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Exercicios de Eletromagnetismo, Exercícios de Engenharia Elétrica

Exercicios do livro do Bo Thidé

Tipologia: Exercícios

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Draft version released 15th November 2000 at 20:39
Downloaded from http://www.plasma.uu.se/CED/Exercises
Tobia Carozzi Anders Eriksson Bengt Lundborg Bo Thidé Mattias Waldenvik
ELECTROMAGNETIC FIELD THEORY
EXERCISES
PLEASE NOTE THAT THIS IS A
VERY PRELIMINARY DRAFT!
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Draft version released 15th November 2000 at 20:

Downloaded from http://www.plasma.uu.se/CED/Exercises

Tobia Carozzi Anders Eriksson Bengt Lundborg Bo Thidé Mattias Waldenvik

ELECTROMAGNETIC FIELD THEORY

EXERCISES

PLEASE NOTE THAT THIS IS A

VERY PRELIMINARY DRAFT!

Companion volume to

ELECTROMAGNETIC FIELD THEORY

by

Bo Thidé

This book was typeset in LATEX 2 ε on an HP9000/700 series workstation and printed on an HP LaserJet 5000GN printer.

Copyright c

(^) 1998 by Bo Thidé Uppsala, Sweden All rights reserved.

Electromagnetic Field Theory Exercises

ISBN X-XXX-XXXXX-X

CONTENTS

Draft version released 15th November 2000 at 20:39 vi

PREFACE

This is a companion volume to the book Electromagnetic Field Theory by Bo Thidé.

The problems and their solutions were created by the co-authors who all have

taught this course or its predecessor.

It should be noted that this is a preliminary draft version but it is being corrected

and expanded with time.

Uppsala, Sweden B. T.

December, 1999

Draft version released 15th November 2000 at 20:39 vii

LESSON 1

Maxwell’s Equations

1.1 Coverage

In this lesson we examine Maxwell’s equations, the cornerstone of electrodynam-

ics. We start by practising our math skill, refreshing our knowledge of vector

analysis in vector form and in component form.

1.2 Formulae used

E  ρ ε 0 (1.1a)

B  0 (1.1b)

E 

∂ t

B (1.1c)

B  μ 0 j

c^2

∂ t

E (1.1d)

1.3 Solved examples

MACROSCOPIC MAXWELL EQUATIONS EXAMPLE 1.

The most fundamental form of Maxwell’s equations is

E  ρ ε 0 (1.2a)

B  0 (1.2b)

E 

t B (1.2c)

B  μ 0 j 

c^2

t

E (1.2d)

Draft version released 15th November 2000 at 20:39 1

2 LESSON 1. MAXWELL’S EQUATIONS

sometimes known as the microscopic Maxwell equations or the Maxwell-Lorentz equa- tions. In the presence of a medium, these equations are still true, but it may sometimes be convenient to separate the sources of the fields (the charge and current densities) into an induced part, due to the response of the medium to the electromagnetic fields, and an extraneous, due to “free” charges and currents not caused by the material properties. One then writes

j  j ind  j ext (1.3)

ρ  ρind  ρext (1.4)

The electric and magnetic properties of the material are often described by the electric polarisation P (SI unit: C/m^2 ) and the magnetisation M (SI unit: A/m). In terms of these, the induced sources are described by

j ind  ∂ P ∂ t 

M (1.5)

ρind 

P (1.6)

To fully describe a certain situation, one also needs constitutive relations telling how P and M depends on E and B. These are generally empirical relations, different for different media.

Show that by introducing the fields

D  ε 0 E  P (1.7)

H  B  μ 0  M (1.8)

the two Maxwell equations containing source terms (1.2a) and ( ?? ) reduce to

D  ρext (1.9)

H  j ext 

t

D (1.10)

known as the macroscopic Maxwell equations.

Solution

If we insert

j  j ind  j ext (1.12)

ρ  ρind  ρext (1.13)

and

Draft version released 15th November 2000 at 20:

4 LESSON 1. MAXWELL’S EQUATIONS

EXAMPLE 1.2^ MAXWELL’S EQUATIONS IN COMPONENT FORM

Express Maxwell’s equations in component form.

