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1.3 ELECTRODYNAMICS

13

dS

v

B(x)

v

C

dl

B(x)

FIGURE 1.4: A loop C which moves with velocity v in a spatially varying magnetic field B(x) will sense a varying magnetic flux during the motion.

where m is the magnetic flux and S is the surface encircled by C which can be interpreted as a generic stationary “loop” and not necessarily as a conducting circuit. Application of Stokes' theorem on this integral equation, transforms it into the differential equation

r E(t;x) =

@

 

@t B(t;x)

(1.32)

which is valid for arbitrary variations in the fields and constitutes the Maxwell equation which explicitly connects electricity with magnetism.

Any change of the magnetic flux m will induce an EMF. Let us therefore consider the case, illustrated if Figure 1.3.4, that the “loop” is moved in such a way that it links a magnetic field which varies during the movement. The convective derivative is evaluated according to the well-known operator formula

d

=

@

+v r

(1.33)

dt

@t

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14

CLASSICAL ELECTRODYNAMICS

which follows immediately from the rules of differentiation of an arbitrary differentiable function f (t;x(t)). Applying this rule to Faraday's law, Equation (1.31) on page 12, we obtain

E(t;x) = dt ZS dS B = ZS dS

@t

ZS dS (v r)B

(1.34)

 

d

@B

 

 

During spatial differentiation v is to be considered as constant, and Equation (1.17) on page 8 holds also for time-varying fields:

r B(t;x) = 0

(1.35)

(it is one of Maxwell's equations) so that, according to Formula (F.59) on page 166,

r (B v) = (v r)B

allowing us to rewrite Equation (1.34) in the following way:

E(t;x) = I dl EEMF = d Z dS B

C dt S

= Z dS @B Z dS r (B v)

S @t S

With Stokes' theorem applied to the last integral, we finally get

E(t;x) = I dl EEMF = Z dS @B I dl (B v)

C S @t C

or, rearranging the terms,

Z Z

dl (EEMF v B) = dS @B

C S @t

(1.36)

(1.37)

(1.38)

(1.39)

where EEMF is the field which is induced in the “loop,” i.e., in the moving system. The use of Stokes' theorem “backwards” on Equation (1.39) above yields

r (EEMF v B) =

@B

 

(1.40)

@t

In the fixed system, an observer measures the electric field

 

E = EEMF v B

 

 

(1.41)

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1.3 ELECTRODYNAMICS

15

Hence, a moving observer measures the following Lorentz force on a charge q

qEEMF = qE +q(v B)

(1.42)

corresponding to an “effective” electric field in the “loop” (moving observer)

EEMF = E +(v B)

(1.43)

Hence, we can conclude that for a stationary observer, the Maxwell equation

r E =

@B

(1.44)

@t

is indeed valid even if the “loop” is moving.

1.3.5 Maxwell's microscopic equations

We are now able to collect the results from the above considerations and formulate the equations of classical electrodynamics valid for arbitrary variations in time and space of the coupled electric and magnetic fields E(t;x) and B(t;x). The equations are

r E

r E r B r B

(t;x)

= "0

= @B

@t

= 0

@E

= "0 0 @t + 0j(t;x)

(1.45a)

(1.45b)

(1.45c)

(1.45d)

In these equations (t;x) represents the total, possibly both time and space dependent, electric charge, i.e., free as well as induced (polarisation) charges, and j(t;x) represents the total, possibly both time and space dependent, electric current, i.e., conduction currents (motion of free charges) as well as all atomistic (polarisation, magnetisation) currents. As they stand, the equations therefore incorporate the classical interaction between all electric charges and currents in the system and are called Maxwell's microscopic equations. Another name often used for them is the Maxwell-Lorentz equations. Together with the appropriate constitutive relations, which relate and j to the fields, and the initial and boundary conditions pertinent to the physical situation at hand, they form a system of well-posed partial differential equations which completely determine E and B.

