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Relativity of Length Distance between two points on a rigid body P & Q can be measured by a light signal’s round-trip time. P Q mirror laser l l can be measured by the time interval: t 2 t 1 , 2 1 2 1 2 ( ) ( ) 2 c l ct t l t t As we have seen, Dt will be different for different inertial observers, l will also !

ch37 young freedman - George Mason Universitycomplex.gmu.edu/.../phys262/soln/ch37_young_freedman3.pdf · 2020. 4. 16. · 'LVWDQFH EHWZHHQ WZR SRLQWV RQ D ULJLG ERG\ 3 4FDQ EH PHDVXUHG

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Page 1: ch37 young freedman - George Mason Universitycomplex.gmu.edu/.../phys262/soln/ch37_young_freedman3.pdf · 2020. 4. 16. · 'LVWDQFH EHWZHHQ WZR SRLQWV RQ D ULJLG ERG\ 3 4FDQ EH PHDVXUHG

Relativity of Length

Distance between two points on a rigid body P & Q can be measured by a light signal’s round-trip time.

PQ

mirror

laser

l

l can be measured by the time interval: t2 – t1, 2 1 2 12 ( ) ( )2

cl c t t l t t

As we have seen, Dt will be different for different inertial observers, l will also !

Page 2: ch37 young freedman - George Mason Universitycomplex.gmu.edu/.../phys262/soln/ch37_young_freedman3.pdf · 2020. 4. 16. · 'LVWDQFH EHWZHHQ WZR SRLQWV RQ D ULJLG ERG\ 3 4FDQ EH PHDVXUHG

Proper LengthSimilar to the concept of proper time which is the measured time interval of a clock which is at rest with the observer, proper length is the measured length of an object at rest with the observer.

0tD

0l

u

S

S’

Observer O’ in S’- frame will measure proper time and proper length for the clock and ruler shown.

Page 3: ch37 young freedman - George Mason Universitycomplex.gmu.edu/.../phys262/soln/ch37_young_freedman3.pdf · 2020. 4. 16. · 'LVWDQFH EHWZHHQ WZR SRLQWV RQ D ULJLG ERG\ 3 4FDQ EH PHDVXUHG

Length Contraction (parallel to u)Let consider a ruler at rest in the moving frame (S’) and it lays parallel to the direction of the relative motion between S and S’ (as shown previously).

Within S’- frame, the ruler is at rest with Mavis.

The length of the ruler is measured using a light-clock by measuring the time interval between two events (light leaving the laser and light arrives back to the source). In this measurement process, light pulse travels a distance of a total of 2l0 within a time interval of Dt0.

Page 4: ch37 young freedman - George Mason Universitycomplex.gmu.edu/.../phys262/soln/ch37_young_freedman3.pdf · 2020. 4. 16. · 'LVWDQFH EHWZHHQ WZR SRLQWV RQ D ULJLG ERG\ 3 4FDQ EH PHDVXUHG

Length Contraction (parallel to u)Since both measurement events are at rest (same location) within S’-frame, Dt0

is the proper time measurement and we have,

00

2lt

cD

Now, let consider the description according to Stanley in S-frame.

The ruler according to Stanley will have a length of l and let the time of travel for the light pulse from the source to the mirror be Dt1.

(note: Since Stanley is measuring these from afar and he is in relative motion with respect to Mavis, his measurement of Dt1 will NOT be proper.)

and is the proper length of the ruler.0l

Page 5: ch37 young freedman - George Mason Universitycomplex.gmu.edu/.../phys262/soln/ch37_young_freedman3.pdf · 2020. 4. 16. · 'LVWDQFH EHWZHHQ WZR SRLQWV RQ D ULJLG ERG\ 3 4FDQ EH PHDVXUHG

Length Contraction (parallel to u)

Within the time interval Dt1, the mirror will have moved a distance of u Dt1

so that the actual distance that the laser light has to travel is,

1d l u t DSince the speed of light is also c in Stanley frame, we can also write,

1d c t D

Page 6: ch37 young freedman - George Mason Universitycomplex.gmu.edu/.../phys262/soln/ch37_young_freedman3.pdf · 2020. 4. 16. · 'LVWDQFH EHWZHHQ WZR SRLQWV RQ D ULJLG ERG\ 3 4FDQ EH PHDVXUHG

Length Contraction (parallel to u)Combing these two equations and eliminating d, we have

1 1

1

c t l u t

lt

c u

D D

D

Now, let consider the return trip of the laser light…

l

Let Dt2 be the time measured by Stanley for the light to travel back from the mirror back to the source.

