Chapter 28: Relativityestrada.cune.edu/facweb/brent.royuk/phys111/docs/Chapter...1 Chapter 28:...

11
1 Chapter 28: Relativity Brent Royuk Phys-111 Concordia University Classical Mechanics Translational Rotational s = r x = vt = t vt = r v = vo + at = o + t at = r x = v o t + 1 2 at 2 θ = ω o t + 1 2 αt 2 v 2 = v o 2 +2 ax ω 2 = ω o 2 + 2αθ F ! τ = ! r × F = rF sin m I = m i r i 2 ! F NET = ! F = m ! a ! τ NET = I ! α W = Fd cosθ W = K TOT = 1 2 mv 2 + 1 2 I ω 2 K = 1 2 mv 2 Krot = 1 2 I ω 2 ! p = m ! v ! L = I ! ω F t = m v t = I P av = ΔE Δt P = Fv P = τω 3 Classical vs. Modern The more important fundamental laws and facts of physical science have all been discovered, and these are now so firmly established that the possibility of their ever being supplanted in consequence of new discoveries is exceedingly remote.... Our future discoveries must be looked for in the sixth place of decimals. - Albert. A. Michelson, speech at the dedication of Ryerson Physics Lab, U. of Chicago 1894

Transcript of Chapter 28: Relativityestrada.cune.edu/facweb/brent.royuk/phys111/docs/Chapter...1 Chapter 28:...

Page 1: Chapter 28: Relativityestrada.cune.edu/facweb/brent.royuk/phys111/docs/Chapter...1 Chapter 28: Relativity Brent Royuk Phys-111 Concordia University Classical Mechanics Translational

1

Chapter 28: Relativity

Brent Royuk Phys-111

Concordia University

Classical Mechanics Translational Rotational

s = r x = vt = t vt = r v = vo + at = o + t

at = r

x = vot +12

at 2 θ = ω ot +

12αt 2

v2 = vo

2 +2 ax ω2 = ω o

2 + 2αθ

! F

! τ =! r ×! F

= rF sin m

I = miri2∑

! F NET =

! F ∑ = m

! a

! τ NET = I

! α

W = Fd cosθ W =

K TOT =

12

mv 2 +12

Iω 2 K =

12

mv 2 Krot =

12

Iω 2

! p = m

! v ! L = I

! ω

F t = m v t = I

Pav =ΔEΔt

P = Fv

P = τω

3

Classical vs. Modern The more important fundamental laws and facts of physical science have all been discovered, and these are now so firmly established that the possibility of their ever being supplanted in consequence of new discoveries is exceedingly remote.... Our future discoveries must be looked for in the sixth place of decimals. - Albert. A. Michelson, speech at the dedication of Ryerson Physics Lab, U. of Chicago 1894

Page 2: Chapter 28: Relativityestrada.cune.edu/facweb/brent.royuk/phys111/docs/Chapter...1 Chapter 28: Relativity Brent Royuk Phys-111 Concordia University Classical Mechanics Translational

2

4

Classical vs. Modern When I began my physical studies [in Munich in 1874] and sought advice from my venerable teacher Philipp von Jolly... he portrayed to me physics as a highly developed, almost fully matured science... Possibly in one or another nook there would perhaps be a dust particle or a small bubble to be examined and classified, but the system as a whole stood there fairly secured, and theoretical physics approached visibly that degree of perfection which, for example, geometry has had already for centuries. - from a 1924 lecture by Max Planck (Sci. Am, Feb 1996 p.10)

5

Classical vs. Modern “There is nothing new to be discovered in physics now. All that remains is more and more precise measurement” -Lord Kelvin, 1900

6

The Correspondence Principle

Text 22178 and your message to 37607 or PollEv.com

Page 3: Chapter 28: Relativityestrada.cune.edu/facweb/brent.royuk/phys111/docs/Chapter...1 Chapter 28: Relativity Brent Royuk Phys-111 Concordia University Classical Mechanics Translational

3

7

Introduction •  What’s relative about relativity?

8

Relativity •  Billy-Bob’s Pickup Truck •  Galilean Relativity •  Inertial Rest Frames

–  A place where Newton’s Laws work. –  A lab on a pickup truck? –  A boxcar? The space shuttle? Earth’s surface?

•  What is light’s reference frame? c = 3 x 108 m/s

•  The search for the luminiferous ether.

9

Relativity

Page 4: Chapter 28: Relativityestrada.cune.edu/facweb/brent.royuk/phys111/docs/Chapter...1 Chapter 28: Relativity Brent Royuk Phys-111 Concordia University Classical Mechanics Translational

4

10

Relativity

11

Relativity

12

Michelson-Morley Experiment

Page 5: Chapter 28: Relativityestrada.cune.edu/facweb/brent.royuk/phys111/docs/Chapter...1 Chapter 28: Relativity Brent Royuk Phys-111 Concordia University Classical Mechanics Translational

5

13

Einstein’s Two Postulates 1.  The Principle of Relativity: The laws of

physics are the same in all inertial frames of reference.

–  Galilean relativity –  There’s no way you can tell you’re moving.

