Kinetic Energy: K = (γ - 1)mc 2 Rest Energy (includes internal kinetic and potential energy): E R mc 2

Size: px
Start display at page:

Download "Kinetic Energy: K = (γ - 1)mc 2 Rest Energy (includes internal kinetic and potential energy): E R mc 2"

Transcription

1 Kinetic Energy: K = (γ - 1)mc 2 Rest Energy (includes internal kinetic and potential energy): E R mc 2 For an object moving in an inertial frame), Total energy : E = K + E R = γmc 2 Problem 1: A mosquito has a mass of 2.5 mg. a) What is its rest energy? b) By what fraction does it change its energy if it is flying at 20 m/s ( 40 miles/hour) a) m = 2.5 x 10-6 kg E R = (2.5 x 10-6 kg) (3 x 10 8 m/s) 2 = 2.25 x J [This is the energy output of Big Sandy power plant in 3.5 minutes days. Therefore, if you could completely convert the mass of 400 mosquitoes/day to energy (we can t!!), you could match the energy output of Big Sandy!] b) Since v <<c, so can use K ½ mv 2 = 0.5 (2.5 x 10-6 kg) (20 m/s) 2 = 5 x 10-4 J So K/E R = 5 x 10-4 / 2.25 x = 2.2 x For everyday objects at ordinary speeds, relativistic corrections to energy are negligible classical mechanics works fine.

2 Kinetic Energy: K = (γ - 1)mc 2 Rest Energy (includes internal kinetic and potential energy): E R mc 2 For an object moving in an inertial frame, Total energy : E = K + E R E = γmc 2 In any process, the total energy is conserved! And: if no external forces, momentum is also conserved!

3 Consider a general reaction in which some species (A j ) react to form new species (B j ): A 1 + A 2 + A 3 +. B 1 + B 2 + B 3 + Conservation of Energy: c 2 A s (γm) = c 2 B s (γm) Conservation of Momentum: A s (γmv) = B s (γmv) [Today: Because masses will be given in atomic mass units (u), we ll use v s, not u s, for particle velocities.] (1u) c 2 = 931 MeV

4 Consider the fusion reaction: 2 D T 1 4 He 2 + n, where 2 D 1 is a deuterium atom, with m(d) = u, 3 T 1 is a tritium atom, with m(t) = u, 4 He 2 is a helium atom, with m(he) = u and n is a neutron, with m(n) = u. The incoming mass = m(d) + m(t) = u. The outgoing mass = m(he) + m(n) = u. Therefore, exothermic with m c 2 = ( u) c 2 Use (1 u)c 2 = 931 MeV m c 2 = 17.6 MeV Problem 2: Of this energy, K(He) = 3.5 MeV and K(n) = 14.1 MeV. Show that these values are consistent with conservation of momentum when the incoming deuterium and tritium have v << c (i.e. p(d) p(t) 0).

5 m(he) = u = 3726 MeV/c 2, m(n) = u = 939 MeV/c 2, m c 2 = 17.6 MeV Of this energy, K(He) = 3.5 MeV and K(n) = 14.1 MeV Show that these values are consistent with conservation of momentum: Because the incoming particles are at rest, the total momentum 0, so the neutron and helium atom should have equal and opposite momenta. K(n) = 14.1 MeV (γ(n) 1) m(n)c 2 = 14.1 MeV γ(n) -1 = 14.1 MeV / 939 MeV = γ= [1-(v/c) γ(n) = ] -1/2 v(n) = 0.17c p(n) = γ m v = (1.015) (939 MeV/c 2 ) (0.017c) =162 MeV/c K(He) = 3.5 MeV (γ(he) -1) m He c 2 = 3.5 MeV γ(he) -1 = 3.5 MeV / 3726 MeV = 9.4 x 10-4 γ(he) = v(he) = 0.043c p(he) = γmv = ( ) (3726 MeV/c 2 ) (.043c) = 162 MeV/c

6 Problem 3: A particle of mass M 0 at rest divides into two particles, with masses m 1 = 1u and m 2 = 4u. The 1u particle has speed v 1 = 0.8c. a) What is the speed of the 4u particle? b) What is the value of M 0? c) What is the total kinetic energy of the outgoing particles? a) p initial = 0 so p 2 = -p 1 γ 2 m 2 v 2 = γ 1 m 1 v 1 4v 2 /[1-(v 2 /c) 2 ] 1/2 = v 1 /[1-(v 1 /c) 2 ] 1/2 = 0.8c / [1-0.64] 1/2 = 0.8c/0.6 v 2 /[1-(v 2 /c) 2 ] 1/2 = c/3 (3v 2 /c) 2 = 1-(v 2 /c) 2 (v 2 /c) 2 = 1/10 v 2 = c

7 Problem 3: A particle of mass M 0 at rest divides into two particles, with masses m 1 = 1u and m 2 = 4u. The 1u particle has speed v 1 = 0.8c. a) What is the speed of the 4u particle? b) What is the value of M 0? c) What is the total kinetic energy of the outgoing particles? a) v 2 = c b) Since M 0 is at rest, its energy = M 0 c 2 M 0 c 2 = γ 1 m 1 c 2 + γ 2 m 2 c 2 M 0 = 1u [1/( ) 1/2 + 4/( ) 1/2 M 0 = 1u [1/0.36 1/2 + 4/0.9 1/2 ] = ( )u = 5.89 u c) Method 1: K total = K 1 + K 2 = (γ 1-1) m 1 c 2 + (γ 2-1)m 2 c 2 = ( (1-1/0.9 1/2 ) uc 2 = ( ) x 931 MeV = 829 MeV Method 2: Since M 0 is at rest, K total = (M 0 -m 1 -m 2 ) c 2 = ( )uc 2 = 0.89 x 931 MeV = 829 MeV

