1 June 17, J.D.Jackson, Classical Electrodynamics, 3rd Edition, Chapter 112 Introduction Einstein s theory of special relativity is based on the assum...

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June 17, 20081

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J.D.Jackson, ”Classical Electrodynamics”, 3rd Edition, Chapter 11 Special Theory of Relativity

Introduction Einstein’s theory of special relativity is based on the assumption (which might be a deep-rooted superstition in physics) that all physical laws should be invariant under transformation between inertial systems. The demand that Maxwell’s equations should be invariant under transformations, and the failure of Galilean transformations to do it led to the Lorentz transformations (β~ = ~v /c, γ = (1 − β 2 )−1/2 ) x0

=

γ(x00 − βx10 )

x1

=

γ(x10 − βx00 )

=

x20 x30

x2

(1)

x0

= γ(x00 + βx10 )

x1

= γ(x10 + βx00 )

x2

=

(2)

x20 x30

x3 = x3 = under which for example the equations of a spherical wave c 2t 2 − x 2 + y 2 + z 2 = 0

(3)

propagating with fixed velocity c are invariant. Lorentz transformations in general demand that the norm s 2 = x02 − x12 + x22 + x32

(4)

is invariant. Special Theory of Relativity

1st Postulate : The laws of nature and the results of all experiments performed in a given frame of reference are independent of the translational motion of the system as a whole 2nd Postulate : The speed of light is finite and independent of the motion of the source From the 1st postulate it follows that the mathematical equations expressing the laws of nature must be covariant, that is, invariant in form, under the Lorentz transformations. These demands call for rules on the ways that the scalars, 4-vectors and 4-tensors will transform in a spacetime whose norm is defined by (4). SPACETIME The space-time continuum is defined in terms of a 4-dimensional space with coordinates x 0 , x 1 , x 2 , x 3 .

Special Theory of Relativity

Tensors If we assume that there is a well defined transformation that yields from the coordinates x 0 , x 1 , x 2 , x 3 a new set of coordinates x 00 , x 01 , x 02 , x 03 according to the rule x 0α = x 0α (x 0 , x 1 , x 2 , x 3 )

(α = 0, 1, 2, 3)

(5)

Here we will defined the tensors under their transformation properties. A scalar (tensor of rank 0) is a single quantity whose value is not changed under the transformation. for example the interval s 2 in (4) is a scalar. Vectors are tensors of rank 1, and we distinguish two kinds. The contravariant vector Aα whose components transformed according to the rule 3 X ∂x 0α β ∂x 0α β A0α = A ≡ A (6) β ∂x ∂x β β=0

where the partial derivatives are calculated from (5). Explicitly we have 4 equations of the form: A0α =

∂x 0α 0 ∂x 0α 1 ∂x 0α 2 ∂x 0α 3 A + A + A + A ∂x 0 ∂x 1 ∂x 2 ∂x 3 Special Theory of Relativity

(7)

The covariant vector Bα is defined by the rule Bα0 =

3 X ∂x β ∂x β B ≡ Bβ β ∂x 0α ∂x 0α

(8)

β=0

where the partial derivatives are calculated from the inverse of (5). The contravariant tensor of rank 2 F αβ consists of 16 quantities (components) that transform according to F 0αβ =

∂x 0α ∂x 0β γδ F ∂x γ ∂x δ

(9)

A covariant tensor of rank 2 Gαβ transforms as 0 Gαβ =

∂x γ ∂x δ Gγδ ∂x 0α ∂x 0β

(10)

The mixed tensor of rank 2 H α β transforms as H 0α β =

∂x 0α ∂x δ γ H δ ∂x γ ∂x 0β

(11)

The generalization to arbitrary rank tensors is quite obvious extension of the above relations. Special Theory of Relativity

The inner or scalar product of two vectors is defined as the product of the components of a covariant and a contravariant vector B · A ≡ Bα Aα

(12)

with this definition the scalar product is an invariant or scalar under the transfomation (5): B 0 · A0

