1. Chapter 37
Relativity

2. Learning Goals for Chapter 37
Looking forward at …
why different observers can disagree about whether two events are simultaneous.
how relativity predicts that moving clocks run slow, and what experimental evidence confirms this.
how the length of an object changes due to the object’s motion.
how the theory of relativity modifies the relationship between velocity and momentum.
some of the key concepts of Einstein’s general theory of relativity.

3. Einstein’s Postulates
Albert Einstein (1879–1955) was only two years old when Michelson reported his first null measurement for the existence of the ether.
At the age of 16 Einstein began thinking about the form of Maxwell’s equations in moving inertial systems.
In 1905, at the age of 26, he published his startling proposal about the principle of relativity, which he believed to be fundamental.

4. The Transition to Modern Relativity
Although Newton’s laws of motion had the same form under the Galilean transformation, Maxwell’s equations did not.
In 1905, Albert Einstein proposed a fundamental connection between space and time and that Newton’s laws are only an approximation.

5. Einstein’s first postulate
Einstein’s first postulate, known as the principle of relativity, states that the laws of physics are the same in every inertial reference frame.
For example, the same emf is induced in the coil whether the magnet moves relative to the coil, or the coil moves relative to the magnet.

6. Inertial Reference Frame
A reference frame is called an inertial frame if Newton laws are valid in that frame.
Such a frame is established when a body, not subjected to net external forces, is observed to move in rectilinear motion at constant velocity.

7. Newtonian Principle of Relativity
If Newton’s laws are valid in one reference frame, then they are also valid in another reference frame moving at a uniform velocity relative to the first system.
This is referred to as the Newtonian principle of relativity or Galilean invariance.

8. Inertial Frames K and K’
K is at rest and K’ is moving with velocity
Axes are parallel
K and K’ are said to be INERTIAL COORDINATE SYSTEMS

9. The Galilean Transformation
For a point P
In system K: P = (x, y, z, t)
In system K’: P = (x’, y’, z’, t’) P x K K’
x’-axis
x-axis

10. Conditions of the Galilean Transformation
Parallel axes
K’ has a constant relative velocity in the x-direction with respect to K
Time (t) for all observers is a fundamental invariant, i.e., the same for all inertial observers

11. The Inverse Relations Step 1. Replace with .
Step 2. Replace “primed” quantities with
“unprimed” and “unprimed” with “primed.”

12. Einstein’s second postulate
Einstein’s second postulate is that the speed of light in vacuum is the same in all inertial frames of reference and is independent of the motion of the source.
Suppose two observers measure the speed of light in vacuum.
One is at rest with respect to the light source, and the other is moving away from it.
According to the principle of relativity, the two observers must obtain the same result, despite the fact that one is moving with respect to the other.

13. The Need for Ether
The wave nature of light suggested that there existed a propagation medium called the luminiferous ether or just ether.
Ether had to have such a low density that the planets could move through it without loss of energy
It also had to have an elasticity to support the high velocity of light waves

14. Maxwell’s Equations
In Maxwell’s theory the speed of light, in terms of the permeability and permittivity of free space, was given by
Thus the velocity of light between moving systems must be a constant.

15. An Absolute Reference System
Ether was proposed as an absolute reference system in which the speed of light was this constant and from which other measurements could be made.
The Michelson-Morley experiment was an attempt to show the existence of ether.

16. The Michelson-Morley Experiment
Albert Michelson (1852–1931) was the first U.S. citizen to receive the Nobel Prize for Physics (1907), and built an extremely precise device called an interferometer to measure the minute phase difference between two light waves traveling in mutually orthogonal directions.
The Michelson Interferometer
AC is parallel to the motion of the Earth inducing an “ether wind”
Light from source S is split by mirror A and travels to mirrors C and D in mutually perpendicular directions
3. After reflection the beams recombine at A slightly out of phase due to the “ether wind” as viewed by telescope E.

17. Typical interferometer fringe pattern expected when the system is rotated by 90°

18. Assuming the Galilean Transformation
The Analysis
Assuming the Galilean Transformation
Time t1 from A to C and back:
Time t2 from A to D and back:
So that the change in time is:

19. Results Using the Earth’s orbital speed as: V = 3 × 104 m/s
together with
ℓ1 ≈ ℓ2 = 1.2 m
So that the time difference becomes
Δt’ − Δt ≈ v2(ℓ1 + ℓ2)/c3 = 8 × 10−17 s
Although a very small number, it was within the experimental range of measurement for light waves.

20. Michelson’s Conclusion
Michelson noted that he should be able to detect a phase shift of light due to the time difference between path lengths but found none.
He thus concluded that the hypothesis of the stationary ether must be incorrect.
After several repeats and refinements with assistance from Edward Morley ( ), again a null result.
Thus, ether does not seem to exist!

21. The Lorentz-FitzGerald Contraction
Another hypothesis proposed independently by both H. A. Lorentz and G. F. FitzGerald suggested that the length ℓ1, in the direction of the motion was contracted by a factor of
…thus making the path lengths equal to account for the zero phase shift.
This, however, was an ad hoc assumption that could not be experimentally tested.