8 Problem 4: A particle of mass M 0 = 15 u at rest decays into three particles. The first particle has mass m 1 = 1 u and velocity v 1 = 0.8 c i. The second particle has mass m 2 = 3 u and velocity v 2 = - v 1. What are the mass and velocity of the third particle? γ 1 = γ 2 = 1/[1 v 12 /c 2 ] 1/2 = 1/[ ] 1/2 = 1/ [1 0.64] 1/2 = 1/0.36 1/2 = 1/0.6 = 5/3 Consvtn. of Energy: M 0 c 2 = γ 1 m 1 c 2 + γ 2 m 2 c 2 + γ 3 m 3 c 2 γ 3 m 3 = [15 u 5/3 (1 u + 3 u] = (25/3) u Consvtn. of momentum: initial momentum = final momentum 0 = γ 1 m 1 v 1 + γ 2 m 2 v 2 + γ 3 m 3 v 3 0 = 5/3 (1 u) (0.8 c)i 5/3 (3 u) (0.8c) i + (25/3 u) v 3 v 3 = (3/25) (5/3) (1-3) (0.8) i = c i (= 9.6 x 10 7 m/s in +x direction) Therefore γ 3 = 1/[1-(v 3 /c) 2 ] 1/2 = 1/[ ] 1/2 = Therefore m 3 = 25/3 u / = 7.90 u (This doesn t correspond to a real particle.)

9 Problem 5: An object with mass m 1 = 900 kg and traveling at speed v 1 = 0.85c collides with a stationary object with mass m 2 = 1400 kg and the two objects stick together. What are the speed and mass of the composite object (#3)? Energy conservation: γ 1 m 1 c 2 + m 2 c 2 = γ 3 m 3 c 2 Momentum conservation: γ 1 m 1 v 1 = γ 3 m 3 v 3 Energy: γ 1 = 1/( ) 1/2 = 1.90 γ 3 m 3 = (1.90 x ) kg = 3110 kg Momentum: γ 3 m 3 v 3 = 1.90 x 900 kg * 0.85c = 1454 kg c v 3 = (1454/3110) c = c γ 3 = 1/( ) 1/2 = 1.13 m 3 = 3110 kg/1.13 = 2750 kg

10 Problem 6: A 6.6 GeV (= 6600 MeV) proton (M P = u) collides with a proton at rest to create a new particle, X. What are the mass and energy of the new particle? stationary proton moving proton Conservation of Energy: (1 + γ P )M P c 2 = γ X M X c 2 Conservation of Momentum: γ P M P v P = γ X M X v X The rest energy of the proton E RP = x 931 MeV = 938 MeV. Therefore the moving proton has γ P = 6600/938 = Since 7.04 = γ P = 1/(1-v P2 /c 2 ) 1/2, the moving proton has speed v P /c = Conservation of Energy: γ X M X = 8.04M P = 8.10 u E X = 8.10 x 931 MeV = 7540 MeV = 7.54 GeV Conservation of Momentum: v X = 7.04 M P (0.990 c) / 8.04 M P = c Then γ X = 1/( ) 1/2 = 2.01 M X = 8.10 u / 2.01 = 4.0 u

11 For a particle with velocity v, p = γmv and E = γmc 2 E 2 p 2 c 2 = (mc) 2 (c 2 -v 2 )/ [1 v 2 /c 2 ] = (mc 2 ) 2 E 2 = p 2 c 2 + (mc 2 ) 2 This equation is true for all particles, even those with mass = 0 (e.g. photons, gravitons, gluons). For a particle with m=0: E R = mc 2 = 0, so all the energy is kinetic. K = γmc 2 0 γ = v = c (Massless particles must travel at speed c.) Then p = (γmv) = E/c. For example, a photon of frequency f and wavelength λ = c/f has energy E = hf. Therefore it has momentum p = hf/c = h/λ.

12 Problem 7: A pion (m π c 2 = 140 MeV) at rest decays to a muon (m µ c 2 = 106 MeV) and antineutrino (m ν 0). Find the energy of the antinuetrino. Since the antineutrino s mass 0, essentially all of its energy is kinetic: E ν = p ν c. Conservation of energy: Conservation of momentum: m π c 2 = γ µ m µ c 2 + p ν c γ µ m µ v µ = p ν m π c 2 = γ µ m µ c 2 (1 + v µ /c) m π / m µ = (1 + v µ /c)/ [1 (v µ /c) 2 ] 1/2 But [1 (v µ /c) 2 ] = (1 v u /c) (1 + v u /c) m π / m µ = [(1 + v µ /c)/ (1 v µ /c)] 1/2 140/106 = 1.32 = [(1+v u /c)/ (1 v u /c) ] 1/ = [(1+v u /c)/ (1 v u /c) ] v u /c = 1 + v u /c 2.74 v u /c = 0.74 v u /c = 0.27 γ µ = E ν = p ν c = m π c 2 - γ µ m µ c 2 = [140 (1.039)106] MeV E ν = 29.9 MeV

13 Recommended reading: Feynman s Lectures on Physics, Volume I, Chapters Available (for free!) online at (or hardcopy for ~ $40). Caution: Many older texts (e.g. Feynman) use different names and notation: What we call mass, m, is often called the rest mass and denoted m 0. What we denote as γm 0 is often called the relativistic mass, m. Quantity Us (Serway/Jewett) Feynman m = mass m 0 = rest mass γm m = (relativistic) mass Momentum (p) γmu γm 0 u = mu kinetic energy (K) (γ-1) mc 2 (γ-1) m 0 c 2 = (m-m 0 )c 2 rest energy (E R ) mc 2 m 0 c 2 total energy (E) γmc 2 γm 0 c 2 = mc 2

