Physics 1161: PreLecture 26 Special Relativity 1.

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Presentation transcript:

Physics 1161: PreLecture 26 Special Relativity 1

Inertial Reference Frame Frame which is in uniform motion (constant velocity) No Accelerating No Rotating Technically Earth is not inertial, but it’s close enough. Small distance gives quantum mechanics. High speed gives relativity

Postulates of Relativity Laws of physics are the same in every inertial frame Perform experiment on a moving train and you should get same results as on a train at rest Speed of light in vacuum is c for everyone Measure c=3x108 m/s if you are on train going east or on train going west, even if light source isn’t on the train. On train….can’t tell you are moving. Toss ball back and forth; do collision experiments; etc. Note that constancy of c is not really a separate postulate. Follows from EM theory. Weird!

Relative Velocity (Ball) Example Gordon Beckham throws a baseball @ 90mph. How fast do I think it goes when I am: Standing still relative to Beckham? Running 15 mph towards him? Running 15 mph away from him? 90 mph 90+15=105 mph 90-15=75 mph

Relative Velocity (Light) Example Now he throws a photon (c=3x108 m/s). How fast do I think it goes when I am: Standing still Running 1.5x108 m/s towards him Running 1.5x108 m/s away from him 3x108 m/s 3x108 m/s 3x108 m/s Strange but True!

Consequences: 1. Time Dilation t0 is call the “proper time”. Here it is the time between two events that occur at the same place, in the rest frame.

Time Dilation L=v Dt D D ½ vDt t0 is proper time Because it is rest frame of event 23

Example Time Dilation A + (pion) is an unstable elementary particle. It decays into other particles in 1 x 10-6 sec. Suppose a + is created at Fermilab with a velocity v=0.99c. How long will it live before it decays? If you are riding along with pion, you will see it decay in 1 us. In that frame, birth and death occur at same point and the time interval between them is the proper time If you are moving with the pion, it lives 1 s In lab frame where it has v=0.99c, it lives 7.1 times longer Both are right! This is not just “theory.” It has been verified experimentally (many times!)

Time Dilation Example v/c  0.1 1.005 0.2 1.021 0.5 1.155 0.9 2.294 0.99 7.089 0.999 22.366 0.9999 70.712 0.99999 223.607 0.999999 707.107 0.9999999 2236.068

Consequences II: Length Contraction How do you measure the length of something? If at rest, it is easy—just use a ruler (“proper length”) If moving with velocity v, a harder problem Here is one way to do it v

Length Contraction Set up a grid of clocks at regular intervals, all sychronized Observer A records time when front of train passes All other observers record time when back of train passes Find Observer B who records same time as A Distance between A and B is the length of the train L measured in the frame of the stationary clocks where the train is moving Question: how does L compare with L0, the proper length? v B A

L vs. L0 Tell observer A to flash light when front passes: event 1 Tell observer B to flash light when back passes: event 2 Observer C halfway between A and B sees light flashes simultaneously: concludes events 1 and 2 are simultaneous What about observer D, who is riding at the center of the train? D sees light pulse from A first, then sees light pulse from B He concludes: event 1 occurs before event 2 D v B C A

event 1: light at front flashes event 2: light at back flashes D sees light pulse from A first, then sees light pulse from B He concludes: event 1 occurs before event 2 In words: front of train passes A before back of train passes B Therefore, train is longer than distance between A and B That is, L0>L In the frame in which the train is moving, the length is “contracted” (smaller) D Event 1 Event 2 B A B A

Derive length contraction using the postulates of special relativity and time dilation.

(i) Aboard train (ii) Train traveling to right speed v the observer on the ground sees : send photon to end of train and back Dt1 = (Dx + v Dt1 )/c = Dx/(c-v) Dt2 = (Dx - v Dt2 )/c = Dx/(c+v) Dt = Dt1 + Dt2 = (2 Dx/c ) g2 = Dt0 g - Use time dilation: Dt = Dt0 g 2 Dx0 = c Dt0 = 2 Dx g Dx = Dx0/ g the moving train length is contracted! Dt0 = 2 Dx0 /c

Space Travel Example Alpha Centauri is 4.3 light-years from earth. (It takes light 4.3 years to travel from earth to Alpha Centauri). How long would people on earth think it takes for a spaceship traveling v=0.95c to reach A.C.? How long do people on the ship think it takes? People on ship have ‘proper’ time they see earth leave, and Alpha Centauri arrive. Dt0 Dt0 = 1.4 years

Length Contraction Example People on ship and on earth agree on relative velocity v = 0.95 c. But they disagree on the time (4.5 vs 1.4 years). What about the distance between the planets? Earth/Alpha L0 = v t = .95 (3x108 m/s) (4.5 years) = 4x1016m (4.3 light years) Ship L = v t = .95 (3x108 m/s) (1.4 years) = 1.25x1016m (1.3 light years) Length in moving frame Length in object’s rest frame

Comparison: Time Dilation vs. Length Contraction Dto = time in reference frame in which object is not moving “proper time” i.e. if event is clock ticking, then Dto is in the reference frame of the clock (even if the clock is in a moving spaceship). Lo = length in rest reference frame as object “proper length” length of the object when you don’t think it’s moving. Dt > Dto Time seems longer from “outside” Lo > L Length seems shorter from “outside”

Relativistic Momentum Note: for v<<c p=mv Note: for v=c p=infinity Relativistic Energy Note: for v=0 E = mc2 Note: for v<<c E = mc2 + ½ mv2 Note: for v=c E = infinity (if m is not 0) Objects with mass always have v<c!

Summary Physics works in any inertial frame “Simultaneous” depends on frame Proper frame is where event is at same place, or object is not moving. Time dilates relative to proper time Length contracts relative to proper length Energy/Momentum conserved For v<<c reduce to Newton’s Laws