∂x 0α ∂x β ∂x β Bβ γ Aγ = Bβ Aγ 0α ∂x ∂x ∂x γ = δ β γ Bβ Aγ = Bγ Aγ = B · A

= Bα0 A0α =

(13)

The geometry of the space-time of STR is defined by the invariant interval s 2 defined in (4), which in differential form can be written as (ds)2 = (dx 0 )2 − (dx 1 )2 − (dx 2 )2 − (dx 3 )2

(14)

This norm or metric is a special case of the general differential length element ds 2 = gαβ dx α dx β (15) where gαβ = gβα is called the metric tensor. Special Theory of Relativity

For the flat space-time of STR the metric tensor is diagonal with elements g00 = 1 ,

g11 = g22 = g33 = −1

(16)

The contravariant tensor g αβ is defined as the normalized cofactor of gαβ . For the flat spacetime of STR they are the same g αβ = gαβ

(17)

The contraction of the covariant and contravariant metric tensors defines the Kronecker delta in 4-dimensions gαγ g γβ = δα β

(18)

where δαβ = 0 if α 6= β and δαα = 1. From the definition of the scalar product (12) and (15) we can easily conclude that xα = gαβ x β

(19)

x α = g αβ xβ

(20)

and its inverse This is a more general procedure for lowering and raising indeces ...α... ... F... = g αβ F...β...

... ...β... and G...α... = gαβ G... Special Theory of Relativity

(21)

From the definition of the flat spacetime metric tensor we can easily prove that: ~ , Aα = (A0 , −A) ~ Aα = (A0 , A) (22) The scalar product (12) of two vectors is ~ ·A ~ B · A ≡ Bα Aα = B 0 A0 − B From the transformation property ∂x β ∂ ∂ = 0α ∂x ∂x 0α ∂x β we conclude that the differentiation with respect ti a contravariant component of the coordinate vector transforms as the component of a covariant vector. Thus we employ the notation ∂ ∂ ∂ ~ ∂ α ~ ∂ ≡ = , −∇ , ∂α ≡ = ,∇ (23) ∂xα ∂x 0 ∂x α ∂x 0 The 4-divergence of a 4-vector A is the invariant ∂A0 ~ ~ +∇·A (24) ∂x 0 an equation familiar in form from continuity of charge and current density. ∂ α Aα = ∂α Aα =

Special Theory of Relativity

The 4-dimensional Laplacian operator is defined to be the invariant contraction ∂2 ≡ ∂α ∂ α = − ∇2 (25) ∂x 0 2 which is of course the operator of the wave equation in vacuum. The previous examples show how the covariance of a physical law emerges provided suitable Lorentz transformation properties are attributed to the quantities entering the equation.

Special Theory of Relativity

Invariance of Electric Charge; Covariance in Electrodynamics The invariance of the equations of electrodynamics under Lorentz transforms was shown by Lorentz and Poincar´e before the formulation of the STR. The invariance in form or covariance of the maxwell and Lorentz force ~, B ~ that enter into equations implies that the various quantities ρ, ~J, E the equations transform in a well defined way under Lorentz transformations. Consider first the Lorentz force equation for a charged particle d~p ~ + ~v × B ~ =q E (26) dt c we know that ~p transforms as the space part of energy and momentum ~ p α = (p0 , ~p ) = m U0 , U where p0 = E /c and U a is the 4-velocity U0 ≡

dx0 dx0 dt ~ ≡ d~x = d~x dt = γ~u = = γc , U dτ dt dτ dτ dt dτ Special Theory of Relativity

(27)

If we use the proper time of the particle which is a Lorentz invariant quantity defined as p 1 1 (28) dτ = ds = dt 1 − β 2 = dt c γ for the differentiation of (26) we can write d~p q ~ ~ ~ = U0 E + U × B (29) dτ c the left hand side is the space part of a 4-vector. The corresponding time component equation is the rate of change of the energy of the particle Z q~ ~ dEmech dp0 ~J · E ~ d 3x = U ·E ⇐ = (30) dt c dt V The right-hand sides of the previous two equations involve three factors, the charge q, the 4-velocity and the electromagnetic fields. If the transformation properties of two of the three factors are known and Lorentz covariance is demanded, then the transformation properties of the 3rd factor can be established. The experimental invariance of electric charge and the requirement of Lorentz covariance of the Lorentz force eqn (29) and (30) determines the Lorentz transformation properties of the EM field. Special Theory of Relativity