Physics 202. Professor P. Q. Hung. 311B, Physics Building. Physics 202 p. 1/2

Physics 202. Professor P. Q. Hung. 311B, Physics Building. Physics 202 p. 1/2 Physics 202 p. 1/2 Physics 202 Professor P. Q. Hung 311B, Physics Building Physics 202 p. 2/2 Momentum in Special Classically, the momentum is defined as p = m v = m r t. We also learned that momentum

More information

Part A-type questions

Part A-type questions PHYS306: lecture 8 th February 008 Part A-type questions. You toss an apple horizontally at 8.7 m/s from a height of.6 m. Simultaneously, you drop a peach from the same height. How long does each take

More information

PHYS1015 MOTION AND RELATIVITY JAN 2015 EXAM ANSWERS

PHYS1015 MOTION AND RELATIVITY JAN 2015 EXAM ANSWERS PHYS1015 MOTION AND RELATIVITY JAN 2015 EXAM ANSWERS Section A A1. (Based on previously seen problem) Displacement as function of time: x(t) = A sin ωt Frequency f = ω/2π. Velocity of mass is v(t) = dx

More information

Welcome back to PHY 3305

Welcome back to PHY 3305 Welcome back to PHY 3305 Today s Lecture: Momentum and Energy Conservation Albert Einstein 879-955 Review: Transforming Velocity Remember: u = dx dt x = γ ν (x + vt ) t = γ ν ( v c 2 x + t ) From this

More information

Problem Set # 2 SOLUTIONS

Problem Set # 2 SOLUTIONS Wissink P640 Subatomic Physics I Fall 007 Problem Set # SOLUTIONS 1. Easy as π! (a) Consider the decay of a charged pion, the π +, that is at rest in the laboratory frame. Most charged pions decay according

More information

Relativity II. Home Work Solutions

Relativity II. Home Work Solutions Chapter 2 Relativity II. Home Work Solutions 2.1 Problem 2.4 (In the text book) A charged particle moves along a straight line in a uniform electric field E with a speed v. If the motion and the electric

More information

Physics 280 Lecture 2

Physics 280 Lecture 2 Physics 280 Lecture 2 Summer 2016 Dr. Jones 1 1 Department of Physics Drexel University June 29, 2016 Objectives Review Lorentz Coordinate Transforms and principles of relativity Objectives Review Lorentz

More information

Slide 1 / 57. Nuclear Physics & Nuclear Reactions Practice Problems

Slide 1 / 57. Nuclear Physics & Nuclear Reactions Practice Problems Slide 1 / 57 Nuclear Physics & Nuclear Reactions Practice Problems Slide 2 / 57 Multiple Choice Slide 3 / 57 1 The atomic nucleus consists of: A B C D E Electrons Protons Protons and electrons Protons

More information

Fundamental Interactions (Forces) of Nature

Fundamental Interactions (Forces) of Nature Chapter 14 Fundamental Interactions (Forces) of Nature Interaction Gauge Boson Gauge Boson Mass Interaction Range (Force carrier) Strong Gluon 0 short-range (a few fm) Weak W ±, Z M W = 80.4 GeV/c 2 short-range

More information

Lecture 5 - Ultra high energy cosmic rays and the GZK cutoff

Lecture 5 - Ultra high energy cosmic rays and the GZK cutoff Lecture 5 - Ultra high energy cosmic rays and the GZK cutoff E. Daw April 4, 2012 1 Review of Lecture 4 Last time we studied use of 4 vectors, particularly the 4 momentum, in relativity calculations. We

More information

A

A 1 (a) They are not fundamental particles because they consist Not: They can be sub-divided of quarks (b) Any two from: electron / positron / neutrino / antineutrino Allow: muon / tau (c) (i) 4 Ca 1 e +

More information

Chapter 26. Relativity

Chapter 26. Relativity Chapter 26 Relativity Time Dilation The vehicle is moving to the right with speed v A mirror is fixed to the ceiling of the vehicle An observer, O, at rest in this system holds a laser a distance d below

More information

PH 253 Exam I Solutions

PH 253 Exam I Solutions PH 253 Exam I Solutions. An electron and a proton are each accelerated starting from rest through a potential difference of 0.0 million volts (0 7 V). Find the momentum (in MeV/c) and kinetic energy (in

More information

Assignment 5. Ian Rittersdorf Nuclear Engineering & Radiological Sciences

Assignment 5. Ian Rittersdorf Nuclear Engineering & Radiological Sciences Assignment 5 Ian Rittersdorf Nuclear Engineering & Radiological Sciences ianrit@umich.edu March 19, 2007 1 All mass values taken from Krane unless otherwise noted. P5.1, 20% Krane, Problem 9.3, p. 332.

More information

Multiple Choice Questions

Multiple Choice Questions Nuclear Physics & Nuclear Reactions Practice Problems PSI AP Physics B 1. The atomic nucleus consists of: (A) Electrons (B) Protons (C)Protons and electrons (D) Protons and neutrons (E) Neutrons and electrons

More information

Chapter 46 Solutions

Chapter 46 Solutions Chapter 46 Solutions 46.1 Assuming that the proton and antiproton are left nearly at rest after they are produced, the energy of the photon E, must be E = E 0 = (938.3 MeV) = 1876.6 MeV = 3.00 10 10 J

More information

Physics 111 Homework Solutions Week #9 - Thursday

Physics 111 Homework Solutions Week #9 - Thursday Physics 111 Homework Solutions Week #9 - Thursday Monday, March 1, 2010 Chapter 24 241 Based on special relativity we know that as a particle with mass travels near the speed of light its mass increases

More information

Physics H7C Midterm 2 Solutions

Physics H7C Midterm 2 Solutions Physics H7C Midterm 2 Solutions Eric Dodds 21 November, 2013 1 Qualitative questions a) The angular resolution of a space based telescope is limited by the wave properties of light, that is, by diffraction.

