Massachusetts Institute of Technology Physics Department

Similar documents
Massachusetts Institute of Technology Physics Department

Physics 8.20 Special Relativity IAP 2008

Massachusetts Institute of Technology Physics Department

Massachusetts Institute of Technology Physics Department Physics 8.20 IAP 2005 Introduction to Special Relativity

(ii) Determine, according to an observer in one of the spaceships, the speed of the other spaceship.

Chapter 1. Relativity 1

Massachusetts Institute of Technology Department of Physics. Physics Out: Friday 29 September 2006 Due: Friday 6 October 2006.

Survey of Astrophysics A110

Spacetime diagrams and Bondi s k-calculus

Astronomy 1 Fall 2016

PHYSICS - CLUTCH CH 34: SPECIAL RELATIVITY.

Relativity. An explanation of Brownian motion in terms of atoms. An explanation of the photoelectric effect ==> Quantum Theory

where = observed wavelength when v = 0

Special Relativity. Principles of Special Relativity: 1. The laws of physics are the same for all inertial observers.

dt = p m, (2.1.1) dt = p

Massachusetts Institute of Technology Physics Department

Advantages of Three-Dimensional Space-Time Frames

Lecture 9 - Applications of 4 vectors, and some examples

Massachusetts Institute of Technology

Massachusetts Institute of Technology Physics Department. Midterm

Particle Physics (concise summary) QuarkNet summer workshop June 24-28, 2013

Recapitulate. Prof. Shiva Prasad, Department of Physics, IIT Bombay

Inflation, vacua and the end of the Universe

Massachusetts Institute of Technology Physics Department. Physics 8.20 IAP 2005 Special Relativity January 28, 2005 FINAL EXAM

Modern Physics. Third Edition RAYMOND A. SERWAY CLEMENT J. MOSES CURT A. MOYER

Astronomy 421. Lecture 24: Black Holes

Special relativity, 3. How big is gamma? The Lorentz transformations depend on the factor γ =

Lecture 13 Notes: 07 / 20. Invariance of the speed of light

2.6 Invariance of the Interval

Simultaneity, Time Dilation, and Length Contraction Using Minkowski Diagrams and Lorentz Transformations

Experimental Values of Lorentz Transformations of Mass and Time

Propagation in the Galaxy 2: electrons, positrons, antiprotons

Lorentz Transformations and the Twin Paradox By James Carter

Relativity and Black Holes

12:40-2:40 3:00-4:00 PM

Test 3 results B A. Grades posted in Learn

The Lorentz Transformations

PHYS 280 Midterm α Fall You may answer the questions in the space provided here, or if you prefer, on your own notebook paper.

PHYSICS 252 EXPERIMENT NO. 11 THE DYNAMICS OF ELEMENTARY PARTICLES

Rotational Mechanics and Relativity --- Summary sheet 1

Before we work on deriving the Lorentz transformations, let's first look at the classical Galilean transformation.

Wallace Hall Academy

1. Convective throughout deliver heat from core to surface purely by convection.

Special Theory of Relativity. PH101 Lec-2

Gravity and Spacetime: Why do things fall?

Postulates of Special Relativity

Experimental Values of Lorentz Transformations of Mass and Time

Introduction. Classical vs Modern Physics. Classical Physics: High speeds Small (or very large) distances

Astronomy 1143 Homework 1

Black Holes -Chapter 21

Physics Quarknet/Service Learning

ENTER RELATIVITY THE HELIOCENTRISM VS GEOCENTRISM DEBATE ARISES FROM MATTER OF CHOOSING THE BEST REFERENCE POINT. GALILEAN TRANSFORMATION 8/19/2016

General Relativity. on the frame of reference!

LECTURE 3: SPACETIME AND GEOMETRY: AN INTRODUCTION TO SPECIAL RELATIVITY. AS204 February

Special Relativity: What Time is it?

Astronomy 182: Origin and Evolution of the Universe

Review Special Relativity. February 3, Absolutes of Relativity. Key Ideas of Special Relativity. Path of Ball in a Moving Train

Cosmic Rays. This showed that the energy of cosmic rays was many times that of any other natural or artificial radiation known at that time.

Consequences of special relativity.