22. Relative velocity of slow-moving objects

23. Relative velocity of light

24. A thought experiment in simultaneity: Slide 1 of 4
Imagine a train moving with a speed comparable to c, with uniform velocity.
Two lightning bolts strike a passenger car, one near each end.

25. A thought experiment in simultaneity: Slide 2 of 4
Stanley is stationary on the ground at O, midway between A and B.
Mavis is moving with the train at in the middle of the passenger car, midway between and .

26. A thought experiment in simultaneity: Slide 3 of 4
Mavis runs into the wave front from before the wave front from catches up to her.
Thus she concludes that the lightning bolt at struck before the one at .

27. A thought experiment in simultaneity: Slide 4 of 4
The two wave fronts from the lightning strikes reach Stanley at O simultaneously, so Stanley concludes that the two bolts struck B and A simultaneously.
Whether or not two events at different locations are simultaneous depends on the state of motion of the observer.

28. Relativity of time intervals
Let’s consider another thought experiment.
Mavis, in frame S', measures the time interval between two events.
Event 1 is when a flash of light from a light source leaves O'.
Event 2 is when the flash returns to O', having been reflected from a mirror a distance d away.
The flash of light moves a total distance 2d, so the time interval is:

29. Relativity of time intervals
The round-trip time measured by Stanley in frame S is a longer interval Δt; in his frame of reference the two events occur at different points in space.

30. Time dilation and proper time
Let Δt0 be the proper time between two events.
An observer moving with constant speed u will measure the time interval to be Δt, where
where the Lorentz factor γ is defined as:

31. The Lorentz factor
When u is very small compared to c, γ is very nearly equal to 1.
If the relative speed u is great enough that γ is appreciably greater than 1, the speed is said to be relativistic.

32. Proper time
Proper time is the time interval between two events that occur at the same point.
A frame of reference can be pictured as a coordinate system with a grid of synchronized clocks, as in the figure at the right.

33. Relativity of length
We attach a light source to one end of a ruler and a mirror to the other end.
The ruler is at rest in reference frame S', and its length in this frame is l0.

34. Relativity of length
In reference frame S the ruler is moving to the right with speed u.
The length of the ruler is shorter in S.

35. Length contraction and proper length
A length measured in the frame in which the body is at rest (the rest frame of the body) is called a proper length.
Thus l0 is a proper length in S', and the length measured in any other frame moving relative to S is less than l0.
This effect is called length contraction.

36. Example of length contraction
The speed at which electrons traverse the 3-km beam line of the SLAC National Accelerator Laboratory is slower than c by less than 1 cm/s.
As measured in the reference frame of such an electron, the beam line (which extends from the top to the bottom of this photograph) is only about 15 cm long!

37. Lengths perpendicular to the direction of motion
There is no length contraction for lengths perpendicular to the direction of relative motion.

38. The Lorentz transformations
This Galilean transformation, as we have seen, is valid only in the limit when u approaches zero.
The more general relationships are called the Lorentz transformations.

39. The Lorentz transformations for coordinates
The Lorentz transformations relate the coordinates and velocities in two inertial reference frames.
They are more general than the Galilean transformations and are consistent with the principle of relativity.

40. The Lorentz transformations for velocities
The Lorentz velocity transformations show us that a body moving with a speed less than c in one frame of reference always has a speed less than c in every other frame of reference.

41. The Lorentz Velocity Transformations
In addition to the previous relations, the Lorentz velocity transformations for u’x, u’y , and u’z can be obtained by switching primed and unprimed and changing v to –v:

42. Experimental Verification
Time Dilation and Muon Decay
Figure 2.18: The number of muons detected with speeds near 0.98c is much different (a) on top of a mountain than (b) at sea level, because of the muon’s decay. The experimental result agrees with our time dilation equation.

43. Atomic Clock Measurement
Figure 2.20: Two airplanes took off (at different times) from Washington, D.C., where the U.S. Naval Observatory is located. The airplanes traveled east and west around Earth as it rotated. Atomic clocks on the airplanes were compared with similar clocks kept at the observatory to show that the moving clocks in the airplanes ran slower.

44. Twin Paradox The Set-up
Twins Mary and Frank at age 30 decide on two career paths: Mary decides to become an astronaut and to leave on a trip 8 light years (ly) from the Earth at a great speed and to return; Frank decides to reside on the Earth.
The Problem
Upon Mary’s return, Frank reasons that her clocks measuring her age must run slow. As such, she will return younger. However, Mary claims that it is Frank who is moving and consequently his clocks must run slow.
The Paradox
Who is younger upon Mary’s return?

45. The Resolution
Frank’s clock is in an inertial system during the entire trip; however, Mary’s clock is not. As long as Mary is traveling at constant speed away from Frank, both of them can argue that the other twin is aging less rapidly.
When Mary slows down to turn around, she leaves her original inertial system and eventually returns in a completely different inertial system.
Mary’s claim is no longer valid, because she does not remain in the same inertial system. There is also no doubt as to who is in the inertial system. Frank feels no acceleration during Mary’s entire trip, but Mary does. Thus, Mary’s trip will be shorter (by the Lorentz factor) and thus she will be younger than Frank upon her return.