2.  The Invariance of c: The speed of light is the same in all IRFs, independent of relative motion.

–  This is the surprising one. –  Justification? Maxwell and experiment.

•  Herman Bondi: The irrelevance of motion and the uniqueness of light.

•  Special vs. General •  Any objections?

14

The Relativity of Simultaneity •  Gedanken

15

Time Dilation •  The Light Clock Derivation, p. 1001-02

•  Notation: β = v/c •  Result: Δt =γ Δto

γ =1

1 −v2

c2

= 1 − β2( )− 1

2

Page 6: Chapter 28: Relativityestrada.cune.edu/facweb/brent.royuk/phys111/docs/Chapter...1 Chapter 28: Relativity Brent Royuk Phys-111 Concordia University Classical Mechanics Translational

6

16

Time Dilation •  Calculating Gamma

γ =1

1 −v2

c2

= 1 − β2( )− 1

2

17

Time Dilation •  Why dilation? •  Is this a change in measured time or actual time?

•  So which observer is right?

18

Time Dilation •  Example: Given β = 0.8, Sammy the

Spaceman’s watch tics off 10 s. What do our watches say during that interval? –  Proper time = the “moving” clock –  Events and spacetime

•  Four Possible Permutations for Time dilation: –  Sammy’s says 10, what do ours say? –  Ours say 10, what does Sammy’s say? –  Sammy sees ours say 10, what does his say? –  During ten of Sammy’s, how much time does he see

pass on ours? •  Remember the first postulate?

Page 7: Chapter 28: Relativityestrada.cune.edu/facweb/brent.royuk/phys111/docs/Chapter...1 Chapter 28: Relativity Brent Royuk Phys-111 Concordia University Classical Mechanics Translational

7

19

Time Dilation •  Example 28.1: Suppose

a cosmic ray colliding with a nucleus in the Earth’s upper atmosphere produces a muon that has a velocity v = 0.95 c. The muon then travels at constant velocity and lives 1.52 µs as measured in the muon’s frame of reference. (You can imagine this as the muon’s internal clock.) How long does the muon live as measured by an Earth-bound observer?

20

Time Dilation •  Example: Hafele and Keating, 1972: atomic

clocks on commercial airplanes –  Time dilation was verified within 5-10% –  Observed time differences: east: -40 ns, west:

+275 ns. (compared to ground) •  When atomic clocks are transported, they get out of

sync. •  GPS satellites have to be synchronized with time

dilation effects accounted for –  NOVA Episode #2612: On a plane trip to London, a

clock gained 40 ns. •  Joe Hafele: “Suppose you were to live for 100 years

and you would spend your entire life on one of these aircraft, flying around the world, you could expect to be younger than people who did not do that by about one ten-thousandth of a second.”

21

Cultural Manifestations

Page 8: Chapter 28: Relativityestrada.cune.edu/facweb/brent.royuk/phys111/docs/Chapter...1 Chapter 28: Relativity Brent Royuk Phys-111 Concordia University Classical Mechanics Translational

8

22

Cultural Manifestations

23

Cultural Manifestations

24

Cultural Manifestations

Page 9: Chapter 28: Relativityestrada.cune.edu/facweb/brent.royuk/phys111/docs/Chapter...1 Chapter 28: Relativity Brent Royuk Phys-111 Concordia University Classical Mechanics Translational

9

25

Length Contraction •  Measured lengths shrink by the gamma

factor for different reference frames. •  This occurs only along the direction of

relative motion. •  This is not just something that happens

to fast meter sticks. Length is really relative to the observer.

•  Equation: L = Lo/γ •  Example: At what speed would a flying

meter stick appear to be half a meter long?

26

Length Contraction http://www.glenbrook.k12.il.us/gbssci/phys/mmedia/specrel/lc.html

27

Visual Distortion

Page 10: Chapter 28: Relativityestrada.cune.edu/facweb/brent.royuk/phys111/docs/Chapter...1 Chapter 28: Relativity Brent Royuk Phys-111 Concordia University Classical Mechanics Translational

10

28

Length ContractionVisual Appearance: Antony Searle, http://www.anu.edu.au/Physics/Searle/

29

Length ContractionVisual Appearance: Antony Searle, http://www.anu.edu.au/Physics/Searle/

30

Length ContractionVisual Appearance: Antony Searle, http://www.anu.edu.au/Physics/Searle/

Page 11: Chapter 28: Relativityestrada.cune.edu/facweb/brent.royuk/phys111/docs/Chapter...1 Chapter 28: Relativity Brent Royuk Phys-111 Concordia University Classical Mechanics Translational

11

33

Velocity Addition

•  Classically, u = v + u’. •  Relativistically, we get:

u = v + u '

1+ vu 'c2

34

Relativistic Time Travel •  How long would it take to go 100 ly at v = 0.9 c?

•  The Twin Paradox – Bobby and Ricky are twins. When

they are 20 years old, Bobby leaves on a space flight to a star that is 20 light years away, traveling very close to the speed of light. At this extreme speed, the gamma factor for time dilation is equal to 20. What happens?

36

The Pole in a Barn Paradox