Homework 11. Relativity Problems PH3110 Fall 2006 Due 12/6/06

Analysis of a bubble chamber picture

Quantum Black Hole and Information. Lecture (1): Acceleration, Horizon, Black Hole

Consequences of special relativity.

Observations versus Measurements

Simultaneity And Time Dilation

Analysis of a bubble chamber picture

Prelims 1997 Question 6

Relativity. Physics April 2002 Lecture 8. Einstein at 112 Mercer St. 11 Apr 02 Physics 102 Lecture 8 1

The spacetime of special relativity

The result is; distances are contracted in the direction of motion.

Chapter S3 Spacetime and Gravity. Agenda. Distinguishing Crackpots

Changing coordinates - the Lorentz transformation

The Foundations of Special Relativity

MASSACHUSETTS INSTITUTE OF TECHNOLOGY Physics Department. Problem Set 5 Solutions

Special and General Relativity (PHZ 4601/5606) Fall 2018 Classwork and Homework. Every exercise counts 10 points unless stated differently.

Midterm Solutions. 1 1 = 0.999c (0.2)

Final Exam - Solutions PHYS/ECE Fall 2011

Lecture 8. CPT theorem and CP violation

- Synchrotron emission: A brief history. - Examples. - Cyclotron radiation. - Synchrotron radiation. - Synchrotron power from a single electron

UNIVERSITY OF SURREY SCHOOL OF PHYSICS AND CHEMISTRY DEPARTMENT OF PHYSICS

Recall from last time

LIGHT and SPECIAL RELATIVITY RELATIVISTIC MASS, MOMENTUM and ENERGY

Welcome back to PHY 3305

Potentially useful formulas: F = G m 1m 2 r 2 F = k q 1q 2 F = ma Distance = Speed Time

Topics: Relativity: What s It All About? Galilean Relativity Einstein s s Principle of Relativity Events and Measurements

Chapter 36 The Special Theory of Relativity. Copyright 2009 Pearson Education, Inc.

1st Year Relativity - Notes on Lectures 3, 4 & 5

Special Relativity: Derivations

SPECIAL RELATIVITY. Introduction:

) 2 = Square of rest energy. E = "m o. c 2, or E = mc 2. Homework & Exam

Light and Relativity

Astronomy 1143 Quiz 2 Review

Tensors and Special Relativity

Introduction to General Relativity

The Twins Paradox. The Twins Paradox p. 1/1

A. B. Lahanas University of Athens, Physics Department, Nuclear and Particle Physics Section, Athens , Greece

The ATLAS Experiment and the CERN Large Hadron Collider

FALL 2004 Final Exam, Part A

Physics 180B Test Points. a. 3/2c b. c c. 15/16c d. 24/25c

8. The Expanding Universe, Revisited

Transcription:

Massachusetts Institute of Technology Physics Department Physics 8.20 IAP 2005 Introduction to Special Relativity Problem Set 2 1. A Lorentz transformation The origins of two inertial frames, Σ and Σ, coincide at t = t = 0. The origin of Σ moves at speed u = 1.8 10 8 m/sec along the positive z axis in Σ. An event occurs at x = 1m, y = 3m, z = 2m and t = 8 sec as observed in Σ. Where and when does this event occur in Σ? [To simplify the algebra, you can take c = 3 10 8 m/sec.] 2. Lorentz transformations are rotations through imaginary angles French 3, p. 87, Problem 3 9. 3. Spacetime diagrams I French 3, p. 87, Problem 3 8. 4. A Moving Clock A clock moves along the x axis in your reference frame at a speed of 0.80c and reads zero as it passes the origin. What time does it read as it passes the 180 meter mark on this axis? How much time has passed in your reference frame? 5. Spacetime diagrams II A space traveler sets off to explore a star 96 light years from Earth. She accelerates rapidly to v = 0.96c, and travels in a straight line. After 100 years (as measured on Earth) she quickly decelerates to v = 0 and explores the star for 20 years. Then she returns to earth by quickly reaccelerating to v = 0.96c, travelling for 100 years and decelerating as she approaches the Earth. Draw a spacetime diagram showing the space traveler s worldline from the point of view of an observer on the Earth. Measure time in years and distance in light years. 6. Moon contraction By what amount is the Moon shortened along its diameter (as measured by an observer at rest relative to the Earth) owing to its orbital motion around the Earth? [You can take the orbital velocity of the Moon to be 0.75 km/sec and its radius to be 1722 km.] 7. How fast a ship? A spaceship is moving at such a speed in the laboratory frame that its measured length is one third its proper length. How fast is the spaceship moving relative to the laboratory frame? 8. Cosmic neutrons? Cosmic rays are particles from interstellar space that impact on our atmosphere, making extensive showers of secondary particles that can be measured in detectors which observe the ionization they create as they descend through our atmosphere. Most cosmic rays are protons or photons. The showers made by protons and photons

