Special Theory of Relativity

Similar documents
Special Theory of Relativity

PHY2061 Enriched Physics 2 Lecture Notes Relativity 4. Relativity 4

x 1 ' = x 1 vt 1 x 1 ' = 4.0 m t 1 = 1.0 s x 2 vt 2 ' = 4.0 m t 2 ' = x 2 = 3.0 s x 1 = x 2 x 1 ' + vt 1 ' + vt 2 v (t 1 t 2 ) = x 2 ' x 1 ' = x 2

High Energy Physics. Lecture 4 More kinematics and a picture show of particle collisions

Solved Problems in Special Relativity

Advanced Topics in Physics: Special Relativity Course Syllabus

Solutions to Problems in Goldstein, Classical Mechanics, Second Edition. Chapter 7

Physics 111 Homework Solutions Week #9 - Tuesday

Relativistic kinematics basic energy, mass and momentum units, Lorents force, track bending, sagitta. First accelerator: cathode ray tube

Experiment 7 ~ Conservation of Linear Momentum

Deformation of the Bodies by the Result of Length Contraction: A new Approach to the Lorentz Contraction

Chapter 8 Conservation of Linear Momentum. Conservation of Linear Momentum

LAB 4: MOMENTUM AND COLLISIONS

Derivation of the relativistic momentum and relativistic equation of motion from Newton s second law and Minkowskian space-time geometry

Mechanics 1: Conservation of Energy and Momentum

Relativistic Dynamics

ACCELERATORS AND MEDICAL PHYSICS 2

Curriculum for Excellence. Higher Physics. Success Guide

Special Relativity. Photo by Philippe Halsman. Used with permission from Mrs. P. Halsman.

Chapter 15 Collision Theory

Problem Set V Solutions

0.33 d down c charm s strange t top b bottom 1 3

G U I D E T O A P P L I E D O R B I T A L M E C H A N I C S F O R K E R B A L S P A C E P R O G R A M

arxiv: v1 [physics.gen-ph] 17 Sep 2013

Welcome back to Physics 211. Physics 211 Spring 2014 Lecture ask a physicist

Cross section, Flux, Luminosity, Scattering Rates

UNIVERSITETET I OSLO

SOLUTIONS TO CONCEPTS CHAPTER 15

Special Theory of Relativity

Masses in Atomic Units

Kinetic Theory of Gases. Chapter 33. Kinetic Theory of Gases

Physics Notes Class 11 CHAPTER 6 WORK, ENERGY AND POWER

Q3.2.a The gravitational force exerted by a planet on one of its moons is 3e23 newtons when the moon is at a particular location.

Lab 8: Ballistic Pendulum

PHOTOELECTRIC EFFECT AND DUAL NATURE OF MATTER AND RADIATIONS

The accurate calibration of all detectors is crucial for the subsequent data

Pearson Physics Level 30 Unit VIII Atomic Physics: Chapter 17 Solutions

9. Momentum and Collisions in One Dimension*

CMS Tracking Performance Results from early LHC Running

Time And Space Deformations In Special Relativity And Measuring Units

Concepts in Theoretical Physics

Physics 125 Practice Exam #3 Chapters 6-7 Professor Siegel

Gravitational Potential Energy

GCE Physics A. Mark Scheme for June Unit G485: Fields, Particles and Frontiers of Physics. Advanced GCE. Oxford Cambridge and RSA Examinations

Chapter 22 The Hamiltonian and Lagrangian densities. from my book: Understanding Relativistic Quantum Field Theory. Hans de Vries

To define concepts such as distance, displacement, speed, velocity, and acceleration.

Vacuum Evaporation Recap

Chapters Magnetic Force. for a moving charge. F=BQvsinΘ. F=BIlsinΘ. for a current

SPATIAL COORDINATE SYSTEMS AND RELATIVISTIC TRANSFORMATION EQUATIONS

How To Teach Physics At The Lhc

8. Potential Energy and Conservation of Energy Potential Energy: When an object has potential to have work done on it, it is said to have potential

AP1 Oscillations. 1. Which of the following statements about a spring-block oscillator in simple harmonic motion about its equilibrium point is false?

