VISUAL PHYSICS ONLINE

 

LIGHT and SPECIAL RELATIVITY

    LENGTH CONTRACTION

 

 

 

SUMMARY

 

Time is a relative quantity: different observers can measurement different time intervals between the occurrence of two events. This arises because the speed of light is a constant and independent of the motion of the source of light or the motion of an observer.

 

Moving clocks run slow

 

Time Dilation Effect

Proper time t0 – the time interval between two events occurring at the same point in space w.r.t. a clock at rest at that point.

Dilated time interval t time interval for an event observed in a moving frame by a stationary observer as measured their synchronised clocks.

                t > t0    since   

 

 

 

Lorentz-Fitzgerald Contraction Equation of a moving object

         

 

 

contracted length L and proper length L0

 

Contraction takes place in the direction of motion only

 

 

 

 

Learning strategies

The way to approach the time dilation effect and the length contract effect is to recognise the fact that there are two frames of reference moving with a constant velocity w.r.t. to each other. An easy way to do this is to label the two frames of reference as Stationary or Fixed (Steve) and Moving (Mary).

·       Steve: stationary (fixed) frame of reference

·       Mary: moving frame of reference (Mary’s frame of reference is moving at a constant velocity  w.r.t  Steve’s frame of reference)

 

The proper length L0 is measured in the moving frame of reference and the constracted length L is the length measured by the observer in the stationary frame of reference.

 

 

 

LENGTH CONTRACTION

Length is a relative quantity

 

When measuring the length of an object it may be necessary measure the exact position of its ends simultaneously.  However, observers in different reference frames may disagree on the simultaneity of two events. So, they may also disagree about the length of objects. In turns out, the length of a moving object appears to contract in the direction of motion relative to a “stationary” observer.

 

Equation (1) is known as the Lorentz-Fitzgerald Contraction Equation of a moving object

        (1)      

 

 

·       Contracted length of object   in direction of motion as measured by observer in stationary frame of reference.

·       Rest length or proper length of object   as measured by observer in the moving frame of reference. The proper length is measured in the frame in which the object is at rest.

·       Velocity v (magnitude) of the object relative to the observer in the stationary frame of reference.

 

 Contraction takes place in the direction of motion only

 

You are a stationary observer in an inertial frame of reference. A train was initially at rest in your frame of reference and you measure its length. However, when the train is in motion your measurement of its length is shorter. There is a contraction in its length. The train is shorter in the direction of motion, but just as high and wide as it was at rest as shown in figure 1.

 

        Fig. 1.   How long is a train? It depends on the relative motion of the observer and the train.

 

This is a real difference in length of the object when it is motion relative to an observer. For a person in the train, there is no contraction in length.

 

Figure 2 shows an animation of the length contract effect. Steve observers the rod in his system as 80 m long. Steve observes the rod in moving frames of reference to be shorter in length. The greater the velocity  of the moving frame w.r.t. the stationary frame, the greater the contraction in length.

Fig. 2.   A moving object is shorter to an observer in a stationary a stationary frame of reference.

 

The time dilation effect and the length contraction effect depend on velocity  of the moving frame w.r.t. the stationary frame (figure 3).

 

Fig. 3.    and  as functions of .

               Newtonian principles can be applied when .

             As  

 

 

Example 1

A spaceship flies past Earth at a speed of 0.990c. Mary on board the spaceship measures its length to be 400 m. What is Steve’s measurement for the length of the spaceship on Earth?

Steve and Eve on Earth are standing 60 m apart as they view the passing spaceship. How far apart are Steve and Eve from Mary’s point of view?

Solution

The problem relates to the length contraction of a moving rod.

 

Moving frame (Mary)

Mary in her system measures the proper length of the spaceship 

 

Stationary frame (Steve)

Steve observes the spaceship moving at uniform velocity v and measures the length of the spaceship as L (contracted length)

            

Lorentz-Fitzgerald Contraction

     

 

The answer makes sense, the moving spaceship is observed to the shorter than in the frame stationary w.r.t. to the spaceship.