2 can be distinguished: the ones made by photons contain many more electrons, for example. A few years ago a puzzling phenomenon was observed: cosmic rays of the proton type appeared to be coming from a bizarre object known as Cygnus X3. The reason this was puzzling was that protons travel on helical paths on their way to Earth in response to interstellar magnetic fields. They would not appear to point back to their source. Scientists looked around for other particles that satisfied three conditions: They had to be stongly interacting, so they could make proton type showers. They had to be electrically neutral, so they would not be bent by interstellar magnetic fields. They would have to live long enough to make it from their source to Earth. One obvious candidate is the neutron. It has an average lifetime of 885.7±0.8 sec. (a) Assuming the distance to Cygnus X3 is 10,000 lyr, what is the minimum speed that a neutron must be travelling so that it could make it to Earth in its own proper lifetime? (b) Assume that the distance to Cygnus X3 was not well known at the time. The experimenters could estimate the γ factor (γ = 1/ 1 v 2 /c 2 ) of the cosmic rays. They found that γ 10 10. Approximately how far away could Cygnus X3 be if neutrons are the source of the puzzling cosmic rays? 9. Cosmic something else? This problem refers to the same phenomenon as the previous problem... Physicists quickly abandoned the idea that neutrons could be the source. They started hypothesizing new, hitherto unknown particles that could be the source of the puzzling events. (a) Taking the distance to Cygnus X3 to be 10,000 lyr, what would be a reasonable estimate of the proper lifetime of a hypothetical new particle (call it an H, for hypothetical) that would give rise to cosmic ray events with γ 10 10? (b) Use Lorentz contraction to describe the journey from the point of view of the H. In particular, how, in its own rest frame, can it cover the distance to Earth in its (short) lifetime? Epilogue: Follow up experiments were unable to reproduce the original phenomenon, ie. the events went away! 10. String of lights across the desert I A series of lights is arrayed in a straight line across the desert. Neighboring lights are separated by a distance d. They are set up to flash in sequence with an interval τ between neighboring lights (as measured in the rest frame of the lights). An observer,

3 O, travels along the same line at a uniform speed v in the same direction of the wave of flashes. (a) At what interval do the flashes occur in the rest frame of O? (b) Suppose O travels in the direction opposite the wave. What is the interval in this case? (c) For what choices of d, τ, and v do all flashes occur simultaneously in the rest frame of O? 11. String of lights across the desert II In the previous problem you were asked for the times at which the flashed occured in the rest frame of O. Now consider what would be seen by the observer O: Again let the straight line of lights be separated by d and flash in sequence with interval τ. Now compute the interval between the sequential flashes as seen by an observer travelling with uniform speed v along the direction of the flashes. [Hint: in this case you must consider not only the Lorentz transform of each flash event, but you must also consider how long it takes a flash to propagate to the observer O.] For what values of d, τ, and v will the flashes appear to be simulataneous to O? 12. Events in two different frames I Two events, A and B, are observed in two different inertial frames, Σ, and Σ. Frame Σ moves along the x axis in Σ. Event A occurs at the spacetime origin in both frames, x A = y A = z A = ct A = 0 x = y = z = ct = 0 A A A A Event B occurs at x B = 10, y B = z B = 0, ct B = 6 (all distances are in meters). The two events occur simultaneously in frame Σ. (a) Find the velocity of Σ with respect to Σ. (b) What is the space separation of the two events in the frame Σ? (c) What is the smallest spatial separation between the two events in any inertial frame? 13. Events in two different frames II Two events, A and B, are observed in two different inertial frame, Σ, and Σ. Event A occurs at the spacetime origin in both frames, x A = y A = z A = ct A = 0 x = y = z = ct = 0 A A A A