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CLASSICAL ELECTRODYNAMICS

1.3.6 Maxwell's macroscopic equations

The microscopic field equations (1.45) provide a correct classical picture for arbitrary field and source distributions, including both microscopic and macroscopic scales. However, for macroscopic substances it is sometimes convenient to introduce new derived fields which represent the electric and magnetic fields in which, in an average sense, the material properties of the substances are already included. These fields are the electric displacement D and the magnetising field H. In the most general case, these derived fields are complicated nonlocal, nonlinear functionals of the primary fields E and B:

D = D[t;x; E;B]

(1.46a)

H = H[t;x; E;B]

(1.46b)

Under certain conditions, for instance for very low field strengths, we may assume that the response of a substance to the fields is linear so that

D = "E

(1.47)

H = 1B

(1.48)

i.e., that the derived fields are linearly proportional to the primary fields and that the electric displacement (magnetising field) is only dependent on the electric (magnetic) field.

The field equations expressed in terms of the derived field quantities D and H are

r D = (t;x)

r E = @B

@t

r B = 0

@D

r H = @t +j(t;x)

(1.49a)

(1.49b)

(1.49c)

(1.49d)

and are called Maxwell's macroscopic equations. We will study them in more detail in Chapter 6.

1.4 Electromagnetic Duality

If we look more closely at the microscopic Maxwell equations (1.45), we see that they exhibit a certain, albeit not a complete, symmetry. Let us follow Dirac

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1.4 ELECTROMAGNETIC DUALITY

17

and make the ad hoc assumption that there exist magnetic monopoles represented by a magnetic charge density, which we denote by m = m(t;x), and a magnetic current density, which we denote by jm = jm(t;x). With these new quantities included in the theory, and with the electric charge density denotede and the electric current density denoted je, the Maxwell equations will be symmetrised into the following four coupled, vector, partial differential equations:

r E =

e

 

 

 

 

 

 

 

 

 

 

 

(1.50a)

"0

 

 

 

 

 

 

 

 

 

 

 

 

r E =

@B

 

0jm

 

(1.50b)

 

 

 

@t

 

r B = 0 m =

1 m

 

(1.50c)

c2

 

"0

 

1 @E

 

r B = "0 0

@E

+ 0je =

+ 0je

(1.50d)

 

 

 

 

 

@t

c2

@t

We shall call these equations Dirac's symmetrised Maxwell equations or the electromagnetodynamic equations.

Taking the divergence of (1.50b), we find that

r (r E) =

@

(r B) 0r jm 0

(1.51)

@t

where we used the fact that, according to Formula (M.95) on page 187, the divergence of a curl always vanishes. Using (1.50c) to rewrite this relation, we obtain the equation of continuity for magnetic monopoles

@m

+r jm = 0

(1.52)

@t

which has the same form as that for the electric monopoles (electric charges) and currents, Equation (1.23) on page 10.

We notice that the new Equations (1.50) exhibit the following symmetry (recall that "0 0 = 1=c2):

E ! cB

(1.53a)

cB !E

(1.53b)

c e ! m

(1.53c)

m !c e

(1.53d)

cje ! jm

(1.53e)

jm !cje

(1.53f)

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CLASSICAL ELECTRODYNAMICS

which is a particular case ( = =2) of the general duality transformation (depicted by the Hodge star operator)

?E = Ecos +cBsin

(1.54a)

c?B = Esin +cBcos

(1.54b)

c? e = c e cos + m sin

(1.54c)

? m = c e sin + m cos

(1.54d)

c?je = cje cos +jm sin

(1.54e)

?jm = cje sin +jm cos

(1.54f)

which leaves the symmetrised Maxwell equations, and hence the physics they describe (often referred to as electromagnetodynamics), invariant. Since E and je are (true or polar) vectors, B a pseudovector (axial vector), e a (true) scalar, then m and , which behaves as a mixing angle in a two-dimensional “charge space,” must be pseudoscalars and jm a pseudovector.

