1 PH300 Modern Physics SP11 1/27 Day 5: Questions? Time Dilation Length Contraction Next Week: Spacetime Relativistic Momentum & Energy “I sometimes ask.

Slides:



Advertisements
Similar presentations
Special Relativistic Paradoxes PHYS 206 – Spring 2014.
Advertisements

Lecture 20 Relativistic Effects Chapter Outline Relativity of Time Time Dilation Length Contraction Relativistic Momentum and Addition of Velocities.
Building Spacetime Diagrams PHYS 206 – Spring 2014.
relativity Quantum Classic physics Modern physics.
Theory of Special Relativity
P1X*Dynamics & Relativity : Newton & Einstein Chris Parkes October 2005 Special Relativity Postulates Time Dilation Length Contraction Lorentz Transformation.
Cutnell/Johnson Physics 7th edition
1 PH300 Modern Physics SP11 1/25 Day 4: Questions? Galilean Relativity Michelson-Morley Experiment Postulates of Special Relativity Next Time: Time dilation.
Wednesday, Feb. 4, 2015PHYS , Spring 2014 Dr. Jaehoon Yu 1 PHYS 3313 – Section 001 Lecture #5 Wednesday, Feb. 4, 2015 Dr. Jaehoon Yu Einstein’s.
Derivation of Lorentz Transformations
Physics 311 Special Relativity Lecture 5: Invariance of the interval. Lorentz transformations. OUTLINE Invariance of the interval – a proof Derivation.
1 Length contraction Length measured differs from frame to frame – another consequence of relativistic effect Gedankan experiment again!
Homework #2 3-7 (10 points) 3-15 (20 points) L-4 (10 points) L-5 (30 points)
Theory of Relativity Albert Einstein Physics 100 Chapt 18.
The laws of physics are the same in any inertial (non- accelerating) frame of reference Galileo & Einstein would both agree (at terrestrial speeds.) F=ma.
Chapter 37 Special Relativity. 37.2: The postulates: The Michelson-Morley experiment Validity of Maxwell’s equations.
Time Dilation, Length Contraction and Doppler
Special Relativity. Topics Motion is Relative Michelson-Morley Experiment Postulates of the Special Theory of Relativity Simultaneity Spacetime Time Dilation.
PH300 Modern Physics SP11 “The only reason for time is so that everything doesn’t happen at once.” - Albert Einstein 2/1 Day 6: Questions? Spacetime Addition.
Further Logistical Consequences of Einstein’s Postulates
Special Relativity Physics 1161: Lecture 35 Sections 29-1 – 29-6.
Announcements Homework: Supplemental Problems 2 nd Project is due at the final exam which is Tuesday May 5 at 1:30 – 3:30pm. A list of potential projects.
Introduction to special relativity
Special Theory of Relativity
Page 1 Phys Baski Relativity I Topic #9: Special Relativity I Transformation of Variables between Reference Frames –Non-relativistic Galilean Transformation.
Special relativity.
1 1.Einstein’s special relativity 2.Events and space-time in Relativity 3. Proper time and the invariant interval 4. Lorentz transformation 5. Consequences.
Announcements Homework Set 1 is due now. I will accept the homework if placed in my mailbox by 5:00pm today Solution to HW Set 1 will be posted soon (Friday?)
25 September 2001Astronomy 102, Fall The world’s most famous patent clerk, c Today in Astronomy 102: relativity, continued  Einstein’s procedures.
Special Relativity The Failure of Galilean Transformations
USC2001 Energy Lecture 4 Special Relativity Wayne M. Lawton Department of Mathematics National University of Singapore 2 Science Drive 2 Singapore
Physics 2170 – Spring Einstein’s theory of special relativity First homework assignment is online. You.
1 1.Einstein’s special relativity 2.Events and space-time in Relativity 3. Proper time and the invariant interval 4.Lorentz transformation Einstein’s special.
Time Dilation We can illustrate the fact that observers in different inertial frames may measure different time intervals between a pair of events by considering.
Physics 2170 – Spring Special relativity Homework solutions are on CULearn Remember problem solving sessions.
Physics 2170 – Spring Special relativity Homework solutions are on CULearn Remember problem solving sessions.
Modern Physics Relativity 1 Space is defined by measurements of length and depends on what “ruler” is used to measure the length. Time is defined by measurements.
The Theory of Special Relativity. Learning Objectives  Einstein’s two postulates in his theory of special relativity: The principle of relativity. (Same.
My Chapter 26 Lecture.
1 Relativity  H3: Relativistic kinematics  Time dilation  Length contraction.
Physics 1202: Lecture 19 Today’s Agenda Announcements: –Lectures posted on: –HW assignments, etc.
Physics 2170 – Spring Einstein’s theory of special relativity Homework was due at 12:50pm today in the.
Consequences of Special Relativity Simultaneity: Newton’s mechanics ”a universal time scale exists that is the same for all observers” Einstein: “No universal.
Module 1Newtonian Relativity1 Module 1 Newtonian Relativity What do we mean by a “theory of relativity”? Let’s discuss the matter using conventional terminology.
Physics 2170 – Spring Special relativity Homework solutions will be on CULearn by 5pm today. Next weeks.
Chapter 39 Relativity. A Brief Overview of Modern Physics 20 th Century revolution 1900 Max Planck Basic ideas leading to Quantum theory 1905 Einstein.
R1 Everything should be made as simple as possible, but not simpler -A. Einstein.
1 PHYS 3313 – Section 001 Lecture #5 Wednesday, Sept. 11, 2013 Dr. Jaehoon Yu Time Dilation & Length Contraction Relativistic Velocity Addition Twin Paradox.
Chapter 1 Relativity 1.
Derivation of Lorentz Transformations Use the fixed system K and the moving system K’ At t = 0 the origins and axes of both systems are coincident with.
Galileo’s Relativity: Text: The laws of mechanics are the same in all inertial reference frames. More general: The laws of mechanics are the same in all.
Lecture 5: PHYS344 Homework #1 Due in class Wednesday, Sept 9 th Read Chapters 1 and 2 of Krane, Modern Physics Problems: Chapter 2: 3, 5, 7, 8, 10, 14,
By: Jennifer Doran. What was Known in 1900 Newton’s laws of motion Maxwell’s laws of electromagnetism.
Special Relativity (Math)  Reference from Tipler chapter 39-1 to 39-3  Newtonian relativity  Einstein’s postulates  Lorentz transformation  Time dilation.
PHYS 342: More info The TA is Meng-Lin Wu: His is His office hour is 10:30am to 12pm on Mondays His office is Physics.
Relativity Part III If twin Astrid aged 10 years during her high-speed trip and Eartha aged 50 years, what is gamma ? What is u ? Ans: γ=5, u~0.980c Twin.
Some places where Special Relativity is needed
Administrative Details: PHYS 344
Wacky Implications of Relativity
PHYS 3313 – Section 001 Lecture #6
Quiz_09 Relativity – simultaneity, time dilation, length contraction
Lecture 4: PHYS 344 Homework #1 Due in class Wednesday, Sept 9th Read Chapters 1 and 2 of Krane, Modern Physics Problems: Chapter 2: 3, 5, 7, 8, 10, 14,
Classical Physics “Inertial Reference Frame” (Section 5.2):
Einstein’s Relativity Part 2
Physics 1161: Lecture 26 Special Relativity Sections 29-1 – 29-6.
RELATIVITY III SPECIAL THEORY OF RELATIVITY
Special Relativity Chapter 1-Class2
Special Relativity Chapter 1-Class3.
Chapter 37 Special Relativity
Special Relativity Chapter 1-Class4.
Presentation transcript:

1 PH300 Modern Physics SP11 1/27 Day 5: Questions? Time Dilation Length Contraction Next Week: Spacetime Relativistic Momentum & Energy “I sometimes ask myself how it came about that I was the one to develop the theory of relativity. The reason, I think, is that a normal adult never stops to think about problems of space and time. These are things which he has thought about as a child. But my intellectual development was retarded, as a result of which I began to wonder about space and time only when I had already grown up.” - Albert Einstein

2 Today: Time dilation, length contraction Next week: Spacetime, relativistic momentum & energy  E=mc 2 !! Exam I – Thursday, Feb. 10 Reminder: HW02 due, beginning of class; HW03 assigned Last time: Galilean relativity Michelson-Morley Experiment & Postulates of SR

L R 0 v L R v L R v L R v L R Lucy: in the trainRicky: on the platform 0 Event L: (x=-3, t=3s) Event R: (x=+3, t=3s) Event L’: (x’=-2, t’=2s) Event R’: (x’=+5, t’=4s) x’x v L R Lucy says: ‘Simultaneous!’ Ricky says: ‘Not simultaneous!’ Recall from last time: Events are recorded by local observers with synchronized clocks. Event 1 (firecracker explodes) occurs at x=x’=0 and t=t’=0

Same location …refers to the time measured by a clock in an inertial frame where it is at rest. Example: Any given clock never moves with respect to itself. It keeps proper time for itself in its own rest frame. Any observer moving with respect to this clock sees it run slow (i.e., time intervals are longer). This is time dilation. Mathematically: Event 1: (x 1,y 1,z 1,t 1 ) Event 2: (x 1,y 1,z 1,t 2 )  Proper time is the shortest time that can be recorded between two events. Proper Time

Speed of light An observer and a ball are at rest in reference frame S. At t = 0, the observer in S flashes a light pulse to be received at x = 3 m. At Δt = 10 ns, the light is received. Observer S measures a distance Δx = 3 m, so the speed of light in frame S is: x S