Charged Particle in a Magnetic Field

Lecture PowerPoints. Chapter 7 Physics: Principles with Applications, 6 th edition Giancoli

Topic 3. Evidence for the Big Bang

Midterm Solutions. mvr = ω f (I wheel + I bullet ) = ω f 2 MR2 + mr 2 ) ω f = v R. 1 + M 2m

Displacement (x) Velocity (v) Acceleration (a) x = f(t) differentiate v = dx Acceleration Velocity (v) Displacement x

Newton s Laws of Motion

Notes on Elastic and Inelastic Collisions

1 Speed of light is the maximal possible speed

POSSIBL-E EXPERIMENTS ON THE 200-GeV ACCELERATOR. A. D. Krisch University of Michigan. R. Serber Columbia University.

Rotation: Moment of Inertia and Torque

Chapter 9. particle is increased.

Einstein s Theory of Special Relativity Made Relatively Simple!

Chapter NP-5. Nuclear Physics. Nuclear Reactions TABLE OF CONTENTS INTRODUCTION OBJECTIVES 1.0 NUCLEAR REACTIONS 2.0 NEUTRON INTERACTIONS

Chapter 7: Acceleration and Gravity

PX408: Relativistic Quantum Mechanics

Online Courses for High School Students

Kinetic Energy (A) stays the same stays the same (B) increases increases (C) stays the same increases (D) increases stays the same.

Monday 11 June 2012 Afternoon

Feynman diagrams. 1 Aim of the game 2

Journal of Theoretics Journal Home Page

1. Degenerate Pressure

Conservation of Momentum and Energy

Boardworks AS Physics

A Guide to Detectors Particle Physics Masterclass. M. van Dijk

Matter Waves. Home Work Solutions

Biasing. 7 th FLUKA Course NEA Paris, Sept.29-Oct.3, 2008

Orbital Mechanics. Angular Momentum

Center of Gravity. We touched on this briefly in chapter 7! x 2

Suggested solutions, FYS 500 Classical Mechanics and Field Theory 2014 fall

Experiment 2: Conservation of Momentum

Some Special Relativity Formulas

Lab #4 - Linear Impulse and Momentum

Measurement of Charge-to-Mass (e/m) Ratio for the Electron

Motion of a Leaky Tank Car

Physical Science Chapter 2. Forces

Lesson 33: Photoelectric Effect

Ground Rules. PC1221 Fundamentals of Physics I. Kinematics. Position. Lectures 3 and 4 Motion in One Dimension. Dr Tay Seng Chuan

Theoretical Particle Physics FYTN04: Oral Exam Questions, version ht15

Atomic and Nuclear Physics Laboratory (Physics 4780)

hij Teacher Resource Bank GCE Physics A Other Guidance: Particle Physics By J Breithaupt

Chemistry 1000 Lecture 2: Nuclear reactions and radiation. Marc R. Roussel

Exam 2 is at 7 pm tomorrow Conflict is at 5:15 pm in 151 Loomis

Torque Analyses of a Sliding Ladder

Phys222 Winter 2012 Quiz 4 Chapters Name

Energy Deposition in MICE Absorbers and Coils

( ) ( ) ( ) ( ) ( ) ( )

HEAT UNIT 1.1 KINETIC THEORY OF GASES Introduction Postulates of Kinetic Theory of Gases

Transcription:

Special Theory of Relativity Up to ~1895, used simple Galilean Transformations x = x - vt t = t But observed that the speed of light, c, is always measured to travel at the same speed even if seen from different, moving frames c = 3 x 10 8 m/s is finite and is the fastest speed at which information/energy/particles can travel Einstein postulated that the laws of physics are the same in all inertial frames. With c=constant he derived Lorentz Transformations light u sees v l =c moving frame also sees v l = c NOT v l = c-u P460 - Relativity 1

Derive Lorentz Transform Bounce light off a mirror. Observe in 2 frames: A velocity=0 with respect to light source A velocity = v observe speed of light = c in both frames c = distance/time = 2L / t A c 2 = 4(L 2 + (x /2) 2 ) / t 2 A Assume linear transform (guess) x = G(x + vt) let x = 0 t = G(t + Bx) so x =Gvt t =Gt some algebra (ct ) 2 = 4L 2 + (Gvt) 2 and L = ct /2 and t =Gt gives (Gt) 2 = t 2 (1 + (Gv/c) 2 ) or G 2 = 1/(1 - v 2 /c 2 ) A mirror L A x P460 - Relativity 2