~ ·E ~ be the time For example, the requirement from (30) that U ~ are the component of a 4-vector establishes that the components of E time-space parts of a 2nd rank tensor F αβ such that ~ ·E ~ = F 0β Uβ U We will consider Maxwell equations and we begin with the charge density ρ(~x , t) and current density ~J(~x , t) and the continuity equation ∂ρ ~ ~ +∇·J =0 ∂t

(31)

It is natural to postulate that ρ and ~J together form a 4-vector J α : J α = cρ, ~J (32) and the continuity equation takes the covariant form: ∂α J α = 0 where the covariant differential operator ∂α is given by (23). Special Theory of Relativity

(33)

If we consider the Lorentz gauge 1 ∂Φ ~ ~ +∇·A=0 c ∂t

(34)

then the wave equations for the vector and scalar potential are ~ 1 ∂2A ~ = 4π ~J − ∇2 A 2 2 c ∂t c (35) 1 ∂2Φ − ∇2 Φ = 4πρ c 2 ∂t 2 Notice that the differential operator in (35) is the invariant 4-D Laplacian (25) while the right hand side are the components of the 4-vector (32). ~ form Obviously, Lorentz covariance requires that the potentials Φ and A a 4-vector potential ~ Aα = Φ, A (36) Then the wave equation (35) and the Lorentz condition (34) take the covariant forms 4π α J , ∂α Aα = 0 (37) Aα = c Special Theory of Relativity

~ and B ~ are expressed in terms of the potentials as The fields E ~ ~ = − 1 ∂ A − ∇Φ ~ , E c ∂t

~ =∇ ~ ~ ×A B

(38)

~ and B ~ are explicitly where, for example, the x-component of E 1 ∂Ax ∂Φ Ex = − − = − ∂ 0 A1 − ∂ 1 A0 c ∂t ∂x (39) ∂Az ∂Ay Bx = − = − ∂ 2 A3 − ∂ 3 A2 ∂y ∂z These equations imply that the 6 in total components of the electric and magnetic fields are the elements of a 2nd-rank, antisymmetric field-strength tensor F αβ = ∂ α Aβ − ∂ β Aα (40) explicitly in matrix form

F αβ

0 Ex = Ey Ez

−Ex 0 Bz −By

−Ey −Bz 0 Bx

−Ez By −Bx 0

Special Theory of Relativity

(41)

In the covariant form is:

Fαβ = gαγ gδβ F γδ

0 −Ex = −Ey −Ez

Ex 0 Bz −By

Ey −Bz 0 Bx

Ez By −Bx 0

~ → −E ~. The elements of Fαβ are obtained from F αβ by putting E

Special Theory of Relativity

(42)

The inhomogeneous Maxwell equations are ~ ~ − 1 ∂ E = 4π ~J ~ ×B ∇ c ∂t c α and J they take the covariant form (HOW?) ~ = 4πρ , ~ ·E ∇

in terms of F αβ

4π β J c Similarly the homogeneous Maxwell equations are ∂α F αβ =

~ = 0, ~ ·B ∇

(43)

~ ~ + 1 ∂B = 0 ~ ×E ∇ c ∂t

take the form (HOW?) ∂α Fβγ + ∂β Fγα + ∂γ Fαβ = 0

(44)

With the above definitions of the various quantities and the reformulation of the wave and Maxwell equations the covariance of the equations of EM is established. Finally, the Lorentz force (29) and rate of change of energy (30) can be set in manifestly covariant form dp α dU α q =m = F αβ Uβ (45) dτ dτ c Special Theory of Relativity