Comparing inertial frames S’ is moving with respect to S at v = 0.2 m/ns. At t = 0, observer in S flashes a light pulse to be received at x = 3 m x v x’

Ten nanoseconds later S’ is moving with respect to S at v = 0.2 m/ns. At Δt = 10 ns, the light is received. In Galilean relativity, how far does the observer in S’ think the light has traveled? a) 3 mb) 2 m c) 1 md) 0 m v

Ten nanoseconds later S’ is moving with respect to S at v = 0.2 m/ns. At Δt=10 ns, the light is received. In Galilean relativity, (Δt=Δt’) the observer in S’ would therefore measure the speed of light as v Uh-oh!

If we are to believe Einstein’s postulate, then: In frame S In frame S’ Conclusion: Since we accepted Einstein's postulate of relativity (‘c’ is the same in all inertial frames) and we found that, we conclude that. I.e., time passes at different rates in the two frames of reference!!

Another argument for time dilation Mirror Lucy h v Lucy measures the time interval: Δ t = 2h / c (Not a big surprise!)

Mirror h Ethel Ricky v Note: This experiment requires two observers. Another argument for time dilation

Ethel Ricky h v · Δt’ / 2 c · Δt’ / 2 Another argument for time dilation

Ethel Ricky h v · Δt’ / 2 c · Δt’ / 2 Ethel and Ricky measure the time interval: But Lucy measured Δt = 2h/c !! Another argument for time dilation

Time dilation in moving frames Lucy measures: Δt Ethel and Ricky: Δt’ = γΔt, with The γ- factor can take on what values? A)B)C) D)E) Something else…

Time dilation in moving frames Lucy measures: Δt Ethel and Ricky: Δt’ = γΔt, with For Lucy time seems to run slower! (Lucy is moving relative to Ethel and Ricky) Δt’ = γΔt ≥ Δt

What we found so far: Simultaneity of two events depends on the choice of the reference frame Lucy v L R … Ricky Lucy concludes: Light hits both ends at the same time. Ricky concludes: Light hits left side first.

Time Dilation: Two observers (moving relative to each other) can measure different durations between two events. Lucy h Lucy measures: Δ t = 2h / c h Ethel Ricky v Ethel and Ricky: Δt’ = γ 2h / c with Here: Δt =Δτ is the proper time What we found so far:

Are your clocks really synchronized? (I know mine are!)

Ricky Lucy v LR Now Lucy and Ricky each have a set of clocks. Lucy’s are synchronized in her frame (the train), while Ricky’s are synchronized in his frame (the tracks). How do the clocks of one frame read in another frame?

Ricky v LR At 3 o’clock in Ricky’s frame, two firecrackers go off to announce the time. It so happens that these firecrackers are at the left and right ends of the train, in Ricky’s frame. Event 1: firecracker 1 explodes at 3:00 Event 2: firecracker 2 explodes at 3:00 Lucy

Ricky Lucy v LR Event 1: firecracker 1 explodes at 3:00 Event 2: firecracker 2 explodes at 3:00 When Lucy sees each flash from the two firecrackers, she sees that Ricky’s clocks both read 3:00 when each of the firecrackers went off.

Ricky Sometime later, the wavefronts meet. The meeting point is halfway between the firecrackers in Ricky’s frame, but is somewhere toward the left in the train car, in Lucy’s frame. Event 3: two light pulses meet, shortly after 3:00. Lucy v LR v LR v LR v LR

RL Ricky The situation as seen by Lucy

RL Lucy Ricky The situation as seen by Lucy

RL Lucy Ricky The situation as seen by Lucy

RL Lucy Ricky The situation as seen by Lucy

RL Lucy Ricky The situation as seen by Lucy

RL Lucy Ricky The situation as seen by Lucy

Lucy LR Ricky In Lucy’s frame, light left first from the right end of the car. The light pulses both show clocks reading 3:00 in Ricky’s frame. According to Lucy’s reference frame, which of the following is true: A) Ricky’s clock on the left reads a later time than Ricky’s clock on the right. B) Ricky’s clock on the right reads a later time than Ricky’s clock on the left. C) Both of Ricky’s clocks read the same time.

Lucy LR Ricky In Lucy’s frame:

Important conclusion S Clocks in S’ (synchronized in S’) moving to the left with respect to S v If this clock reads 3:00 in S, then: This clock reads a little after 3:00 in S This clock reads even a little later in S S’ Even though the clocks in S’ are synchronized (in S’) the observer in S sees each clock showing a different time!! Clocks in S’ as seen by observer in S

Length of an object This stick is 3m long. I measure both ends at the same time in my frame of reference. “Same time” or not doesn’t actually matter here, because the stick isn’t going anywhere. This length, measured in the stick’s rest frame, is its proper length.