EXAMPLE 1.1 BFARADAY'S LAW AS A CONSEQUENCE OF CONSERVATION OF MAGNETIC CHARGE

Postulate 1.1 (Indestructibility of magnetic charge). Magnetic charge exists and is indestructible in the same way that electric charge exists and is indestructible. In other words we postulate that there exists an equation of continuity for magnetic charges:

@m(t;x) +r jm(t;x) =0

@t

Use this postulate and Dirac's symmetrised form of Maxwell's equations to derive

Faraday's law.

The assumption of the existence of magnetic charges suggests a Coulomb-like law for magnetic fields:

Bstat(x) = 40

ZV0d3x0

m(x0)

x x00

3

=

40

ZV0d3x0

m(x0)r x

1

x0

 

 

 

 

 

 

 

 

x

x

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

j

 

 

 

j

 

 

 

 

 

 

 

j

 

 

j

=

0

rZV0d3x0 m(x0)

 

 

1

 

 

 

 

 

 

 

 

 

 

4

j

x

x0

j

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

(1.55)

[cf. Equation (1.5) on page 4 for Estat] and, if magnetic currents exist, a Biot-Savart- like law for electric fields [cf. Equation (1.15) on page 8 for Bstat]:

Estat(x) = 40

ZV0d3x0

jm(x0) x

 

x00

3

= 40

ZV0d3x0

jm(x0) r x

1

x0

 

 

 

 

 

 

 

 

 

x

 

x

 

 

 

 

 

 

 

 

 

= 40 r ZV0d3x0

jx

 

j

 

 

j

 

 

 

 

 

j

 

j

( x00

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

m x )

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

j

j

 

 

 

 

 

 

 

 

 

 

 

 

 

(1.56)

Taking the curl of the latter and using the operator “bac-cab” rule, Formula (F.59) on

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1.4 ELECTROMAGNETIC DUALITY

19

page 166, we find that

r Estat(x) = 0 r r

4

= 0 Z d3x0 jm(x0)r2

4 V0

ZV0d3x0 jx ( x00

 

=

 

 

 

 

 

 

 

 

 

 

 

m x )

 

 

 

 

 

 

 

 

 

 

 

j

 

j

 

 

 

 

 

 

 

 

1

 

 

+

0

ZV0d3x0 [jm(x0) r0]r0

 

 

1

 

 

j

x

x0

 

4

j

x

x0

 

 

 

j

 

 

 

 

 

 

j

 

 

 

 

 

 

 

 

 

 

 

 

(1.57)

Comparing with Equation (1.18) on page 9 for Estat and the evaluation of the integrals there, we obtain

Z

r Estat(x) = 0 d3x0 jm(x0) (x x0) = 0jm(x) (1.58)

V0

We assume that Formula (1.56) on the preceding page is valid also for time-varying magnetic currents. Then, with the use of the representation of the Dirac delta function, Equation (M.86) on page 185, the equation of continuity for magnetic charge, Equation (1.52) on page 17, and the assumption of the generalisation of Equation (1.55) on the facing page to time-dependent magnetic charge distributions, we obtain, formally,

r E(t;x) = 0 ZV0d3x0 jm(t;x0) (x x0) 40 @@t ZV0d3x0 m(t;x0)r0 jx 1x0j

= 0jm(t;x) @ B(t;x) @t

(1.59)

[cf. Equation (1.24) on page 10] which we recognise as Equation (1.50b) on page 17. A transformation of this electromagnetodynamic result by rotating into the “electric realm” of charge space, thereby letting jm tend to zero, yields the electrodynamic Equation (1.50b) on page 17, i.e., the Faraday law in the ordinary Maxwell equations. This process also provides an alternative interpretation of the term @B@t as a magnetic displacement current, dual to the electric displacement current [cf. Equation (1.26) on page 11].

By postulating the indestructibility of a hypothetical magnetic charge, we have thereby been able to replace Faraday's experimental results on electromotive forces and induction in loops as a foundation for the Maxwell equations by a more appealing one.

END OF EXAMPLE 1.1C

BDUALITY OF THE ELECTROMAGNETODYNAMIC EQUATIONS

 

EXAMPLE 1.2

 

Show that the symmetric, electromagnetodynamic form of Maxwell's equations (Dirac's symmetrised Maxwell equations), Equations (1.50) on page 17, are invariant under the duality transformation (1.54).

