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12.1 The Special Theory of Relativity

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Electrodynamics and Relativity

Does the principle of relativity apply to the laws of electrodynamics?

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12.1 The Special Theory of Relativity

Does the principle of relativity apply to the laws of electrodynamics?

On the other hand, for someone on the train the magnet is in motion and the conductor at rest. No

magnetic force, because the conductor is at rest. But, a changing magnetic field induces an electric field by Faraday’s law, resulting in an electric force (induced emf).

If the magnet is stationary and the conductor in motion, no electric field arises in the neighborhood of the magnet. In the conductor, however, we find an magnetic force (motional emf)

Take, for example, the reciprocal electrodynamic action of a magnet and a conductor:

The observable phenomenon here depends only on the relative motion of the conductor and the magnet.

 The motional emf and the induced emf give rise to electric currents of the same path and intensity.

 Was the equality of the two emf's Just a lucky accident?

Einstein could not believe this was a mere coincidence; he took it, rather, as a clue that electromagnetic phenomena, like mechanical ones, obey the principle of relativity.

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1. The principle of relativity. (first elevated by Galileo Galilei)

 The laws of physics apply in all inertial reference systems.

 It states that there is no absolute rest system.

2. The universal speed of light.

 The speed of light in vacuum is the same for all inertial observers, regardless of the motion of the source.

Einstein's velocity addition rule:

Galileo's velocity addition rule:

The three most striking geometrical consequences of Einstein's postulates:

 the relativity of simultaneity:

Two events that are simultaneous in one inertial system are not, in general, simultaneolus in another.

 time dilation:

Moving clocks run slow.

 Lorentz contraction:

Moving objects looks shorter, from ground point of view.

(measured on car) (measured on ground)

t t

 

2 2

1

1 /

tc t t

      

2 2

1 1 /

x x x

c

 

    

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12.1 The Special Theory of Relativity

(i) the relativity of simultaneity:

Two events that are simultaneous in one inertial system are not, in general, simultaneolus in another.

(ii) Time dilation:

Moving clocks run slow.

(iii) Lorentz (length) contraction:

Moving objects looks shorter.

Only along the direction of its motion.

Dimensions perpendicular to the velocity are not contracted.

2 2

1 /

tc t

   

2 2

1 1 /

x x

c

  

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Galilean transformations

Lorentz transformations

( , , , ) S x y z t

( , , , ) S x y z t

, since

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12.1.3 The Lorentz Transformations

(Ex) Einstein's velocity addition rule

In S, suppose a particle moves a distance dx in a time dt:

Velocity

in a time a distance

( , , , ) S x y z t

( , , , ) S x y z t

t 1 t

    

 Moving clocks run slow.

x 1 x

    

 Moving object looks shorter.

-

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Four-vectors

 to changing the unit of time from the second to the meter

1 meter of xocorresponds to the time it takes light to travel 1 meter

Lorentz transformation matrix: 

: Lorentz transformation matrix

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12.1.4 The Structure of Spacetime

Four-vectors =

any set of four components that transform under Lorentz transformations

A B   Four-dimensional scalar product:

(Prove; Prob. 12.17) The 4-dim. Dot product has the same value in all inertial systems:

Einstein summation convention

0 0 1 2 3 0 1 2 3

1 2 3 0 1 2 3

A B    a ba ba ba ba ba ba ba b

A B  

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Displacement 4-vector:

Interval between two events:

where t is the time difference between the two events and d is their spatial separation.

When you transform to a moving system, the time between A and B, and the spatial separation are altered.

But, the interval I remains the same!

Depending on the two events in question, the interval can be positive, negative, or zero:

timelike

spacelike

lightlike

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Space-time diagrams ( Minkowski diagrams) and World line time

space

Trajectory of a particle on a Minkowski diagram world line.

timelike (slope greater than 1) spacelike (slope less than 1)

lightlike (slope 1)

world line

Light line

Minkowski diagrams

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