More information

1st year Relativity - Notes on Lectures 6, 7 & 8

1st year Relativity - Notes on Lectures 6, 7 & 8 1st year Relativity - Notes on Lectures 6, 7 & 8 Lecture Six 1. Let us consider momentum Both Galilean and relativistic mechanics define momentum to be: p = mv and p i = P = a constant i i.e. Total momentum

More information

Relativistic Kinematics Cont d

Relativistic Kinematics Cont d Phy489 Lecture 5 Relativistic Kinematics Cont d Last time discussed: Different (inertial) reference frames, Lorentz transformations Four-vector notation for relativistic kinematics, invariants Collisions

More information

Thursday, April 23, 15. Nuclear Physics

Thursday, April 23, 15. Nuclear Physics Nuclear Physics Some Properties of Nuclei! All nuclei are composed of protons and neutrons! Exception is ordinary hydrogen with just a proton! The atomic number, Z, equals the number of protons in the

More information

Modern Physics Part 2: Special Relativity

Modern Physics Part 2: Special Relativity Modern Physics Part 2: Special Relativity Last modified: 23/08/2018 Links Relative Velocity Fluffy and the Tennis Ball Fluffy and the Car Headlights Special Relativity Relative Velocity Example 1 Example

More information

26.c4 What two speed measurements will to observers in relative motion always agree upon?

26.c4 What two speed measurements will to observers in relative motion always agree upon? Ch.26 Problems Name Note: γ=1/(1-(v/c) 2 ).5 26.c1 A spherical spacecraft with diameter D moves past an observer on Earth with a speed of.500c. What shape does the observer see? Describe the change mathematically.

More information

RELATIVISTIC ENERGY AND MOMENTUM

RELATIVISTIC ENERGY AND MOMENTUM RELATIVISTIC ENERGY AND MOMENTUM Non-relativistically, the momentum and the energy of a free particle are related to its velocity v as p = mv, E = const + 1 2 mv2, (1) where m is the particle s mass. In

More information

Welcome back to PHY 3305

Welcome back to PHY 3305 Welcome back to PHY 3305 Today s Lecture: Applications of Energy and Momentum Conservation; Albert Einstein 1879-1955 AnNouncements -Reading Assignment for Thursday, September 7th: chapter 2, section 2.8-2.9.

More information

The ATLAS Experiment and the CERN Large Hadron Collider

The ATLAS Experiment and the CERN Large Hadron Collider The ATLAS Experiment and the CERN Large Hadron Collider HEP101-4 February 20, 2012 Al Goshaw 1 HEP 101 Today Introduction to HEP units Particles created in high energy collisions What can be measured in

More information

Collisions. Conservation of Momentum Elastic and inelastic collisions. Serway For practice: Chapter 9, problems 10, 11, 23, 70, 75

Collisions. Conservation of Momentum Elastic and inelastic collisions. Serway For practice: Chapter 9, problems 10, 11, 23, 70, 75 Collisions Conservation of Momentum Elastic and inelastic collisions Serway 9.3-9.4 For practice: Chapter 9, problems 10, 11, 23, 70, 75 Momentum: p = mv Impulse (a vector) is defined as F t (for a constant

More information

Physics 121 Hour Exam #5 60 Minutes, Take Home, Closed Book

Physics 121 Hour Exam #5 60 Minutes, Take Home, Closed Book Physics 121 Hour Exam #5 60 Minutes, Take Home, Closed Book What s different about this exam? ˆ This is a 60-minute exam (like exams 1 through 3, but not like exam 4). The standard exam instructions: This

More information

PHYS120 Lecture 5 - Energy, momentum and mass 5-1

PHYS120 Lecture 5 - Energy, momentum and mass 5-1 PHYS120 Lecture 5 - Energy, momentum and mass 5-1 Demonstration: photoelectric effect Text: Mod. Phys. 3.A, 3.B, 3.C, 3.D Problems: 3, 4, 6, 17, 19 from Ch. 3 What s important: Einstein s energy equation

More information

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

Introduction. Classical vs Modern Physics. Classical Physics: High speeds Small (or very large) distances Introduction Classical vs Modern Physics High speeds Small (or very large) distances Classical Physics: Conservation laws: energy, momentum (linear & angular), charge Mechanics Newton s laws Electromagnetism

More information

MASSACHUSETTS INSTITUTE OF TECHNOLOGY Physics Department. Problem Set 5 Solutions

MASSACHUSETTS INSTITUTE OF TECHNOLOGY Physics Department. Problem Set 5 Solutions MASSACHUSETTS INSTITUTE OF TECHNOLOGY Physics Department Physics 8.033 October, 003 Problem Set 5 Solutions Problem A Flying Brick, Resnick & Halliday, #, page 7. (a) The length contraction factor along

More information

Lecture 9 - Applications of 4 vectors, and some examples

Lecture 9 - Applications of 4 vectors, and some examples Lecture 9 - Applications of 4 vectors, and some examples E. Daw April 4, 211 1 Review of invariants and 4 vectors Last time we learned the formulae for the total energy and the momentum of a particle in

More information

Visit for more fantastic resources. AQA. A Level. A Level Physics. Particles (Answers) Name: Total Marks: /30

Visit   for more fantastic resources. AQA. A Level. A Level Physics. Particles (Answers) Name: Total Marks: /30 Visit http://www.mathsmadeeasy.co.uk/ for more fantastic resources. AQA A Level A Level Physics Particles (Answers) Name: Total Marks: /30 Maths Made Easy Complete Tuition Ltd 2017 1. This question explores

More information

Relativistic Dynamics

Relativistic Dynamics Chapter 13 Relativistic Dynamics 13.1 Relativistic Action As stated in Section 4.4, all of dynamics is derived from the principle of least action. Thus it is our chore to find a suitable action to produce