46. Spacetime
When describing events in relativity, it is convenient to represent events on a spacetime diagram.
In this diagram one spatial coordinate x, to specify position, is used and instead of time t, ct is used as the other coordinate so that both coordinates will have dimensions of length.
Spacetime diagrams were first used by H. Minkowski in 1908 and are often called Minkowski diagrams. Paths in Minkowski spacetime are called worldlines.

47. Spacetime Diagram

48. Particular Worldlines

49. Worldlines and Time

50. Moving Clocks

51. The Light Cone

52. Spacetime Interval Since all observers “see” the same speed of
light, then all observers, regardless of their
velocities, must see spherical wave fronts.
s2 = x2 – c2t2 = (x’)2 – c2 (t’)2 = (s’)2

53. Spacetime Invariants
If we consider two events, we can determine the quantity Δs2 between the two events, and we find that it is invariant in any inertial frame. The quantity Δs is known as the spacetime interval between two events.

54. Spacetime Invariants
There are three possibilities for the invariant quantity Δs2:
Δs2 = 0: Δx2 = c2 Δt2, and the two events can be connected only by a light signal. The events are said to have a lightlike separation.
Δs2 > 0: Δx2 > c2 Δt2, and no signal can travel fast enough to connect the two events. The events are not causally connected and are said to have a spacelike separation.
Δs2 < 0: Δx2 < c2 Δt2, and the two events can be causally connected. The interval is said to be timelike.

55. Doppler effect for electromagnetic waves
When a source moves toward the observer, the observed frequency f is greater than the emitted frequency f0.

56. Doppler effect for electromagnetic waves
This handheld radar gun emits a radio beam of frequency f0, which in the frame of reference of an approaching car has a higher frequency f.
The reflected beam also has frequency f in the car’s frame, but has an even higher frequency f ' in the police officer’s frame.
The radar gun calculates the car’s speed by comparing the frequencies of the emitted beam and the doubly Doppler-shifted reflected beam.

57. Relativistic Momentum
Because physicists believe that the conservation of momentum is fundamental, we begin by considering collisions where there do not exist external forces and
dp/dt = Fext = 0

58. Relativistic momentum
Shown is a graph of the magnitude of the momentum of a particle of rest mass m as a function of speed v.
Also shown is the Newtonian prediction, p = mv, which gives correct results only at speeds much less than c.

59. Relativistic Momentum
Frank (fixed or stationary system) is at rest in system K holding a ball of mass m. Mary (moving system) holds a similar ball in system K that is moving in the x direction with velocity v with respect to system K.

60. Relativistic Momentum
If we use the definition of momentum, the momentum of the ball thrown by Frank is entirely in the y direction:
pFy = mu0
The change of momentum as observed by Frank is
ΔpF = ΔpFy = −2mu0

61. According to Mary
Mary measures the initial velocity of her own ball to be u’Mx = 0 and u’My = −u0.
In order to determine the velocity of Mary’s ball as measured by Frank we use the velocity transformation equations:

62. Relativistic Momentum
Before the collision, the momentum of Mary’s ball as measured by Frank becomes
Before
For a perfectly elastic collision, the momentum after the collision is
After
The change in momentum of Mary’s ball according to Frank is
(2.42)
(2.43)
(2.44)

63. Relativistic Momentum
The conservation of linear momentum requires the total change in momentum of the collision, ΔpF + ΔpM, to be zero. The addition of Equations (2.40) and (2.44) clearly does not give zero.
Linear momentum is not conserved if we use the conventions for momentum from classical physics even if we use the velocity transformation equations from the special theory of relativity.
There is no problem with the x direction, but there is a problem with the y direction along the direction the ball is thrown in each system.

64. Relativistic momentum
Suppose we measure the mass of a particle to be m when it is at rest relative to us: We call m the rest mass.
When such a particle has a velocity v, its relativistic momentum is:
We can rewrite this in terms of the Lorentz factor of the particle’s rest frame with respect to the rest frame of the system:

65. Relativistic work and energy
Graph of the kinetic energy of a particle of rest mass m as a function of speed v.
Also shown is the Newtonian prediction, which gives correct results only at speeds much less than c.

66. Relativistic energy and rest energy
The relativistic kinetic energy is:
Note that the kinetic energy approaches infinity as the speed approaches the speed of light.
The rest energy is mc2.

67. Relativistic energy and momentum
The total energy of a particle is:
The total energy, rest energy, and momentum are related by:

68. The general theory of relativity
Objects in the space station seem to be weightless, but without looking outside the station there is no way to determine whether gravity has been turned off or whether the station and all its contents are accelerating toward the center of the earth.
If we cannot distinguish experimentally between a uniform gravitational field at a particular location and a uniformly accelerated reference frame, then there cannot be any real distinction between the two.
In the general theory of relativity the geometric properties of space are affected by the presence of matter.

69. What happens when an astronaut drops her watch?
In gravity-free space, the floor accelerates upward at a = g and hits the watch.

70. What happens when an astronaut drops her watch?
On the earth’s surface, the watch accelerates downward at a = g and hits the floor.

71. A two-dimensional representation of curved space