Abstract
The aim of this first chapter is to present the physics framework of electromagnetism, in relation to the main sets of equations, that is, Maxwell’s equations and some related approximations. In that sense, it is neither a purely physical nor a purely mathematical point of view. The term model might be more appropriate: sometimes, it will be necessary to refer to specific applications in order to clarify our purpose, presented in a selective and biased way, as it leans on the authors’ personal view. This being stated, this chapter remains a fairly general introduction, including the foremost models in electromagnetics. Although the choice of such applications is guided by our own experience, the presentation follows a natural structure.
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Notes
- 1.
Unless otherwise specified, in this chapter, a domain is an open region of space. Another meaning is given for the mathematical studies, starting in Chap. 2.
- 2.
H is sometimes called the magnetizing field.
- 3.
The standard differential operators , div, \( \operatorname {\mathrm {\mathbf {grad}}}\), and Δ are mathematically defined in Sect. 1.5.1.
- 4.
By definition, δ Σ is the surface Dirac mass on Σ, so one has \(\int \varrho v = \int _\varSigma \sigma _\varSigma v_{|\varSigma } \,dS\) for ad hoc functions v.
- 5.
See the end of the section.
- 6.
By definition, \(\delta _{{\boldsymbol {x}}_0}\) is the Dirac mass in x 0, so one has \(\int \varrho _0 v = q_0 v({\boldsymbol {x}}_0)\) for ad hoc functions v.
- 7.
Or: electrostatically.
- 8.
To deserve the label fixed frequency problem, one assumes a non-vanishing value of the pulsation. Otherwise, one solves a static problem, cf. Sect. 1.4.1.
- 9.
The fields and are respectively called electric and magnetic polarizations .
- 10.
Other conditions on lead to the same conclusion. For instance, if is a real-valued, even function of ω that can be expressed as a rational fraction, with decaying condition for large |ω|.
- 11.
In particular, this is the case for the Lorentz force (1.75). As a matter of fact, div v F(t, x, v) = q (div v E + div v (v ×B)) = 0, since the electromagnetic fields are independent of v in the phase space.
- 12.
- 13.
It can happen that, in Maxwell’s equations, parts of ϱ and J are due to external charge and current sources. In this case, E and B depend in an affine way on f.
- 14.
Id est, consider \(f_\alpha ({\boldsymbol {v}})\approx A_\alpha \exp (-B_\alpha |{\boldsymbol {v}}-\boldsymbol {u}_\alpha |{ }^2)\), with A α , B α > 0.
- 15.
See the upcoming Sect. 1.5 for a precise definition.
- 16.
More precisely, ω is a pulsation and the corresponding frequency is ω∕(2π).
- 17.
One may also use the interface conditions to describe electromagnetic fields globally in \(\mathbb {R}^3\): this is an integral representation. More precisely [167, §5.5], consider that \(\mathbb {R}^3\) is split into two media M + and M −, one of them being bounded, and let Σ be the interface between the two media. If one is interested in the electromagnetic fields that are governed by the homogeneous time-harmonic equations in M + and M −, then, assuming that the jump j Σ = −[H ×n Σ ] Σ (condition (1.12 right)) is known, one can use integral representation formulas for the values of E(x) and H(x), for all \({\boldsymbol {x}}\in \mathbb {R}^3\setminus \varSigma \). The integrals are taken over Σ and depend only on j Σ . In the same spirit, one can represent the (different) values of E ±(x Σ ) and H ±(x Σ ) for all x Σ ∈ Σ. Within this framework, one may generalize these results in the presence of magnetic polarization by assuming that the magnetic current on Σ, m Σ = [E ×n Σ ] Σ , is also different from 0. In this case, one ends up with integral representation formulas of E and H, with integrals over Σ that depend on j Σ and m Σ . In the same manner, one may use the jump relation σ Σ = [D ⋅n Σ ] Σ (1.11 left) to solve a diffraction problem expressed as a scalar Helmholtz equation, assuming σ Σ is known, where the unknown is the scalar electric potential.
- 18.
Instead of B(O, R), one can choose any reasonable volume in which the computations ought to be performed: a cube, as in Fig. 1.3 (right, rightmost Γ A ), etc.
- 19.
For instance (see [187]), if the artificial boundary Γ A is a cylinder of radius R and axis Oz, one gets
with E = E r e r + E θ e θ + E z e z in cylindrical coordinates.
- 20.
Manipulating Maxwell’s equations thusly is certainly admissible, since one is dealing with artificial media, in which the electromagnetic fields are artifacts…
- 21.
Indeed, the unit outward normal vector to ∂B(O, R) is n = e r . Moreover, since x = r e r on ∂B(O, R), for an outgoing plane wave that propagates normally to ∂B(O, R) (k out = k e r ), one finds k out ⋅x = kr. Respectively, for an incoming plane wave that propagates normally to ∂B(O, R) (k in = −k e r ), k in ⋅x = −kr.
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Assous, F., Ciarlet, P., Labrunie, S. (2018). Physical Framework and Models. In: Mathematical Foundations of Computational Electromagnetism. Applied Mathematical Sciences, vol 198. Springer, Cham. https://doi.org/10.1007/978-3-319-70842-3_1
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