More information

Class XII Chapter 13 - Nuclei Physics

Class XII Chapter 13 - Nuclei Physics Question 13.1: (a) Two stable isotopes of lithium and have respective abundances of 7.5% and 92.5%. These isotopes have masses 6.01512 u and 7.01600 u, respectively. Find the atomic mass of lithium. (b)

More information

Final Exam Sample Problems

Final Exam Sample Problems UNIVERSITY OF ALABAMA Department of Physics and Astronomy PH 253 / LeClair Spring 2010 Final Exam Sample Problems 1. The orbital speed of the Earth around the Sun is 30 km/s. In one year, how many seconds

More information

1. (a) An ion of plutonium Pu has an overall charge of C. (iii) electrons... (3) (2) (Total 5 marks)

1. (a) An ion of plutonium Pu has an overall charge of C. (iii) electrons... (3) (2) (Total 5 marks) AQA Questions from 2004 to 2006 Particle Physics 239 94 1. (a) An ion of plutonium Pu has an overall charge of +1.6 10 19 C. For this ion state the number of (i) protons... neutrons... (iii) electrons...

More information

Lecture 3 - Compton Scattering

Lecture 3 - Compton Scattering Lecture 3 - Compton Scattering E. Daw March 0, 01 1 Review of Lecture Last time we recalled that in special relativity, as in pre-relativistic dynamics, the total energy in an interaction or collision

More information

Mechanics and Special Relativity (MAPH10030) Assignment 4

Mechanics and Special Relativity (MAPH10030) Assignment 4 MAPH0030) Assignment 4 Issue Date: Tuesday 3 April 00 Due Date: Wednesday April 00 Collection Date: Friday 3 April 00 In these questions, you may use the following conversion factor relating the electron-volt

More information

Physics 2203, Fall 2012 Modern Physics

Physics 2203, Fall 2012 Modern Physics Physics 2203, Fall 2012 Modern Physics. Monday, Aug. 27 th, 2011: Start Ch. 2: Rela@vis@c Momentum, Energy, Conversion of mass and Energy. Do classical laws of momentum and energy conserva@on remain valid

More information

Physics 225 Relativity and Math Applications

Physics 225 Relativity and Math Applications Physics 225 Relativity and Math Applications Fall 2012 Unit 6 Conservation, Conversion, and Nuclear Power N.C.R. Makins University of Illinois at Urbana-Champaign 2010 Physics 225 6.2 6.2 Physics 225 6.3

More information

NJCTL.org 2015 AP Physics 2 Nuclear Physics

NJCTL.org 2015 AP Physics 2 Nuclear Physics AP Physics 2 Questions 1. What particles make up the nucleus? What is the general term for them? What are those particles composed of? 2. What is the definition of the atomic number? What is its symbol?

More information

FUSION NEUTRON DEUTERIUM HELIUM TRITIUM.

FUSION NEUTRON DEUTERIUM HELIUM TRITIUM. FUSION AND FISSION THE SUN Nuclear Fusion Nuclear fusion is the process by which multiple nuclei join together to form a heavier nucleus. It is accompanied by the release or absorption of energy depending

More information

Physics 30: Chapter 8 Exam Nuclear

Physics 30: Chapter 8 Exam Nuclear Physics 30: Chapter 8 Exam Nuclear Name: Date: Mark: /34 Numeric Response. Place your answers to the numeric response questions, with units, in the blanks at the side of the page. (1 mark each) 1. A 100

More information

1 Stellar Energy Generation Physics background

1 Stellar Energy Generation Physics background 1 Stellar Energy Generation Physics background 1.1 Relevant relativity synopsis We start with a review of some basic relations from special relativity. The mechanical energy E of a particle of rest mass

More information

PHY-105: Introduction to Particle and Nuclear Physics

PHY-105: Introduction to Particle and Nuclear Physics M. Kruse, Spring 2011, Phy-105 PHY-105: Introduction to Particle and Nuclear Physics Up to 1900 indivisable atoms Early 20th century electrons, protons, neutrons Around 1945, other particles discovered.

More information

General Physics (PHY 2140)

General Physics (PHY 2140) General Physics (PHY 2140) Lecture 20 Modern Physics Nuclear Energy and Elementary Particles Fission, Fusion and Reactors Elementary Particles Fundamental Forces Classification of Particles Conservation

More information

Physics 8.20 Special Relativity IAP 2008

Physics 8.20 Special Relativity IAP 2008 Physics 8.20 Special Relativity IAP 2008 Problem Set # 4 Solutions 1. Proper acceleration (4 points) Note: this problem and the next two ask you to work through the details of results derived in lecture.

More information

University of California, Berkeley Physics H7C Spring 2011 (Yury Kolomensky) THE FINAL EXAM Monday, May 9, 7 10pm. Maximum score: 200 points

University of California, Berkeley Physics H7C Spring 2011 (Yury Kolomensky) THE FINAL EXAM Monday, May 9, 7 10pm. Maximum score: 200 points 1 University of California, Berkeley Physics H7C Spring 2011 (Yury Kolomensky) THE FINAL EXAM Monday, May 9, 7 10pm Maximum score: 200 points NAME: SID #: You are given 180 minutes for this exam. You are

More information

Relativity Albert Einstein: Brownian motion. fi atoms. Photoelectric effect. fi Quantum Theory On the Electrodynamics of Moving Bodies

Relativity Albert Einstein: Brownian motion. fi atoms. Photoelectric effect. fi Quantum Theory On the Electrodynamics of Moving Bodies Relativity 1905 - Albert Einstein: Brownian motion fi atoms. Photoelectric effect. fi Quantum Theory On the Electrodynamics of Moving Bodies fi The Special Theory of Relativity The Luminiferous Ether Hypothesis:

More information

We start with a reminder of a few basic concepts in probability. Let x be a discrete random variable with some probability function p(x).