 

Moving frame (Steve and Eve)

Steve and Eve are at rest in the frame of the Earth. Their separation distance of 60 m is the proper length.

 

Stationary frame (Mary)

 From Mary perspective, Steve and Eve are moving at a speed v. So, Mary will measure a contracted length L as the separation distance:

          

 

 

 

 

 

Example 2

The diameter of our galaxy is 6.0x1020 m.

(a)        If the speed of the spaceship was 0.99999c, how long would it take to cross the galaxy as measured from the frame of reference of the spaceship?

(b)       How much time would elapse on Earth for this journey across the galaxy?

 

Solution

(a)

Relative velocity of moving frame w.r.t. stationary frame 

Stationary frame (Earth and Galaxy)   proper length    

 

Moving frame (observer in spaceship)

A traveller in the spacecraft would be at rest in the spaceship and would see the galaxy approaching at speed v. The traveller would see the galaxy contracted in the direction of motion. The contracted length L is

         

 

If the time t0 is measured in the spacecraft, the time for the journey across the galaxy is

        t0 = ? s = ? years

        L = 2.7x1018  m           

        L = v t0

       

 

Even a spaceship travelling at speeds 0.99999c it still takes 300 years to cross the galaxy.

 

(b)

Moving frame (observer in spaceship)  proper time  

Stationary frame (observer on Earth)

An Earth bound observer will view the moving clock on the spaceship and measure a dilated time interval

        dilated time interval for Earth observer  t = ?  years

        v = 0.99999c

      

 

 

Alternative calculation for space ship to reach galaxy

       

 

 

WOW!!!  For the Earth observer, 64 000 years pass for the spaceship to cross the galaxy but on the spaceship only 300 years have passed.

 

Only, spaceships travelling at speeds extremely close to the speed of light can traverse the huge astronomical distances need for space travel in “reasonable” times.

 

 

 

 

Example 3

This problem is more difficult than you would normally encounter at school. However, it is a very interesting one, and emphasizes some of the important conceptual difficulties in special relativity. Reference: Modern Physics, J.R. Taylor and C.D. Zafiratos

 

A relativistic snake called Mary of proper length 1.00 m is moving at speed v = 0.60 c to the right across a table. Steve, wishes to tease the snake, and holds two knives 1.00 m apart and plans to bounce them simultaneously on the on the table so the left knife lands immediately behind the snake’s tail. Steve argues as follows

“The snake (Mary) is moving with v = 0.60 c. Its contracted length is only 0.80 m

           

 

Therefore, the right knife will land 0.20 m in front of the snake’s head, and the snake will not be harmed.”

 

However, Mary the snake argues, “the knives are approaching me at v = 0.60 c and the distance between them is contracted to 0.80 m. So, I will be cut into two pieces when the knives fall”.

 

The snake Mary and Steve cannot be both correct. The snake will or will not be cut into two. We can resolve this paradox using special relativity. What appears to be simultaneous in one frame of reference is not necessarily simultaneous in another frame of reference.

 

 

In Steve’s frame of reference, the snake is moving at speed v = 0.60 c and will observe the contraction in the snake’s length. The two knives are stationary in Steve’s frame. So, the statement that the two knives fall simultaneously at t = 0 is a correct.

 

To see what really happens, we need to examine the moving frame more carefully. We now know that time and space are connected. The connection between time intervals and spatial coordinates of two frames of reference (Stationary and Moving) is given by the equations (not in syllabus)

        

           

 

Stationary frame (Steve)

Left-hand knife falls at  = 0 when  = 0

Right-hand knife falls at  = 1.00 m when  = 0

Contracted length of snake    

 

Moving frame (Snake / Mary)

Left hand knife falls at  = 0 when  = 0

As expected, the left knife falls immediately besides the snake’s tail at time  = 0.