‘Proper length’ Proper length: Length of object measured in the frame where it is at rest (use a ruler)

Remember ‘proper time’ Proper time: Time interval between two events measured in the frame where the two events occur at the same spatial coordinate, i.e. a time interval that can be measured with one clock. v

Length of an object Observer in S measures the proper length L of the blue object. Another observer comes whizzing by at speed v. This observer measures the length of the stick, and keeps track of time. S Event 1 – Origin of S’ passes left end of stick. 0 v S’

Length of an object S 0 v S’ Event 1 – Origin of S’ passes left end of stick. Event 2 – Origin of S’ passes right end of stick.

A little math In frame S: (rest frame of the stick) length of stick = L (this is the proper length) time between events = Δt speed of frame S’ is v = L/Δt In frame S’: length of stick = L’ (this is what we’re looking for) time between events = Δt’ speed of frame S is -v = -L’/Δt’ Q: a)  Δt = Δt’ b) Δt = Δt’ c) Δt’ =  Δt Follow the proper time! S v S’

A little math Speeds are the same (both refer to the relative speed). And so Length in moving frame Length in stick’s rest frame (proper length) Length contraction is a consequence of time dilation (and vice-versa).

The Lorentz transformation 0 v S’ S A stick is at rest in S’. Its endpoints are the events (x,t) = (0,0) and (x’,0) in S’. S’ is moving to the right with respect to frame S. Event 1 – left of stick passes origin of S. Its coordinates are (0,0) in S and (0,0) in S’. x’

Lorentz transformation v S As viewed from S, the stick’s length is. Time t passes. According to S, where is the right end of the stick? (Assume the left end of the stick was at the origin of S at time t=0.) A)B)C) D) E) Something else… x An observer at rest in frame S sees a stick flying past him with velocity v: 0 x’ S’

The Lorentz transformation S This relates the spatial coordinates of an event in one frame to its coordinates in the other. Algebra 0 x’ S’ v

Transformations If S’ is moving with speed v in the positive x direction relative to S, then the coordinates of the same event in the two frames are related by: Note: This assumes (0,0,0,0) is the same event in both frames. Galilean transformation (classical) Lorentz transformation (relativistic)

A note of caution: The way the Lorentz and Galileo transformations are presented here assumes the following: An observer in S would like to express an event (x,y,z,t) (in his frame S) with the coordinates of the frame S', i.e. he wants to find the corresponding event (x',y',z',t') in S'. The frame S' is moving along the x-axes of the frame S with the velocity v (measured relative to S) and we assume that the origins of both frames overlap at the time t=0. S x z y S' x' z' y' v (x,y,z,t) (x',y',z',t')

Transformations If S’ is moving with speed v in the positive x direction relative to S, then the coordinates of the same event in the two frames are related by: Galilean transformation (classical) Lorentz transformation (relativistic)

George has a set of synchronized clocks in reference frame S, as shown. Lucy is moving to the right past George, and has (naturally) her own set of synchronized clocks. Lucy passes George at the event (0,0) in both frames. An observer in George’s frame checks the clock marked ‘?’. Compared to George’s clocks, this one reads v ? George Lucy A) a slightly earlier time B) a slightly later time C) same time

The event has coordinates (x = -3, t = 0) for George. In Lucy’s frame, where the ? clock is, the time t’ is, a positive quantity v ? George Lucy ‘?’ = slightly later time

Spacetime Diagrams (1D in space) In PHYS I: x v t x ΔxΔx ΔtΔt v = Δx / Δt

Spacetime Diagrams (1D in space) In PH300: t x x t c ·

Spacetime Diagrams (1D in space) In PH300: x t c·c· object moving with 0<v<c. ‘Worldline’ of the object x c·t object at rest at x= x c·t object moving with v = -c. x=0 at time t=0 object moving with 0>v>-c

Lucy L R Ricky Recall: Lucy plays with a fire cracker in the train. Ricky watches the scene from the track. v

Example: Lucy in the train L R x ct In Lucy’s frame: Walls are at rest Light travels to both walls Light reaches both walls at the same time. Lucy concludes: Light reaches both sides at the same time

Example: Ricky on the tracks L R x ct In Ricky’s frame: Walls are in motion Ricky concludes: Light reaches left side first.

v=0.5c S S’ Frame S’ is moving to the right at v = 0.5c. The origins of S and S’ coincide at t=t’=0. Which shows the world line of the origin of S’ as viewed in S? ct x x x x ABCD

Frame S’ as viewed from S x ct ct’ This is the time axis of the frame S’ x’ This is the space axis of the frame S’ These angles are equal

Frame S’ as viewed from S x ct ct’ x’ Both frames are adequate for describing events – but will give different spacetime coordinates for these events, in general. In S: (3,3) In S’: (1.8,2)