We start with a reminder of a few basic concepts in probability. Let x be a discrete random variable with some probability function p(x). 1 Probability We start with a reminder of a few basic concepts in probability. 1.1 discrete random variables Let x be a discrete random variable with some probability function p(x). 1. The Expectation

More information

[1] (c) Some fruits, such as bananas, are naturally radioactive because they contain the unstable isotope of potassium-40 ( K.

[1] (c) Some fruits, such as bananas, are naturally radioactive because they contain the unstable isotope of potassium-40 ( K. (a) State, with a reason, whether or not protons and neutrons are fundamental particles....... [] (b) State two fundamental particles that can be classified as leptons.... [] (c) Some fruits, such as bananas,

More information

Earlier in time, all the matter must have been squeezed more tightly together and a lot hotter AT R=0 have the Big Bang

Earlier in time, all the matter must have been squeezed more tightly together and a lot hotter AT R=0 have the Big Bang Re-cap from last lecture Discovery of the CMB- logic From Hubble s observations, we know the Universe is expanding This can be understood theoretically in terms of solutions of GR equations Earlier in

More information

Revision Guide for Chapter 17

Revision Guide for Chapter 17 Revision Guide for Chapter 17 Contents Revision Checklist Revision Notes Accelerators... 4 Alpha scattering... 7 Energy level... 7 Model of the atom... 8 Quark... 9 Pair production and annihilation...

More information

Baryons, mesons and leptons are affected by particle interactions. Write an account of these interactions. Your account should:

Baryons, mesons and leptons are affected by particle interactions. Write an account of these interactions. Your account should: Baryons, mesons and leptons are affected by particle interactions. Write an account of these interactions. Your account should: include the names of the interactions identify the groups of particles that

More information

Question 13.1: Two stable isotopes of lithium and have respective abundances of 7.5% and 92.5%. These isotopes have masses 6.01512 u and 7.01600 u, respectively. Find the atomic mass of lithium. Boron

More information

Chapter 26. Special Relativity

Chapter 26. Special Relativity Chapter 26 Special Relativity The Postulates of Special Relativity THE POSTULATES OF SPECIAL RELATIVITY 1. The Relativity Postulate. The laws of physics are the same in every inertial reference frame.

More information

CHAPTER 7 TEST REVIEW

CHAPTER 7 TEST REVIEW IB PHYSICS Name: Period: Date: # Marks: 94 Raw Score: IB Curve: DEVIL PHYSICS BADDEST CLASS ON CAMPUS CHAPTER 7 TEST REVIEW 1. An alpha particle is accelerated through a potential difference of 10 kv.

More information

Part II Particle and Nuclear Physics Examples Sheet 1

Part II Particle and Nuclear Physics Examples Sheet 1 T. Potter Lent/Easter Terms 2017 Part II Particle and Nuclear Physics Examples Sheet 1 Matter and Forces 1. (A) Explain the meaning of the terms quark, lepton, hadron, nucleus and boson as used in the

More information

General Physics (PHY 2140) Lecture 14

General Physics (PHY 2140) Lecture 14 General Physics (PHY 2140) Lecture 14 Modern Physics 1. Relativity Einstein s General Relativity 2. Quantum Physics Blackbody Radiation Photoelectric Effect X-Rays Diffraction by Crystals The Compton Effect

More information

BIG BANG SUMMARY NOTES

BIG BANG SUMMARY NOTES BIG BANG SUMMARY NOTES BIG BANG THEORY Studies of red-shifts of distant galaxies show that the universe is expanding. This and other observations has led to the Big Bang Theory The Big Bang Theory claims

More information

Name Solutions to Final Exam December 14, 2016

Name Solutions to Final Exam December 14, 2016 Name Solutions to Final Exam December 14, 016 This test consists of five parts. Please note that in parts II through V, you can skip one question of those offered. Part I: Multiple Choice (mixed new and

More information

Introduction to Modern Physics Problems from previous Exams 3

Introduction to Modern Physics Problems from previous Exams 3 Introduction to Modern Physics Problems from previous Exams 3 2007 An electron of mass 9 10 31 kg moves along the x axis at a velocity.9c. a. Calculate the rest energy of the electron. b. Calculate its

More information

PHY 142! Assignment 11! Summer 2018

PHY 142! Assignment 11! Summer 2018 Reading: Modern Physics 1, 2 Key concepts: Bohr model of hydrogen; photoelectric effect; debroglie wavelength; uncertainty principle; nuclear decays; nuclear binding energy. 1.! Comment on these early

More information

6 C, in units of y 1.

6 C, in units of y 1. PHYS 203 Homework #12 Solutions 1. (8 points) Carbon-14 has a half-life of 5715 y. It decays via β decay, emitting an electron. (A) Determine the rate constant λ of 14 6 C, in units of y 1. (B) Carbon-14

More information

Conversation with Tom Bailey about how a photon can have momentum even though it has zero mass 9 September 2012 at 17:57

Conversation with Tom Bailey about how a photon can have momentum even though it has zero mass 9 September 2012 at 17:57 Conversation with Tom Bailey about how a photon can have momentum even though it has zero mass 9 September 2012 at 17:57 Only me Tom Bailey Could Planck constant be seen as a minimum possible mass if E=MC2?

More information

Physics 228. Momentum and Force Kinetic Energy Relativistic Mass and Rest Mass Photoelectric Effect Energy and Momentum of Photons

Physics 228. Momentum and Force Kinetic Energy Relativistic Mass and Rest Mass Photoelectric Effect Energy and Momentum of Photons Physics 228 Momentum and Force Kinetic Energy Relativistic Mass and Rest Mass Photoelectric Effect Energy and Momentum of Photons Lorentz Transformations vs. Rotations The Lorentz transform is similar

More information

Midterm Solutions. 1 1 = 0.999c (0.2)

Midterm Solutions. 1 1 = 0.999c (0.2) Midterm Solutions 1. (0) The detected muon is seen km away from the beam dump. It carries a kinetic energy of 4 GeV. Here we neglect the energy loss and angular scattering of the muon for simplicity. a.