Note that as the train moves forward, the source also moves forward to meet the laser light

Page 7: ch37 young freedman - George Mason Universitycomplex.gmu.edu/.../phys262/soln/ch37_young_freedman3.pdf · 2020. 4. 16. · 'LVWDQFH EHWZHHQ WZR SRLQWV RQ D ULJLG ERG\ 3 4FDQ EH PHDVXUHG

Length Contraction (parallel to u)Combing these two equations by eliminating d, we have

1 1

1

c t l u t

lt

c u

D D

D

Now, let consider the return trip of the laser light…

l

Let Dt2 be the time measured by Stanley for the light to travel back from the mirror back to the source.

Note that as the train moves forward, the source also moves forward to meet the laser light

Page 8: ch37 young freedman - George Mason Universitycomplex.gmu.edu/.../phys262/soln/ch37_young_freedman3.pdf · 2020. 4. 16. · 'LVWDQFH EHWZHHQ WZR SRLQWV RQ D ULJLG ERG\ 3 4FDQ EH PHDVXUHG

Length Contraction (parallel to u)

Analogous to the outgoing trip, the return trip of the laser light will be shortened by uDt2 and

2 2 2

lc t l u t t

c uD D D

The total travel time for the laser pulse is 1 2t t tD D D

(l l l c ut

c u c u

D

c u

2 2 2 2 2 2 2

) 2 2

1 1

lc l

c u c u c c u c

l

2u tD 2c tD

Page 9: ch37 young freedman - George Mason Universitycomplex.gmu.edu/.../phys262/soln/ch37_young_freedman3.pdf · 2020. 4. 16. · 'LVWDQFH EHWZHHQ WZR SRLQWV RQ D ULJLG ERG\ 3 4FDQ EH PHDVXUHG

Length Contraction (parallel to u)From the time dilation formula, we also have

0t tD D

Combing these two equations for Dt, we have

01/ 22 2 2 2

01/ 22 2

22 1

1 1

1

ll

cc u c u c

ll

u c

or 0ll

(length contraction)

Recall: The two timingevents for the length measurement are at rest in S’-frame so that Mavis measure the proper time Dt0

and proper length l0.

On the other hand, Stanley’s measurements (Dt and l) of the same two events are not proper.

Note: The proper length l0 is always the longest among all inertial observers.

Page 10: ch37 young freedman - George Mason Universitycomplex.gmu.edu/.../phys262/soln/ch37_young_freedman3.pdf · 2020. 4. 16. · 'LVWDQFH EHWZHHQ WZR SRLQWV RQ D ULJLG ERG\ 3 4FDQ EH PHDVXUHG

Unreality Check

According to Galilean Velocity Transformation, in S-frame, we have

On the out going trip, 1c c u so that 11

l l lt

c u u cc uD

On the returning trip, 2c c u so that 22

l l lt

c u u cc uD

Now, the total time for the whole trip is now,

1 2

2lt t t

cD D D

From our previous “unreality check”, 0t tD D

00

22o

llt t l l

c cD D

(all clocks clicks at the same rate)

Page 11: ch37 young freedman - George Mason Universitycomplex.gmu.edu/.../phys262/soln/ch37_young_freedman3.pdf · 2020. 4. 16. · 'LVWDQFH EHWZHHQ WZR SRLQWV RQ D ULJLG ERG\ 3 4FDQ EH PHDVXUHG

Relativity of Simultaneity

Simultaneity

flash a flash b

Definition: Two flashes (event a and b) are considered to be simultaneous with respect to observer O if light from a & b (equal distance to observer O in the middle) arrive at the observer at the same time.

