-plane (see<br />

Brosseau [4]). Stokes parameters can be written (using the notation 11 <strong>of</strong> R.<br />

11 The notation for Stokes’ parameters is not universal. The notation <strong>of</strong> Stokes [22] was<br />

(A,B,C,D), another notation is (S 0 , S 1 , S 2 , S 3 ) used by e.g. Jackson [12] and Brosseau [4].

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