More information

Name Final Exam December 14, 2016

Name Final Exam December 14, 2016 Name Final Exam December 14, 016 This test consists of five parts. Please note that in parts II through V, you can skip one question of those offered. Part I: Multiple Choice (mixed new and review questions)

More information

Problems of Chapter 1: Introduction

Problems of Chapter 1: Introduction Chapter 1 Problems of Chapter 1: Introduction 1.1 Problem 1 1: Luminosity of Gaussian bunches a) If the bunches can be described by Gaussian ellipsoids with ( ( )) x 2 ρ exp 2σx 2 + y2 2σy 2 + z2 2σz 2,

More information

Phys 102 Lecture 27 The strong & weak nuclear forces

Phys 102 Lecture 27 The strong & weak nuclear forces Phys 102 Lecture 27 The strong & weak nuclear forces 1 4 Fundamental forces of Nature Today Gravitational force (solar system, galaxies) Electromagnetic force (atoms, molecules) Strong force (atomic nuclei)

More information

Massachusetts Institute of Technology

Massachusetts Institute of Technology Massachusetts Institute of Technology Physics Department Physics 8.0 IAP 005 Introduction to Special Relativity Problem Set 4 1. Non relativistic limit The correct relativistic formula for the energy of

More information

More Energetics of Alpha Decay The energy released in decay, Q, is determined by the difference in mass of the parent nucleus and the decay products, which include the daughter nucleus and the particle.

More information

Lecture 6-4 momentum transfer and the kinematics of two body scattering

Lecture 6-4 momentum transfer and the kinematics of two body scattering Lecture 6-4 momentum transfer and the kinematics of two body scattering E. Daw March 26, 2012 1 Review of Lecture 5 Last time we figured out the physical meaning of the square of the total 4 momentum in

More information

T7-1 [255 marks] The graph shows the relationship between binding energy per nucleon and nucleon number. In which region are nuclei most stable?

T7-1 [255 marks] The graph shows the relationship between binding energy per nucleon and nucleon number. In which region are nuclei most stable? T7-1 [255 marks] 1. In the Geiger Marsden experiment alpha particles were directed at a thin gold foil. Which of the following shows how the majority of the alpha particles behaved after reaching the foil?

More information

Lecture 2: Quantum Mechanics and Relativity

Lecture 2: Quantum Mechanics and Relativity Lecture 2: Quantum Mechanics and Relativity Atom Atomic number A Number of protons Z Number of neutrons A-Z Number of electrons Z Charge of electron = charge of proton ~1.6 10-19 C Size of the atom ~10-10

More information

Chapter 26 Special Theory of Relativity

Chapter 26 Special Theory of Relativity Chapter 26 Special Theory of Relativity Classical Physics: At the end of the 19 th century, classical physics was well established. It seems that the natural world was very well explained. Newtonian mechanics

More information

Ch., Problem 3 After acceleration through 0 MV both the electron and proton will each have a kinetic energy of 0 MeV. For the electron, E K + mc 0:5 M

Ch., Problem 3 After acceleration through 0 MV both the electron and proton will each have a kinetic energy of 0 MeV. For the electron, E K + mc 0:5 M Physics 3304 Assignment solutions Grading: The problems that will be graded in detail for this assignment are Ch., number 35 and Ch. 3, number 9 èeach worth 5 points totalè. You will receive point for

More information

32 IONIZING RADIATION, NUCLEAR ENERGY, AND ELEMENTARY PARTICLES

32 IONIZING RADIATION, NUCLEAR ENERGY, AND ELEMENTARY PARTICLES 32 IONIZING RADIATION, NUCLEAR ENERGY, AND ELEMENTARY PARTICLES 32.1 Biological Effects of Ionizing Radiation γ-rays (high-energy photons) can penetrate almost anything, but do comparatively little damage.

More information

General Physics (PHY 2140)

General Physics (PHY 2140) General Physics (PHY 2140) Lecture 37 Modern Physics Nuclear Physics Radioactivity Nuclear reactions http://www.physics.wayne.edu/~apetrov/phy2140/ Chapter 29 1 Lightning Review Last lecture: 1. Nuclear

More information

The slides with white background you need to know. The slides with blue background just have some cool information.

The slides with white background you need to know. The slides with blue background just have some cool information. The slides with white background you need to know. The slides with blue background just have some cool information. The Big Bang cosmology the study of the origin, properties, processes, and evolution

More information

= : K A

= : K A Atoms and Nuclei. State two limitations of JJ Thomson s model of atom. 2. Write the SI unit for activity of a radioactive substance. 3. What observations led JJ Thomson to conclusion that all atoms have

More information

Weak interactions. Chapter 7

Weak interactions. Chapter 7 Chapter 7 Weak interactions As already discussed, weak interactions are responsible for many processes which involve the transformation of particles from one type to another. Weak interactions cause nuclear

More information

TWO BASIC RESULTS. Time dilation t(v) = [1/(1 v 2 /c 2 ) 1/2 ] t(0) Length Contraction d(v) = (1 v 2 /c 2 ) 1/2 d(0)

TWO BASIC RESULTS. Time dilation t(v) = [1/(1 v 2 /c 2 ) 1/2 ] t(0) Length Contraction d(v) = (1 v 2 /c 2 ) 1/2 d(0) TWO BASIC RESULTS Time dilation t(v) = [1/(1 v 2 /c 2 ) 1/2 ] t(0) Length Contraction d(v) = (1 v 2 /c 2 ) 1/2 d(0) These two basic results are at the core of special relativity: Moving clocks run slow,

More information

The Exchange Model. Lecture 2. Quantum Particles Experimental Signatures The Exchange Model Feynman Diagrams. Eram Rizvi

The Exchange Model. Lecture 2. Quantum Particles Experimental Signatures The Exchange Model Feynman Diagrams. Eram Rizvi The Exchange Model Lecture 2 Quantum Particles Experimental Signatures The Exchange Model Feynman Diagrams Eram Rizvi Royal Institution - London 14 th February 2012 Outline A Century of Particle Scattering

More information

FLAP P9.2 Radioactive decay COPYRIGHT 1998 THE OPEN UNIVERSITY S570 V1.1

FLAP P9.2 Radioactive decay COPYRIGHT 1998 THE OPEN UNIVERSITY S570 V1.1 Atoms of a given substance with differing atomic masses are said to be isotopes of that substance. The various isotopes of an element all contain the same number of protons but different numbers of neutrons.