Explicit application of the transformation yields

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CLASSICAL ELECTRODYNAMICS

r ?E = r (Ecos +cBsin ) = e cos +c 0 m sin

"0

 

 

 

 

 

 

 

 

1

 

 

 

 

 

 

 

 

 

 

 

 

 

 

1

 

 

 

 

 

 

 

 

 

 

 

 

? e

 

 

 

 

 

 

=

 

e cos +

 

 

 

 

m sin

=

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

"0

c

"0

 

 

 

 

 

 

@?

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

@

 

 

 

 

 

1

 

 

 

 

 

 

 

 

 

r ?E +

B

= r (Ecos +cBsin )

+

 

 

 

 

 

 

Esin +Bcos

@t

@t

c

 

 

 

 

 

 

= 0jm cos

 

@B

 

 

 

 

 

 

 

 

 

 

 

 

 

 

1 @E

 

 

 

 

 

 

 

 

 

 

 

 

 

cos

+c 0je sin +

 

 

 

 

 

 

sin

 

 

 

 

 

 

 

@t

c

@t

 

 

 

 

 

 

 

 

 

 

1 @E

 

@B

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

sin +

 

 

 

 

 

 

cos = 0jm cos +c 0je sin

 

 

 

 

 

 

 

c

 

@t

 

@t

 

 

 

 

 

 

= 0( cje sin +jm cos ) = 0?jm

 

 

 

 

 

 

 

 

 

 

 

1

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

e

 

 

r ?B = r (

 

 

 

Esin +Bcos ) =

 

 

 

sin + 0 m cos

 

 

c

c"0

 

 

 

 

 

 

=

 

 

 

 

 

 

 

 

 

 

 

 

 

 

e

+

 

 

 

m

 

 

 

= ? m

 

?

1 @?E

 

0

c 1 sin

 

 

 

 

 

 

 

 

 

 

cos

10

@

 

 

 

 

 

 

 

 

 

 

 

 

r

B

 

 

 

 

= r (

 

 

Esin +Bcos )

 

 

 

(Ecos +cBsin )

c2

@t

c

c2

@t

 

 

 

 

 

 

=

1

0jm sin +

1

 

@B

cos + 0je cos +

1

 

@E

cos

 

 

 

 

 

 

 

c @t

 

 

 

 

 

 

 

 

 

 

c

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

c2 @t

 

 

 

 

 

 

 

 

 

 

 

1 @E

 

 

 

 

 

1 @B

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

cos

 

 

 

sin

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

c2

@t

c

@t

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

1

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

= 0

 

 

jm sin +je cos = 0?je

 

 

 

 

 

 

c

(1.60)

(1.61)

(1.62)

(1.63)

QED

END OF EXAMPLE 1.2C

EXAMPLE 1.3

BDIRAC'S SYMMETRISED MAXWELL EQUATIONS FOR A FIXED MIXING ANGLE

 

 

 

 

 

Show that for a fixed mixing angle such that

 

 

 

 

 

 

 

 

 

m =c e tan

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

(1.64a)

 

jm =cje tan

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

(1.64b)

 

the symmetrised Maxwell equations reduce to the usual Maxwell equations.

 

 

Explicit application of the fixed mixing angle conditions on the duality transformation

 

(1.54) on page 18 yields

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

? e

 

 

e

 

1

 

m

 

e

 

1

 

 

e

 

 

 

 

 

 

 

=

 

cos +

 

 

 

sin =

 

 

cos +

 

c

 

tan sin

 

 

 

c

 

 

 

c

 

(1.65a)

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

1

 

 

 

 

 

 

 

 

1

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

=

 

( e cos2 + e sin2 ) =

 

e

 

 

 

 

 

 

 

cos

cos

 

 

 

 

 

 

? m = c e sin +c e tan cos = c e sin +c e sin =0

(1.65b)

 

 

 

 

 

 

 

 

 

 

 

 

 

1

 

 

 

 

 

 

1

 

 

 

 

?je

= je cos +je tan sin =

 

(je cos2 +je sin2 ) =

 

je

(1.65c)

 

cos

cos

 

?jm = cje sin +cje tan cos = cje sin +cje sin = 0

(1.65d)

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1.4 ELECTROMAGNETIC DUALITY

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Hence, a fixed mixing angle, or, equivalently, a fixed ratio between the electric and magnetic charges/currents, “hides” the magnetic monopole influence ( m and jm) on the dynamic equations.

