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http://www.zamandayolculuk.com/cetinbal/timetravelscience.htm PHY100S Lecture 15 http://www.zamandayolculuk.com/cetinbal/htmldosya1/twinparadox-2.htm PHY100S (K. Strong) - Lecture 15 - Slide 1

Current Assignments... For today Read Sections 10.6-10.7 For Lecture 16 Read Sections 10.8, 11.1 Office hours: 3-4 Tuesdays & Thursdays Homework #3 (new due date) Handed out February 14, due FRIDAY, MARCH 8 Writing Assignment #2 Handed out Feb. 28. Due 11:00 AM, Thurs., April 4 Suggested Conceptual Exercises Chapter 10: 21,25,27,31,35,37,39,41,43,47,49,51 Tutorial #7 PHY100S (K. Strong) - Lecture 15 - Slide 2

Review of Lecture 14 Textbook, Sections 10.5-10.6 More on the speed of light The relativity of time - time dilation Time travel Rule: Moving clocks run slow. Time is relative it depends on the relative speed of the clock and the observer. T (1 T o v 2 c 2 ) T T o so T To PHY100S (K. Strong) - Lecture 15 - Slide 3

Plan for Lecture 15 Textbook, Sections 10.6-10.7 Time travel The relativity of space length contraction The relativity of mass PHY100S (K. Strong) - Lecture 15 - Slide 4

From L14: How fast do Mort and Velma age? If Velma passes Mort at 75% of lightspeed, then Mort and his descendants see Velma age 120 years during his 80-year lifetime. She lives for 120 years as measured by Mort s clock. He sees her age slowly, by 1 yr for each of his 1.5 yrs. He dies after 80 of his years and she dies after 120 of Mort s years, but she looks like an 80-year-old. Velma and her descendants see Mort age 120 years during her 80-year lifetime. And both are correct! Each will see the other age more slowly. PHY100S (K. Strong) - Lecture 15 - Slide 5

The Twin Paradox ** ** actually it is NOT a paradox Now, suppose Mort stays on Earth while Velma takes a long trip in space at close to the speed of light. When Velma returns to Earth, she is (A) older than Mort (B) younger than Mort (C) the same age as Mort What happened to special relativity?! It only applies to unaccelerated motion. In order for Velma to go away and come back, she had to accelerate (three times). PHY100S (K. Strong) - Lecture 15 - Slide 6

The Twin Paradox How is this different from the previous example? Velma has accelerated. Velma and Mort begin and end in the same reference frame (Earth). When they are back together, they must agree on who is older because there is only a single time in that reference frame. Mort does not accelerate, so the Special Theory of Relativity does apply ppy to his observations: If Velma s trip takes 60 years measured in Mort s reference frame, he sees only 40 of her years pass. When she returns, he is 60 and she is 40. He sees her age slowly, by 1 yr for each of his 1.5 yrs. PHY100S (K. Strong) - Lecture 15 - Slide 7

Time Travel Velma has traveled into the future at least, into Mort s future. It s a one way trip, though there s no way to go back. So time dilation allows time travel. But only time travel into the future is possible. PHY100S (K. Strong) - Lecture 15 - Slide 8

Concept Check 8 It is physically possible for your mother to leave Earth after you were born and return: (A) before you were born (B) before she was born (C) younger than you (D) older than you (E) younger than she was when she left (F) older than she was when she left PHY100S (K. Strong) - Lecture 15 - Slide 9

What Is Space? Space is something we measure with rulers. How can we measure the length of a moving object? There are two ways. (1) Measure the position of both ends of the object simultaneously, i.e., with two clocks. Otherwise the object will move while measured (2) Measure the time it takes for the object to pass a certain point, and use the speed to find the length. PHY100S (K. Strong) - Lecture 15 - Slide 10

Measuring Length Velma is again in the spaceship moving relative to Mort. Again, the situation is symmetric: Mort s window is shorter as measured by Velma. Textbook Figure 10.10 The window in Velma s spaceship as measured by Velma. The window in Velma s spaceship as measured by Mort. PHY100S (K. Strong) - Lecture 15 - Slide 11

Length Contraction No matter how we measure length, we find the same result: lengths in the direction of motion are contracted. L L o (1 v 2 c 2 ) L Textbook o / L o so L L o where L o = object s rest length, Figure 10.1111 L = object s length when moving at v PHY100S (K. Strong) - Lecture 15 - Slide 12

Length Contraction Animations Try these at home yourself: Relativistic length contraction http://www.physicsclassroom.com/mmedia/ specrel/lc.cfmcfm http://www.upscale.utoronto.ca/pvb/harris on/specrel/flash/lengthcontract.htmlhtml Online tutorial showing time dilation and length contraction http://physics.ucsc.edu/~snof/tutorial/index.html PHY100S (K. Strong) - Lecture 15 - Slide 13

The Relativity of Space Suppose that Velma observes Mort's car as she passes it at 60% of lightspeed. She passes lengthwise over the car. Mort's car is 4 meters long as measured by Mort. How long is it as measured by Velma? (A) 0.8 meters The length (B) 3.2 meters contraction factor (C) 4 meters is 0.8 for 60% of lightspeed. PHY100S (K. Strong) - Lecture 15 - Slide 14

Back to Newton s Second Law a = F/m predicts that a constant force will give a constant acceleration This implies that there is no maximum speed. This cannot be correct! Relativity alters Newton s Law of Motion. The relativity of time means that accelerations differ from one frame to another. Moving objects are observed to accelerate more slowly for the same force. PHY100S (K. Strong) - Lecture 15 - Slide 15

More Mort and Velma Imagine that Mort and Velma each have a 1 kg book, and that Velma is moving past Mort. If Mort pushes his book with a 1 N force, it will accelerate at 1 m/s 2. If Mort pushes on Velma s moving book with a 1Nf force, Newton s Second Law predicts that it will accelerate at 1 m/s 2. Relativity predicts that it will accelerate at less than 1 m/s 2 (as seen by Mort). PHY100S (K. Strong) - Lecture 15 - Slide 16

m The Relativity of Mass If the same force yields a smaller acceleration, the mass must be larger. Therefore, mass is also relative. Moving masses appear to heavier than those at rest. We call the mass of an object in its own reference frame (not moving) its rest mass. This is a constant for any particular object. ( 1 m v o 2 c 2 ) so m m o m o m o = object s rest mass, m = object s mass when moving at v PHY100S (K. Strong) - Lecture 15 - Slide 17

This diagram shows time dilation, mass increase, and length contraction as the speed approaches the speed of light: - duration of 1 sec on a moving clock - length of a moving meter stick - mass of a moving standard kilogram Time dilation and mass increase Textbook Figure 10.12 Length contraction PHY100S (K. Strong) - Lecture 15 - Slide 18

Our last Mort and Velma question As measured by Velma, her spaceship has a mass of 10,000 kg and a length of 100 m. She moves at 80% of lightspeed relative to Mort. According to Mort's measurements, the mass and length of her spaceship are: (A) 16,500 kg, 165 m (B) 6000 kg, 60 m (C) 6000 kg, 165 m (D) 16,500 kg, 60 m (E) This question cannot be answered without t knowing which observer is really at rest. For 80% of lightspeed, the mass increase factor is 1.65 and the length contraction factor is 0.60. PHY100S (K. Strong) - Lecture 15 - Slide 19