More information

Particle Physics Outline the concepts of particle production and annihilation and apply the conservation laws to these processes.

Particle Physics Outline the concepts of particle production and annihilation and apply the conservation laws to these processes. Particle Physics 12.3.1 Outline the concept of antiparticles and give examples 12.3.2 Outline the concepts of particle production and annihilation and apply the conservation laws to these processes. Every

More information

Chapter 2. Relativity 2

Chapter 2. Relativity 2 Chapter 2 Relativity 2 Acceleration transformation x = γ x vt t = γ t v x u x = u x v 1 vu x a x = u y = u y γ 1 vu x γ 3 a x 1 vu x 3 u z = u z γ 1 vu x F = m a?? Conservation of momentum p is conserved

More information

Theory English (Official)

Theory English (Official) Q3-1 Large Hadron Collider (10 points) Please read the general instructions in the separate envelope before you start this problem. In this task, the physics of the particle accelerator LHC (Large Hadron

More information

Physics 116. Nov 21, Session 31 De Broglie, duality, and uncertainty. R. J. Wilkes

Physics 116. Nov 21, Session 31 De Broglie, duality, and uncertainty. R. J. Wilkes Physics 116 Session 31 De Broglie, duality, and uncertainty Nov 21, 2011 R. J. Wilkes Email: ph116@u.washington.edu Announcements HW 6 due today Clicker scores have been updated on Webassign gradebook

More information

Activity 12: Energy from Nuclear Reactions

Activity 12: Energy from Nuclear Reactions Name Section Activity 12: Energy from Nuclear Reactions 12.1 A Model of the Composition of Nucleons 1) Formation of Nucleons Nucleons consist of quark trios. a) Place orange or green quarks into the metal

More information

Elementary particles and typical scales in high energy physics

Elementary particles and typical scales in high energy physics Elementary particles and typical scales in high energy physics George Jorjadze Free University of Tbilisi Zielona Gora - 23.01.2017 GJ Elementary particles and typical scales in HEP Lecture 1 1/18 Contents

More information

PHY313 - CEI544 The Mystery of Matter From Quarks to the Cosmos Fall 2005

PHY313 - CEI544 The Mystery of Matter From Quarks to the Cosmos Fall 2005 PHY313 - CEI544 The Mystery of Matter From Quarks to the Cosmos Fall 2005 Peter Paul Office Physics D-143 www.physics.sunysb.edu PHY313 Peter Paul 09/8/05 PHY313-CEI544 Fall-05 1 The Energy Scales of Matter

More information

Matter and Energy. Previous studies have taught us that matter and energy cannot be created nor destroyed We balance equations to obey this law.

Matter and Energy. Previous studies have taught us that matter and energy cannot be created nor destroyed We balance equations to obey this law. Fission & Fusion Matter and Energy Previous studies have taught us that matter and energy cannot be created nor destroyed We balance equations to obey this law. 2 H 2 O 2 H 2 + O 2 We now need to understand

More information

Lecture 31 Chapter 22, Sections 3-5 Nuclear Reactions. Nuclear Decay Kinetics Fission Reactions Fusion Reactions

Lecture 31 Chapter 22, Sections 3-5 Nuclear Reactions. Nuclear Decay Kinetics Fission Reactions Fusion Reactions Lecture Chapter, Sections -5 Nuclear Reactions Nuclear Decay Kinetics Fission Reactions Fusion Reactions Gamma Radiation Electromagnetic photons of very high energy Very penetrating can pass through the

More information

The Compton Effect and Photon Momentum

The Compton Effect and Photon Momentum Section 5: The Compton Effect and Photon Momentum In this lesson you will Describe the Compton Effect experiment carried out by A.H. Compton Define the term scattering Express an understanding of Compton's

More information

DEEP INELASTIC SCATTERING

DEEP INELASTIC SCATTERING DEEP INELASTIC SCATTERING Electron scattering off nucleons (Fig 7.1): 1) Elastic scattering: E = E (θ) 2) Inelastic scattering: No 1-to-1 relationship between E and θ Inelastic scattering: nucleon gets

More information

General Physics (PHY 2140)

General Physics (PHY 2140) General Physics (PHY 2140) Lecture 20 Modern Physics Nuclear Energy and Elementary Particles Fission, Fusion and Reactors Elementary Particles Fundamental Forces Classification of Particles Conservation

More information

2007 Section A of examination problems on Nuclei and Particles

2007 Section A of examination problems on Nuclei and Particles 2007 Section A of examination problems on Nuclei and Particles 1 Section A 2 PHYS3002W1 A1. A fossil containing 1 gramme of carbon has a radioactivity of 0.03 disintegrations per second. A living organism

More information

energy loss Ionization + excitation of atomic energy levels Mean energy loss rate de /dx proportional to (electric charge) 2 of incident particle

energy loss Ionization + excitation of atomic energy levels Mean energy loss rate de /dx proportional to (electric charge) 2 of incident particle Lecture 4 Particle physics processes - particles are small, light, energetic à processes described by quantum mechanics and relativity à processes are probabilistic, i.e., we cannot know the outcome of

More information