introductiontotheelectromagnetictheory · q electriccharge[c] ˆ electricchargedensity[c/m3] j =...
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Introduction to the Electromagnetic Theory
Andrea Latina (CERN)[email protected]
Basics of Accelerator Physics and Technology
7-11 October 2019, Archamps, France
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Table of contents
I Introduction
I ElectrostaticsI E.g. Space-charge forces
I MagnetostaticsI E.g. Accelerator magnets
I Non-static caseI E.g. RF acceleration and wave guides
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Part 1.
Introduction:
Maxwell’s Equations
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Motivation: control of charged particle beamsTo control a charged particle beam we use electromagnetic fields. Recall theLorentz force:
~F = q ·(~E + ~v × ~B
)where, in high energy machines, |~v | ≈ c ≈ 3 · 108 m/s. In particle accelerators,transverse deflection is usually given by magnetic fields, whereas acceleration canonly be given by electric fields.
Comparison of electric and magnetic force:∣∣∣~E ∣∣∣ = 1 MV/m∣∣∣~B∣∣∣ = 1 T
Fmagnetic
Felectric=
evBeE
=βcBE
' β3 · 108
106= 300β
⇒ the magnetic force is much stronger then the electric one: in an accelerator, usemagnetic fields whenever possible.
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Some references
1. Richard P. Feynman, Lectures on Physics, 1963, on-line
2. J. D. Jackson, Classical Electrodynamics, Wiley, 1998
3. David J. Griffiths, Introduction to Electrodynamics, Cambridge University Press, 2017
4. Thomas P. Wangler, RF Linear Accelerators, Wiley, 2008
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Variables and units
E electric field [V/m]B magnetic field [T]D electric displacement [C/m2]H magnetizing field [A/m]
q electric charge [C]ρ electric charge density [C/m3]j = ρv current density [A/m2]
ε0 permittivity of vacuum, 8.854 · 10−12 [F/m]µ0 = 1
ε0c2permeability of vacuum, 4π · 10−7 [H/m or N/A2]
c speed of light in vacuum, 2.99792458 · 108 [m/s]
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Differentiation with vectors
I We define the operator “nabla”:
∇ def=
(∂∂x ,
∂∂y ,
∂∂z
)which we treat as a special vector.
I Examples:
∇ · F =∂Fx
∂x+∂Fy
∂y+∂Fz
∂zdivergence
∇× F =(∂Fz∂y −
∂Fy∂z ,
∂Fx∂z −
∂Fz∂x ,
∂Fy∂x −
∂Fx∂y
)curl
∇φ =(∂φ∂x ,
∂φ∂y ,
∂φ∂z
)gradient
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Maxwell’s equations: integral form
1. Maxwell’s equations can be written in integral or in differential form (SIunits convention):
(1) Gauss’ law;(2) Gauss’ law for magnetism;(3) Maxwell–Faraday equation (Faraday’s law of induction);(4) Ampère’s circuital law
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Maxwell’s equations: differential form
1. Maxwell’s equations can be written in integral or in differential form (SIunits convention):
(1) Gauss’ law;(2) Gauss’ law for magnetism;(3) Maxwell–Faraday equation (Faraday’s law of induction);(4) Ampère’s circuital law
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Part 2.
Electromagnetism:
Static case
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Static case
I We will consider relatively simple situations.I The easiest circumstance is one in which nothing depends on the time—this is
called the static case:I All charges are permanently fixed in space, or if they do move, they move as
a steady flow in a circuit (so ρ and j are constant in time).I In these circumstances, all of the terms in the Maxwell equations which are time
derivatives of the field are zero. In this case, the Maxwell equations become:
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Electrostatics: principle of superposition
I Coulomb’s Law: Electric field due to a stationary point charge q, located in r1:
E (r) =q
4πε0r − r1|r − r1|3
I Principle of superposition, tells that a distribution of charges qi generates anelectric field:
E (r) =1
4πε0
∑qi
r − ri|r − ri |3
I Continuous distribution of charges, ρ (r)
E (r) =1
4πε0
˚Vρ(r′) r − r′
|r − r′|3dr
with Q =˝
V ρ (r′) dr as the total charge, and where ρ is the charge density.
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Recall: Gauss’ theorem
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Electrostatics: Gauss’ lawGauss’ law states that the flux of ~E is:
¨A
~E ·d~A=ˆ
any closedsurface A
En da=sum of charges inside A
ε0
We know that
E (r) =1
4πε0
˚Vρ(r′) r − r′
|r − r′|3dr
In differential form, using the Gauss’ theorem (diver-gence theorem):¨
~E · d~A =
˚∇ · ~E dr
which gives the first Maxwell’s equation in differentialform:
∇ · ~E=ρ
ε0
Example: case of a single point charge
¨~E · d~A =
{qε0
if q lies inside A
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Electrostatics: Gauss’ law
The flux of E out of the surface S is zero.