Solution

Maxwell’s equations in vector form are written:

E  ρ ε 0 (1.27)

B  0 (1.28)

E 

t

B (1.29)

B  μ 0 j 

c^2

t

E (1.30)

In these equations, E , B , and j are vectors, while ρ is a scalar. Even though all the equations contain vectors, only the latter pair are true vector equations in the sense that the equations themselves have several components. When going to component notation, all scalar quantities are of course left as they are.

Vector quantities, for example E , can always be expanded as E  ∑^3 j & 1 E j x ˆ j  E j x ˆ j ,

where the last step assumes Einstein’s summation convention: if an index appears twice in the same term, it is to be summed over. Such an index is called a summation index. Indices which only appear once are known as free indices, and are not to be summed over. What

symbol is used for a summation index is immaterial: it is always true that aibi  akbk ,

since both these expressions mean a 1 b 1  a 2 b 2  a 3 b 3  a

b. On the other hand, the

expression ai  ak is in general not true or even meaningful, unless i  k or if a is the null

vector. The three E (^) j are the components of the vector E in the coordinate system set by the three unit vectors x ˆ (^) j. The E (^) j are real numbers, while the x ˆ (^) j are vectors, i.e. geometrical objects. Remember that though they are real numbers, the E (^) j are not scalars. Vector equations are transformed into component form by forming the scalar product of both sides with the same unit vector. Let us go into ridiculous detail in a very simple case:

G  H (1.31)

G

x ˆ k  H

x ˆ k (1.32)

 G^ j x ˆ^ j 

x ˆ k   Hi x ˆ i 

x ˆ k (1.33)

G j δ jk  Hi δ ik (1.34)

Gk  Hk (1.35)

This is of course unnecessarily tedious algebra for an obvious result, but by using this careful procedure, we are certain to get the correct answer: the free index in the resulting equation necessarily comes out the same on both sides. Even if one does not follow this complicated way always, one should to some extent at least think in those terms. Nabla operations are translated into component form as follows:

Draft version released 15th November 2000 at 20:

1.3. SOLVED EXAMPLES 5

∇ φ  x ˆ i

xi

∂ φ ∂ xi

V 

xi

Vi ('

Vixi

V  ε i jk x ˆ i

x (^) j

Vk (' ε i jk

Vkx (^) j

where V is a vector field and φ is a scalar field.

Remember that in vector valued equations such as Ampère’s and Faraday’s laws, one must be careful to make sure that the free index on the left hand side of the equation is the same as the free index on the right hand side of the equation. As said above, an equation of the

form Ai  B j is almost invariably in error!

With these things in mind we can now write Maxwell’s equations as

E 

ρ ε 0

Eixi

ρ ε 0

B  0 )'

Bixi

E *

∂ B

t

)' ε i jk

Ekx (^) j

t

Bi (1.41)

B  μ 0 j 

c^2

∂ E

t

)' ε i jk

Bkx (^) j

μ 0 ji 

c^2

Eit

END OF EXAMPLE 1.2 %

THE CHARGE CONTINUITY EQUATION EXAMPLE 1.

Derive the continuity equation for charge density ρ from Maxwell’s equations using (a) vector notation and (b) component notation. Compare the usefulness of the two systems of notations. Also, discuss the physical meaning of the charge continuity equation.

Solution

Vector notation In vector notation, a derivation of the continuity equation for charge

looks like this:

Compute

t E^ in two ways:

  1. Apply ∂^ ∂ t to Gauss’s law:

∂ t 

E +

ε 0

t

ρ (1.43)

Draft version released 15th November 2000 at 20:

1.3. SOLVED EXAMPLES 7

Comparing the two notation systems We notice a few points in the derivations

above:

It is sometimes difficult to see what one is calculating in the component system. The vector system with div, curl etc. may be closer to the physics, or at least to our picture of it.

2 In the vector notation system, we sometimes need to keep some vector formulas in

memory or to consult a math handbook, while with the component system you need only the definitions of ε i jk and δ i j.

2 Although not seen here, the component system of notation is more explicit (read

unambiguous) when dealing with tensors of higher rank, for which vector notation becomes cumbersome.

2 The vector notation system is independent of coordinate system, i.e. , ∇ φ is ∇ φ in

any coordinate system, while in the component notation, the components depend on the unit vectors chosen.