Dual Field-Strength Tensor

Fαβ =

1 αβγδ Fγδ 2

0 Bx = By Bz

−Bx 0 −Ez Ey

−By Ez 0 −Ex

−Bz −Ey Ex 0

(46)

where αβγδ =0, +1, -1. ~ →B ~ and The elements of F αβ are obtained from F αβ by putting E ~ → −E ~ . The homogeneous Maxwell equations can be written in terms B of the dual field-strength tensor as ∂α F αβ = 0

Special Theory of Relativity

(47)

Transformation of Electromagnetic Fields ~ and B ~ are the elements of a 2nd-rank tensor F αβ , their Since both E values in one inertial frame can be expressed in terms of the values in another inertial frame, according to F 0αβ =

∂x 0α ∂x 0β γδ F ∂x γ ∂x δ

(48)

If the one system travels along the direction of x1 with speed cβ the explicit transformations are (HOW?) E10

=

E1

B10 = B1

E20

=

γ(E2 − βB3 )

B20 = γ(B2 + βE3 )

E30

=

γ(E3 + βB2 )

B30 = γ(B3 − βE2 )

(49)

This suggest that for a general Lorentz transformation between two systems moving with a speed v relative to each other the transformation of the fields can be written (HOW): Special Theory of Relativity

~0 E

2 ~ + β~ × B ~ − γ β~ β~ · E ~ = γ E γ+1

~0 B

2 ~ − β~ × E ~ − γ β~ β~ · B ~ = γ B γ+1

(50)

~ and B ~ have no independent • These transformations show that E existence. • A purely electric or magnetic field in one coordinate system will appear as a mixture of electric and magnetic fields in another coordinate frame. • Thus one should properly speak of the electromagnetic field F αβ ~ and B ~ separately. rather than E Finally, if no magnetic field exists in a frame K 0 the inverse of (48) shows ~ and the electric field E ~ are that in the frame K the magnetic field B linked by the simple relation ~ = β~ × E ~ B ~ is the transformed field from K 0 to K . note that E Special Theory of Relativity

(51)

We will study the fields seen by an observer in the system K when a point charge q moves in a straight line with velocity ~v . The charge is at rest in the system K 0 and the transformation of the fields is given by the inverse of (48) or (48)

The observer is at the point P. In the frame K 0 the observer’s point P, 0 0 0 where the fields are to be evaluated, p has coordinates x1 = −vt , x2 = b, 0 0 2 2 x3 = 0 and is at a distance r = b + (vt) In the rest frame K 0 of the charge the electric and magnetic fields at the observation point are (WHY?) E10 = − qvt r 03 B10 = 0

0

E20 = rqb03 B20 = 0

E30 = 0 B20 = 0

Special Theory of Relativity

In terms of the coordinates of K the nonzero field components are E10 = −

qγvt , (b 2 + γ 2 v 2 t 2 )3/2

E20 =

qb (b 2 + γ 2 v 2 t 2 )3/2

(52)

Then using the inverse of (48) we find the transformed fields in the system K : E1 E2 B3

qγvt + γ 2 v 2 t 2 )3/2 γqb = γE20 = 2 (b + γ 2 v 2 t 2 )3/2 = γβE20 = βE2 = E10 = −

(b 2

(53) (54)

with all the other components vanishing. Notice the magnetic induction in the direction x3 . The magnetic field becomes nearly equal to the transverse electric field E2 as β → 1.

Special Theory of Relativity

• At low velocities (γ ≈ 1) the magnetic induction is ~ ≈ q ~v × ~r B c r3 which is the approximate Amp´ere-Biot-Savart expression for the magnetic field of a moving charge. • At high velocities (γ 1) we see that the transverse electric field E2 becomes equal to γ times its non-relativistic value. • At high velocities (γ 1) the duration of appreciable field strengths at point P is decreased.

Special Theory of Relativity

Figure: Fields of a uniformly moving charged oarticle (a) Fields at the observation point P as function of time. (b) Lines of electric force for a particle at rest and in motion (γ = 3). Special Theory of Relativity

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