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Electrostatics: scalar potential and Poisson equationThe equations for electrostatics are:
∇ · ~E =ρ
ε0
∇× ~E = 0
The two can be combined into a single equation:
~E=-∇φ
which leads to the Poisson’s equation:
∇ · ∇φ = ∇2φ=-ρ
ε0
Where the operator ∇2 is called Laplacian:
∇ · ∇ = ∇2 =∂2
∂x2+
∂2
∂y2+
∂2
∂z2
The Poisson’s equation allows to compute the electric field generated by arbitrarycharge distributions.
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Electrostatics: Poisson’s equation∇2φ = −
ρ
ε0(∂2
∂x2+
∂2
∂y2+
∂2
∂z2
)φ = −
ρ
ε0
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Recall: Stokes’ theorem
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Magnetostatics: Ampère’s and Biot-Savart laws
The equations for electrostatics are:
∇ · ~B = 0
∇× ~B =~jε0c2
The Stokes’ theorem tells that:˛C
~B · d~r =
¨A
(∇× ~B
)· d~A
This equation gives the Ampère’s law:˛C
~B · d~r =1ε0c2
¨A
~j · ~n dA
From which one can derive the Biot-Savart law, stating that, along a current j :
~B (~r) =1
4πε0c2 =
˛C
j d~r ′ × (~r −~r ′)|~r −~r ′|3
This provides a practical way to compute ~B from current distributions.
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Magnetostatics: vector potential
The equations for electrostatics are:
∇ · ~B = 0
∇× ~B =~jε0c2
They can be unified into one, introducing the vector potential ~A:
~B = ∇× ~A
Using the Stokes’ theorem
~B (~r) =1
4πε0c2 =
˛C
j d~r ′ × (~r −~r ′)|~r −~r ′|3
one can derive the expression of the vector potential ~A from of the current ~j :
~A (r) =µ04π
˚ ~j (~r ′)|~r −~r ′|d
3~r ′
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Summary of electro- and magneto- statics
One can compute the electric and the magnetic fields from the scalar and the vectorpotentials
~E = −∇φ~B = ∇× ~A
with
φ (r) =1
4πε0
˚ρ (~r ′)|~r −~r ′|d
3~r ′
~A (r) =µ04π
˚ ~j (~r ′)|~r −~r ′|d
3~r ′
being ρ the charge density, and ~j the current density.
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Motion of a charged particle in an electric field
~F = q ·(~E + ~v ×��SS~B
)
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Motion of a charged particle in a magnetic field
~F = q ·(��SS~E + ~v × ~B
)
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Part 3.
Electromagnetism:
Non-static case
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Magnetostatics: Faraday’s law of induction
“The electromotive force around a closed path is equal to the negative of the time rateof change of the magnetic flux enclosed by the path.”
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Non-static case: electromagnetic wavesElectromagnetic wave equation:
~E (~r , t) = ~E0e i(ωt−~k·~r)
~B (~r , t) = ~B0e i(ωt−~k·~r)
Important quantities:
∣∣∣~k∣∣∣ = 2πλ
=ω
cwave-number vector
λ =cf
wave length
f frequency
ω = 2πf angular frequency
Magnetic and electric fields are transverse to direction of propagation:
~E ⊥ ~B ⊥ ~k
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Spectrum of electromagnetic waves
Examples:I yellow light ≈ 5 · 1014 Hz (i.e. ≈ 2 eV !)I LEP (SR) ≤ 2 · 1020 Hz (i.e. ≈ 0.8 MeV !)I gamma rays ≤ 3 · 1021 Hz (i.e. ≤ 12 MeV !)
(For estimates using temperature: 3 K ≈ 0.00025 eV )
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Electromagnetic waves impacting highly conductivematerials
Highly conductive materials: RF cavities, wave guides.
I In an ideal conductor:~E‖ = 0, ~B⊥ = 0
I This implies:I All energy of an electromagnetic wave is reflected from the surface of an
ideal conductor.
I Fields at any point in the ideal conductor are zero.
I Only some field patterns are allowed in waveguides and RF cavities.
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Example: RF cavities and wave guides
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Example: Fields in RF cavities
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Example: Consequences for RF cavities
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Example: Consequences for wave guides
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Classification of modes
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Classification of modes
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...The End!
Thank you
for your attention!
Special thanks to Werner Herr, for the pictures I took from his slides.37/37 A. Latina - Electromagnetic Theory