Lorentz Transformations Define b = u/c and g = 1/sqrt(1 - b 2 ) x = g (x + ut) u = velocity of transform y = y between frames is in z = z x-direction. If do x x then t = g (t + bx/c) + -. Use common sense can differentiate these to get velocity transforms v x = (v x - u) / (1 -u v x / c 2 ) v y = v y / g / (1 - u v x / c 2 ) v z = v z / g / (1 - u v x / c 2 ) usually for v < 0.1c non-relativistic (non-newtonian) expressions are OK. Note that 3D space point is now 4D space-time point (x,y,z,t) P460 - Relativity 3

Time Dilation Saw that t = g t. The clock runs slower for an observer not in the rest frame muons in atmosphere. Lifetime = t =2.2 x 10-6 sec ct = 0.66 km decay path = bgtc b g average in lab lifetime decay path.1 1.005 2.2 ms 0.07 km.5 1.15 2.5 ms 0.4 km.9 2.29 5.0 ms 1.4 km.99 7.09 16 ms 4.6 km.999 22.4 49 ms 15 km P460 - Relativity 4

Time Dilation Short-lived particles like tau and B. Lifetime = 10-12 sec ct = 0.03 mm time dilation gives longer path lengths measure second vertex, determine proper time in rest frame If measure L=1.25 mm L and v =.995c t(proper)=l/vg =.4 ps Twin Paradox. If travel to distant planet at v~c then age less on spaceship then in lab frame P460 - Relativity 5

Adding velocities Rocket A has v = 0.8c with respect to DS9. Rocket B have u = 0.9c with respect to Rocket A. What is velocity of B with respect to DS9? DS9 A B V =(v-u)/(1-vu/c 2 ) v = (.9+.8)/(1+.9*.8)=.988c Notes: use common sense on +/- if v = c and u = c v = (c+c)/2= c P460 - Relativity 6

Adding velocities Rocket A has v = 0.826c with respect to DS9. Rocket B have u = 0.635c with respect to DS9. What is velocity of A as observed from B? DS9 A Think of O as DS9 and O as rocket B V =(v-u)/(1-vu/c B 2 ) v = (.826-.635)/(1-.826*.635)=.4c If did B from A get -.4c (.4+.635)/(1+.4*.635)=1.04/1.25 =.826 P460 - Relativity 7

Relativistic Kinematics E 2 = (pc) 2 + (mc 2 ) 2 E = total energy m= mass and p=momentum natural units E in ev, p in ev/c, m in ev/c 2 c = 1 effectively. E 2 =p 2 +m 2 kinetic energy K = T = E - m @ 1/2 mv 2 if v << c Can show: b = p/e and g = E/m p = bgm if m.ne.0 or p=e if m=0 (many massless particles, photon, gluon and (almost massless) neutrinos) relativistic mass m = gm 0 a BAD concept P460 - Relativity 8

Derive Kinematics de = -Fdx = -dp/dt*dx = -vdp = - vd(gmv) assume p=gmv (need relativistic for p) d(gmv) = mgdv + mvdg = mdvg 3 dv = de = v= final v = 0 mv g 3 dv mv(1 v 2 = gmc 2 - mc 2 / c 2 ) 3/ 2 =Total Energy - rest energy = Kinetic Energy dv P460 - Relativity 9

Lorentz Transformations P and E are components of a 4 vector and so transform by same Lorentz Transformation Define b = u/c and g = 1/sqrt(1 - b 2 ) px = g (px + ue) u = velocity of transform py = py between frames is in pz = pz x-direction. If do x x then E = g (E + bpx/c) + -. common sense Examples with particle with mass=m at rest transformed to moving with velocity v P460 - Relativity 10

What are the momentum, kinetic, and total energies of a proton with v=.86c? v =.86c g = 1/(1.86*.86) 0.5 = 1.96 E = g m = 1.96*938 MeV/c 2 = 1840 MeV T = E - mc 2 = 1840-938 = 900 MeV p = be = gbm =.86*1840 MeV = 1580 MeV/c or p = (E 2 - m 2 ) 0.5 Note units: MeV, MeV/c and MeV/c 2. Usually never have to use c = 300,000 km/s in calculation P460 - Relativity 11