4 Event B occurs at x B = 2, y B = z B = 0, ct B = 10 (all distances are in meters) as observed in Σ. The two events occur at the same point in frame Σ. (a) Find the velocity of Σ with respect to Σ. (b) What is the time separation of the two events in the frame Σ? (c) What is the shortest time separation between the two events in any inertial frame? 14. Events in two different frames III Two events, A and B, are observed in two different inertial frame, Σ, and Σ. Event A occurs at the spacetime origin in both frames, x A = y A = z A = ct A = 0 x = y = z = ct = 0 A A A A Event B occurs at x B = 2, y B = z B = 0, ct B = 3 in Σ, and at (all distances are in meters) in Σ. x = 3, y = z = 0 B B B (a) What time does event B occur in Σ? (b) What is the relative velocity of Σ relative to Σ? 15. The travels of elementary particles reconsidered Return to Problem 2 on Problem Set 1 and recalculate the speed of the particles given their lifetimes and pathlengths. The problem is reproduced below for your convenience: Elementary particles have very short average lifetimes (at least measured on our perceptual scale). In experiments at accelerators the particles are produced and then detected at points away from the point of production. If the rules of Newtonian physics were correct for particles travelling at great speeds, the particles would have to travel much faster than the speed of light in order to go so far before they decay. Assuming that the particle in question lives for the average lifetime of that species, compute its average speed using Newtonian mechanics: (a) A π meson has a lifetime of 2.6 10 8 sec. It is observed 1 kilometers away from its point of production. (b) A Lambda hyperon has a lifetime of 2.6 10 10 sec. It is observed 30 meters away from its point of production. (c) A Λ B baryon has lifetime 1.23 10 12 sec. It is observed 3 millimeters away from its point of production.

5 16. Invariance of the interval (a) Show that the square of the spacetime interval (Δs 2 ) associated with two events (assumed to occur in the x x axis) is invariant under a Lorentz transformation. That is, show that (cδt) 2 (Δx) 2 = (cδt ) 2 (Δx ) 2 (b) For each of the following pairs of events, say whether i. there is a frame where they are simultaneous, or ii. there is a frame where they occur at the same place, or iii. neither 17. The expanding universe I x A = 2, y A = 1, z A = 0, ct A = 2 x B = 1, y B = 2, z B = 0, ct B = 1 II x A = 6, y A = 7, z A = 2, ct A = 8 x B = 3, y B = 3, z B = 2, ct B = 3 III x A = 2, y A = 4, z A = 1, ct A = 2 x B = 3, y B = 3, z B = 2, ct B = 4 Adapted from Resnick and Halliday, Basic Concepts in Relativity (MacMillan, New York, 1992). (a) Galaxy A is reported to be receding from us with a speed of 0.4c. Galaxy B, located in precisely the opposite direction, is also found to be receding from us at this same speed. What recessional speed would an observer on Galaxy A find i) for our galaxy? ii) for Galaxy B? (b) It is concluded from measurements of the red shift of the emitted light that quasar Q 1 is moving away from us at a speed of 0.75c. Quasar Q 2, which lies in the same direction in space, but is closer to us, is moving away from us at speed 0.50c. What velocity for Q 2 would be measured by an observer on Q 1?

6 18. Perpendicular velocities Adapted from Resnick and Halliday, Basic Concepts in Relativity (MacMillan, New York, 1992). A and B are trains on perpendicular tracks (see the figure), shown radiating from stations S. Both trains travel at a speed v = 0.8c in the rest frame of the station. (a) Find V AB, the velocity of train B with respect to train A. (b) Find V BA, the velocity of train A with respect to train B. (c) Comment on the fact that these two relative velocities do not point in opposite directions. th 0.8 c A 19. Transforming angles I A particle moves with speed u in the x y plane, making an angle θ with respect to the x axis in frame Σ. The origin of Σ moves to the right (along the positive x axis) in the frame Σ with speed v. What speed u and angle θ will the particle appear to have to an observer in Σ? 20. Transforming angles II A right triangular plate is at rest in the frame Σ. Its legs are placed on the x and y axes and its hypotenuse makes an angle θ with respect to the x axis. The origin of Σ moves to the right (along the positive x axis) in the frame Σ with speed v. What are the angles of the triangle as measured in Σ? S B 0.8 c t