Interpreting the continuity equation The equation

t

j  0 (1.51)

is known as a continuity equation. Why? Well, integrate the continuity equation over some volume V bounded by the surface S. By using Gauss’s theorem, we find that

d Q d t

V

t

ρ d^3 x 

V

j d^3 x 

S

j

d S (1.52)

which says that the change in the total charge in the volume is due to the net inflow of electric current through the boundary surface S. Hence, the continuity equation is the field theory formulation of the physical law of charge conservation.

END OF EXAMPLE 1.3 %

Draft version released 15th November 2000 at 20:

  • 1 Maxwell’s Equations Preface vii
    • 1.1 Coverage
    • 1.2 Formulae used
    • 1.3 Solved examples
      • Example 1.1 Macroscopic Maxwell equations
      • Solution
      • Example 1.2 Maxwell’s equations in component form
      • Solution
      • Example 1.3 The charge continuity equation
      • Solution
  • 2 Electromagnetic Potentials and Waves
    • 2.1 Coverage
    • 2.2 Formulae used
    • 2.3 Solved examples
      • Example 2.1 The Aharonov-Bohm effect
      • Solution
      • Example 2.2 Invent your own gauge
      • Solution
      • Example 2.3 Fourier transform of Maxwell’s equations
      • Solution
      • Example 2.4 Simple dispersion relation
      • Solution
  • 3 Relativistic Electrodynamics
    • 3.1 Coverage
    • 3.2 Formulae used ii
    • 3.3 Solved examples
      • Example 3.1 Covariance of Maxwell’s equations
      • Solution
      • Example 3.2 Invariant quantities constructed from the field tensor
      • Solution - ics formulas Example 3.3 Covariant formulation of common electrodynam-
      • Solution - transformation Example 3.4 Fields from uniformly moving charge via Lorentz
      • Solution
  • 4 Lagrangian and Hamiltonian Electrodynamics
    • 4.1 Coverage
    • 4.2 Formulae used
    • 4.3 Solved examples
      • Example 4.1 Canonical quantities for a particle in an EM field
      • Solution
      • Example 4.2 Gauge invariance of the Lagrangian density
      • Solution
  • 5 Electromagnetic Energy, Momentum and Stress
    • 5.1 Coverage
    • 5.2 Formulae used
    • 5.3 Solved examples
      • Example 5.1 EM quantities potpourri
      • Solution
      • Example 5.2 Classical electron radius
      • Solution
      • Example 5.3 Solar sailing
      • Solution
      • Example 5.4 Magnetic pressure on the earth
      • Solution
  • 6 Radiation from Extended Sources
    • 6.1 Coverage
    • 6.2 Formulae used
    • 6.3 Solved examples
      • Example 6.1 Instantaneous current in an infinitely long conductor
        • Draft version released 15th November 2000 at 20:
      • Solution iii
      • Example 6.2 Multiple half-wave antenna
      • Solution
      • Example 6.3 Travelling wave antenna
      • Solution
      • Example 6.4 Microwave link design
      • Solution
  • 7 Multipole Radiation
    • 7.1 Coverage
    • 7.2 Formulae used
    • 7.3 Solved examples
      • Example 7.1 Rotating Electric Dipole
      • Solution
      • Example 7.2 Rotating multipole
      • Solution
      • Example 7.3 Atomic radiation
      • Solution
      • Example 7.4 Classical Positronium
      • Solution
  • 8 Radiation from Moving Point Charges
    • 8.1 Coverage
    • 8.2 Formulae used
    • 8.3 Solved examples
      • Example 8.1 Poynting vector from a charge in uniform motion
      • Solution - eration Example 8.2 Synchrotron radiation perpendicular to the accel-
      • Solution
      • Example 8.3 The Larmor formula
      • Solution
      • Example 8.4 Vavilov- ˇCerenkov emission
      • Solution
  • 9 Radiation from Accelerated Particles
    • 9.1 Coverage
    • 9.2 Formulae used
    • 9.3 Solved examples - Draft version released 15th November 2000 at 20:
    • EM fields Example 9.1 Motion of charged particles in homogeneous static
  • Solution
  • Example 9.2 Radiative reaction force from conservation of energy
  • Solution
  • Example 9.3 Radiation and particle energy in a synchrotron
  • Solution
  • Example 9.4 Radiation loss of an accelerated charged particle
  • Solution
  • Draft version released 15th November 2000 at 20:39