O

Page 12: ch37 young freedman - George Mason Universitycomplex.gmu.edu/.../phys262/soln/ch37_young_freedman3.pdf · 2020. 4. 16. · 'LVWDQFH EHWZHHQ WZR SRLQWV RQ D ULJLG ERG\ 3 4FDQ EH PHDVXUHG

Relativity of Simultaneity

At time t = 0:

O’ and O are respectively in the middle of A-B and A’-B’.

We will analyze the situation in Stanley’s S-frame in the following slides.

Page 13: ch37 young freedman - George Mason Universitycomplex.gmu.edu/.../phys262/soln/ch37_young_freedman3.pdf · 2020. 4. 16. · 'LVWDQFH EHWZHHQ WZR SRLQWV RQ D ULJLG ERG\ 3 4FDQ EH PHDVXUHG

Relativity of SimultaneityOn the ground (S-frame) after some time t,

Light travels at the same speed c in both frames.

Page 14: ch37 young freedman - George Mason Universitycomplex.gmu.edu/.../phys262/soln/ch37_young_freedman3.pdf · 2020. 4. 16. · 'LVWDQFH EHWZHHQ WZR SRLQWV RQ D ULJLG ERG\ 3 4FDQ EH PHDVXUHG

Relativity of Simultaneity

Then, a bit later, when Stanley see the lights from A and B reach him simultaneously, Mavis in S’- frame still waiting for the light from the lighting strike at the rear of the train to reach her.

According to Mavis, the lighting strikes at A’ and B’ did not occur simultaneously. Stanley agrees with Mavis’ observation.

On the ground (S-frame) after some more time t,

Page 15: ch37 young freedman - George Mason Universitycomplex.gmu.edu/.../phys262/soln/ch37_young_freedman3.pdf · 2020. 4. 16. · 'LVWDQFH EHWZHHQ WZR SRLQWV RQ D ULJLG ERG\ 3 4FDQ EH PHDVXUHG

Unreality CheckIn the (incorrect) Galilean view, according to Stanley, cA’ and cB’ inside the train will be modified according to their relative speed u.

'

'

A

B

c c u

c c u

Speed of light from A’ and B’ will be modified by the box car’s speed u.

So that light signals from A’ will speed up and signal from B’ will slow down in Stanley’s viewpoint.

This changes in speed for c will result in signals from A’ and B’ to arrive at O’ at the same time so that Stanley will say that both Marvis and himself will observe the lighting strikes simultaneously.

Page 16: ch37 young freedman - George Mason Universitycomplex.gmu.edu/.../phys262/soln/ch37_young_freedman3.pdf · 2020. 4. 16. · 'LVWDQFH EHWZHHQ WZR SRLQWV RQ D ULJLG ERG\ 3 4FDQ EH PHDVXUHG

Sequence of Events according to Mavis (S’- frame) [box car stationary]At t’ = 0, lightning strikes on B and B’:

Some time later, lightning strikes on A and A’:

A’ B’

O’

OA B

u

A’ B’

O’

O B

u

A

Note: 1.platform is length

contracted and the box car’s rest length is longer.

2.Speed of light is the same in both frame according to O’.

Page 17: ch37 young freedman - George Mason Universitycomplex.gmu.edu/.../phys262/soln/ch37_young_freedman3.pdf · 2020. 4. 16. · 'LVWDQFH EHWZHHQ WZR SRLQWV RQ D ULJLG ERG\ 3 4FDQ EH PHDVXUHG

Sequence of Events according to Mavis (S’- frame)

Some time later, the light pulses reach O’

A’ B’

O’

O B

u

A

Page 18: ch37 young freedman - George Mason Universitycomplex.gmu.edu/.../phys262/soln/ch37_young_freedman3.pdf · 2020. 4. 16. · 'LVWDQFH EHWZHHQ WZR SRLQWV RQ D ULJLG ERG\ 3 4FDQ EH PHDVXUHG

Sequence of Events according to Mavis (S’- frame)

A’ B’

O’

OA B

u

Some more time later, the light pulses reach O at the same time but light pulse from A’ still has not reach O’ yet.

Mavis see the flashes at different time but agrees with Stanley that the light signals in Stanley’s frame arrive at him at the same time. Both see the same sequence of events but the notion of simultaneity is relative.