 

Right-hand knife falls at position  and time  where

                   

 

                      

 

                       

 

Thus, the snake will observe that the two knives not falling simultaneously, since the right knife falls 2.50 ns before the left knife. Therefore, the right knife does not necessarily have to hit the snake, even though the two knives are 0.80 m apart. We know the knife does miss the snake because the right knife falls at 1.25 m well ahead of the snake’s head as shown in the following animation.

 

 

The resolution of this paradox, and many similar paradoxes, is seen to be that two events which are simultaneous as observed in one frame are not necessarily simultaneous when observed in a different frame.      

             

 

 

DERIVATIONS OF THE LENGTH CONTRACTION EQUATION

(1)

Consider a high-speed aircraft flying from the Earth to a planet at a constant velocity  as shown in figure 4 as observed by Steve on earth and Mary on the aircraft.

                         (Remember the definition of velocity in [1D]  )

 

Fig. 4.   A length is measured to be shorter when it is moving relative to the observer than when it is at rest.

 

Stationary frame (observer Steve on earth)

Steve needs two clocks to measure the departure time  from Earth and the arrival time  at the planet to measure the time interval  for the journey of length .  Hence the length of the journey according to Steve is .

 

Moving frame (observer Mary on aircraft)

Mary only need one clock to measure the time interval  (proper time) for the journey. Mary will observe the Earth receding at speed v and the planet approaching at speed v. Therefore, Mary will conclude that the distance between the Earth and planet is .

Hence, using the dilation effect equation, we can derive the equation for length contraction.

Time dilation effect  

 

 

Length contraction  

 

                                            

 

 

(2)

We attach a laser to one end of a rod and a mirror at the other. The rod is at rest in Mary’s system, and the length of the rod is L0 (proper length since it is at rest w.r.t observer Mary).

 

Moving system (Mary)

Mary measures a time interval t0 for a pulse of light to make the round trip from laser to mirror and back. This is the proper time interval since the departure and return occur at the same location in Mary’s system.

Fig. 5.  The rod is stationary in Mary’s system. The light pulse travels a distance L0 from the light source to the mirror. The time for the round trip is t0.

 

 

Stationary system (Steve)

In Steve’s system, the rod is moving to the right with constant speed v. Steve’s measures the length of the rod as L and the time for the light to travel from laser to mirror as t1. During this time interval t1, the rod with laser and mirror attached moves a distance to the right.

 

Fig. 6.  The rod is moving to the right with constant speed v in Steve’s system. The light pulse travels a distance d1 from the laser to the mirror in time t1.

 

The total length of the path d1 from laser to mirror is therefore . But, the light pulse travels with speed c, so it is also true that . Eliminating d, we find

                  

 

 

Note: the division of L by c-u does not mean that light travels with speed c-u, but rather the light pulse travels in Steve’s frame a distance greater than L.

 

Repeating a similar calculation, the time interval t2 from the return journey of the light pulse from the mirror to the laser is

                       

 

The total time t for the for the round trip is

                    

 

 

The proper time t0 and the dilated time t intervals are connected by

              but     

 

 

 

Hence, we can conclude

 

 

(3)

There are two inertial frames of reference, Steve’s and Mary’s. From Steve’s point of view, Mary’s frame in moving with a constant velocity of magnitude v. They both make measurements of the length of a rod. The rod is stationary in Mary’s frame but moving with velocity v in Steve’s frame. They both measure the length of the rod by observing the time interval for a light pulse to travel from one end of the rod to the other. They observe know that the speed of light is the same w.r.t both frames of reference.

        Distance measured by Mary is

       Distance measured by Steve is

 

So far everything is straight forward, but now here comes the “tricky part”. We must identify the proper and dilated time intervals and the proper length and the contracted length.

Steve’s clock is stationary w.r.t. his frame, therefore, his clock records the proper time and he view Mary’s clock which is the dilated time interval

         

 

 

Steve views the moving rod, so he measures the contracted length, while the rod is stationary in Mary’s frame, so it is the proper length

 

           

      

 

          

        

 

Length contraction is real. This is not an optical illusion. The rod is really shorter in Mary’s system than in Steve’s system.