We notice that the inverse of the transformation given by Equation (1.54) on page 18 yields

E = ?Ecos c?Bsin

(1.66)

This means that

r E = r ?Ecos cr ?Bsin

(1.67)

Furthermore, from the expressions for the transformed charges and currents above, we find that

r ?E =

? e

=

 

1 e

 

(1.68)

"0

cos

 

"0

 

 

and

 

 

 

 

 

 

 

 

 

 

r ?B = 0? m =0

 

(1.69)

so that

 

 

 

 

 

 

 

 

 

 

1

 

 

e

 

 

 

 

e

 

r E =

 

 

 

cos 0 =

 

(1.70)

cos

"0

"0

and so on for the other equations.

 

QED

END OF EXAMPLE 1.3C

The invariance of Dirac's symmetrised Maxwell equations under the similarity transformation means that the amount of magnetic monopole densitym is irrelevant for the physics as long as the ratio m=e = tan is kept constant. So whether we assume that the particles are only electrically charged or have also a magnetic charge with a given, fixed ratio between the two types of charges is a matter of convention, as long as we assume that this fraction is the same for all particles. Such particles are referred to as dyons [14]. By varying the mixing angle we can change the fraction of magnetic monopoles at will without changing the laws of electrodynamics. For = 0 we recover the usual Maxwell electrodynamics as we know it.1

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CLASSICAL ELECTRODYNAMICS

EXAMPLE 1.4

BTHE COMPLEX FIELD SIX-VECTOR

 

 

 

 

 

 

 

 

 

 

 

 

 

The complex field six-vector

 

 

 

 

 

 

 

 

 

G(t;x) = E(t;x) +icB(t;x)

 

 

 

 

 

 

(1.71)

 

where E;B 2 R3 and hence G 2 C3, has a number of interesting properties:

 

 

1. The inner product of G with itself

 

 

 

 

 

G G =(E +icB) (E +icB) = E2 c2 B2 +2icE B

(1.72)

 

is conserved. I.e.,

 

 

 

 

 

 

 

 

 

E2 c2 B2 =Const

 

 

 

 

 

 

(1.73a)

 

E B =Const

 

 

 

 

 

 

(1.73b)

 

as we shall see later.

 

 

 

 

 

 

 

 

 

2. The inner product of G with the complex conjugate of itself

 

 

G G = (E +icB) (E icB) = E2 +c2 B2

(1.74)

 

is proportional to the electromagnetic field energy.

 

 

3. As with any vector, the cross product of G itself vanishes:

 

 

G G = (E +icB) (E +icB)

 

 

 

 

=

 

2

B B

+

ic(E B)

+

ic(B E)

(1.75)

 

 

E E c

 

 

 

=0 +0 +ic(E B) ic(E B) = 0

4.The cross product of G with the complex conjugate of itself

G G =(E +icB) (E icB)

=

E E

+

2

B B ic(E B)

+

ic(B E)

(1.76)

 

 

c

 

 

=0 +0 ic(E B) ic(E B) = 2ic(E B) is proportional to the electromagnetic power flux.

END OF EXAMPLE 1.4C

EXAMPLE 1.5 BDUALITY EXPRESSED IN THE COMPLEX FIELD SIX-VECTOR

Expressed in the complex field vector, introduced in Example 1.4, the duality trans-

1Nobel laureate Julian Schwinger (1918–1994) has put it [15]:

“. . . there are strong theoretical reasons to believe that magnetic charge exists in nature, and may have played an important role in the development of the universe. Searches for magnetic charge continue at the present time, emphasizing that electromagnetism is very far from being a closed object.”

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