Page 19: ch37 young freedman - George Mason Universitycomplex.gmu.edu/.../phys262/soln/ch37_young_freedman3.pdf · 2020. 4. 16. · 'LVWDQFH EHWZHHQ WZR SRLQWV RQ D ULJLG ERG\ 3 4FDQ EH PHDVXUHG

Ladder | Barn ParadoxPictures from wikipedia

Barn’sFrame

Ladder’sFrame

Page 20: ch37 young freedman - George Mason Universitycomplex.gmu.edu/.../phys262/soln/ch37_young_freedman3.pdf · 2020. 4. 16. · 'LVWDQFH EHWZHHQ WZR SRLQWV RQ D ULJLG ERG\ 3 4FDQ EH PHDVXUHG

Relative Speed of a Spaceship

event 1

S

S’S’

,S x tD D' ', 'S x tD D event 2

' contracted

' /

x prope

x

r

xx D D

D

D'

'

t dilated

t

t proper

tD D D

D ' /

'' /

x x xu u

t t t

D D D D D D

Page 21: ch37 young freedman - George Mason Universitycomplex.gmu.edu/.../phys262/soln/ch37_young_freedman3.pdf · 2020. 4. 16. · 'LVWDQFH EHWZHHQ WZR SRLQWV RQ D ULJLG ERG\ 3 4FDQ EH PHDVXUHG

Summary of Results

u

S

S’

flash a’ flash b’

Time Dilation: (moving clock runs slow)

2 20 , 1 1t t u c D D

Measured by S

Measured by S’

Length Contraction: (moving ruler get shorter)0L L

is measured at the same location wrtS’

0tD

is measured at the same time wrt S’0l

Page 22: ch37 young freedman - George Mason Universitycomplex.gmu.edu/.../phys262/soln/ch37_young_freedman3.pdf · 2020. 4. 16. · 'LVWDQFH EHWZHHQ WZR SRLQWV RQ D ULJLG ERG\ 3 4FDQ EH PHDVXUHG

Numerical Notes1. Keep u in units of c, e.g., 0.8u c since we always have the ratio u/c. Then,

2. Since the ratio u /c occurs so often, it has a special symbol:

2 221 1 0.8 1 1 0.8c c can be calculated simply.

2and 1 1u c

3. Approximation when u << c (low speed: non-relativistic):

Recall Binominal Expansion:

(1 ) 1n n for small.

Page 23: ch37 young freedman - George Mason Universitycomplex.gmu.edu/.../phys262/soln/ch37_young_freedman3.pdf · 2020. 4. 16. · 'LVWDQFH EHWZHHQ WZR SRLQWV RQ D ULJLG ERG\ 3 4FDQ EH PHDVXUHG

Numerical Notes

2 2

1 22 2

1 1

1

u c

u c

3. Approximation when u << c (low speed: non-relativistic):

If u /c is small, will be really small !2 22u c

Problem: calculator might treat 2 21 2u c

Relativistic (u=0.3c) :

simply as 1 and you will loose all significant figures if you combine1 and .2 22u c

2 2 22 0.3 2 0.045

1.24

u c

Non-Relativistic (u=0.003c) : 2 2 22 0.03 2 0.0000045

1.0000045

u c

(quite diff. from 1) (not much diff. from 1)

Typically, if , one should consider speed to be relativistic.0.1u c

2 2

2 2

11 1

2 2

u u

c c

(1 ) 1n n

Page 24: ch37 young freedman - George Mason Universitycomplex.gmu.edu/.../phys262/soln/ch37_young_freedman3.pdf · 2020. 4. 16. · 'LVWDQFH EHWZHHQ WZR SRLQWV RQ D ULJLG ERG\ 3 4FDQ EH PHDVXUHG

Example: Muon Life Time

earth

cosmic rays atom

muon Muon is an unstable elementary particle with:•e-charge•207 Me

Produced by cosmic rays (mostly high energy protons) collide with atoms high up in the atmosphere (>4 km).

In a the rest frame of the muon, it has an average life-time of:

2.2muon s

Without Einstein’s SR, if 0.99muonu c8 6avg. dist. travelled = 0.99(3 10 / )(2.2 10 )

600

m s s

m