Accelerate electron to 0.99c and then to 0.999c. How much energy is added at each step? v =.99c g = 7.1 v =.999c g = 22.4 E = g m = 7.1*0.511 MeV = 3.6 Mev = 22.4*0.511 MeV = 11.4 MeV step 1 adds 3.1 MeV and step 2 adds 7.8 MeV even though velocity change in step 2 is only 0.9% P460 - Relativity 12

Lorentz Transformations (px,py,px,e) are components of a 4-vector which has same Lorentz transformation px = g (px + ue/c 2 ) u = velocity of transform py = py between frames is in pz = pz x-direction. If do px px E = g (E + upx) + - Use common sense also let c = 1 Frame 1 Frame 2 (cm) Before and after scatter P460 - Relativity 13

center-of-momentum frame Sp = 0. Some quantities are invariant when going from one frame to another: py and pz are transverse momentum M total = Invariant mass of system derived from E(total) and P(total) as if just one particle How to get to C.M. system? Think as if 1 particle E(total) = E1 + E2 Px(total) = px1 + px2 (etc) M(total) 2 = E(total) 2 - P(total) 2 g(c.m.) = E(total)/M(total) and b(c.m.) = P(total)/E(total) 1 2 at rest p1 = p2 1 Lab 2 C.M. P460 - Relativity 14

Particle production convert kinetic energy into mass - new particles assume 2 particles 1 and 2 both mass = m Lab or fixed target E(total) = E1 + E2 = E1 + m2 P(total) = p1 M(total) 2 = E(total) 2 - P(total) 2 M(total) = (E1 2 +2E1*m + m*m - p1 2 ).5 M(total)= (2m*m + 2E1*m) 0.5 ~ (2E1*m) 0.5 CM: E1 = E2 E(total) = E1+E2 and P(total) = 0 M(total) = 2E1 1 2 at rest p1 = p 2 1 2 Lab CM P460 - Relativity 15

p + p p + p + p + pbar what is the minimum energy to make a protonantiproton pair? In all frames M(total) (invariant mass) at threshold is equal to 4*mp (think of cm frame, all at rest) Lab M(total) = (E1 2 +2E1*m + m*m - p1 2 ).5 M(total)= (2m*m + 2E1*m) 0.5 = 4m E1 = (16*mp*mp - 2mp*mp)/2mp = 7mp CM: M(total) = 2E1 = 4mp or E1 and E2 each =2mp at threshold all at rest in c.m. after reaction 1 2 at rest p1 = p 2 1 Lab 2 CM P460 - Relativity 16

Transform examples Trivial: at rest E = m p=0. boost velocity = v E = g(e + bp) = gm p = g(p + be) = gbm moving with velocity v = p/e and then boost velocity = u (letting c=1) E = g(e + pu) p = g(p + Eu) calculate v = p /E = (p +Eu)/(E+pu) = (p/e + u)/(1+up/e) = (v+u)/(1+vu) prove velocity addition formula P460 - Relativity 17

A p=1 GeV proton hits an electron at rest. What is the maximum pt and E of the electron after the reaction? Elastic collision. In cm frame, the energy and momentum before/after collision are the same. Direction changes. 90 deg = max pt 180 deg = max energy bcm = Ptot/Etot = Pp/(Ep + me) Pcm = gcmbcm*me (transform electron to cm) Ecme = gcm*me ( easy as at rest in lab) pt max = Pcm as elastic scatter same pt in lab Emax = gcm(ecm + bcmpcm) 180 deg scatter = gcm(gcm*me + gbb*me) = g*g*me(1 + b*b) P460 - Relativity 18

p=1 GeV proton (or electron) hits a stationary electron (or proton) mp =.94 GeV me =.5 MeV incoming target bcm gcm Ptmax Emax p e.7 1.5.4 MeV 1.7 MeV p p.4 1.2.4 GeV 1.4 GeV e p.5 1.2.5 GeV 1.7 GeV e e.9995 30 15 MeV 1 GeV Emax is maximum energy transferred to stationary particle. Ptmax is maximum momentum of (either) outgoing particle transverse to beam. Ptmax gives you the maximum scattering angle a proton can t transfer much energy to the electron as need to conserve E and P. An electron scattering off another electron can t have much Pt as need to conserve E and P. P460 - Relativity 19