General Physics I. Lecture 19: Relativistic Energy and Momentum. Prof. WAN, Xin ( 万歆 )

Size: px
Start display at page:

Download "General Physics I. Lecture 19: Relativistic Energy and Momentum. Prof. WAN, Xin ( 万歆 )"

Transcription

1 General Physics I Lecture 19: Relativistic Energy and Momentum Prof. WAN, Xin ( 万歆 ) xinwan@zju.edu.cn

2 Outline Minkowski diagram Relativistic velocity, momentum, and energy The mass-energy equivalence Nuclear energy

3 Lorentz Transformation The complete transformation 1) t = γ(t ' + x ' v /c 2 ) y y ' v 2) x = γ(x ' + vt ') 3) 4) y = y ' z = z ' z Frank x z ' Mary x ' Or, 1) 2) 3) 4) ct = γ[(ct ') + β x '] x = γ[β(ct ') + x '] y = y ' z = z ' β = v /c γ = = 1 1 v 2 /c β 2

4 Space-Time Squeezing in (ct ', x ') = (1,0) (ct, x) = (γ, γ β) (ct ', x ') = (0,1) (ct, x) = (γ β, γ) Unit lengths for the ct' and x' axes change to ( ct x ) = ( γ γ β γ β γ ) ( ct ' x ' ) = γ ( 1 β β 1 ) ( ct ' x ' ) γ 1 + β 2 x X x ' X Frank = 1 + β2 1 β 2 ct ct ' X x ' X Mary v ct '

5 Minkowski Diagram x x ' What does now mean? What does here mean? q ct ' Well, they depend on the choice of frame. q ct tan θ = β

6 Minkowski Diagram x x ' now What does now mean? What does here mean? here ct ' In the rest frame K, now means t = const, and here means x = const. ct

7 Minkowski Diagram x x ' now here What does now mean? What does here mean? ct ' ct In the moving frame K', now means t' = const, and here means x' = const.

8 Length Contraction, Again right end same time in K C B left end x O q A same time in K' x ' tan θ = β ct ' ct Suppose the length of the stick is 1 in the K' frame. This means the length of OA is OA = 1 + β2 1 β 2 The length measured by Frank in the K frame is the length of OB. OC = OAcos θ BC = AC tanθ AC = OAsinθ OB =?

9 Length Contraction, Again same time in K x same time in K' x ' Therefore, the length of the stick measured in the K frame is OB = OC BC right end C B q A ct ' = 1 β 2 which is the standard length contraction result. Note that you can figure out left end O tan θ = β ct cosθ = β 2

10 Length Contraction, Again same time in K x same time in K' x ' Suppose the length of the stick is 1 in the K frame, i.e. Therefore, OA = 1 right end left end A O q E tan θ = β ct ' ct OE = OA/cosθ = 1 + β 2 The length measured by Mary in the K' frame is in units of the x' axis, or OE 1 + β 2 / 1 β 2 = 1 β 2

11 Rotation in Space ( x y ) = ( cosθ sin θ sinθ cosθ ) ( x ' y ' ) y y ' x ' Show that if we define Frank x Rose tanh ϕ = β = v/c The Lorentz transformations in the matrix form become ( ct x ) = ( cosh ϕ sinh ϕ sinh ϕ cosh ϕ ) ( ct ' x ' )

12 Velocity Transformation The complete transformation 1) t ' = γ(t vx/c 2 ) y y ' v 2) x ' = γ(x vt) 3) 4) y ' = y z ' = z z Frank x z ' Mary x ' Therefore, Recognize the velocity addition rule?

13 Velocity Transformation The complete transformation 1) t ' = γ(t vx/c 2 ) y y ' v 2) x ' = γ(x vt) 3) 4) y ' = y z ' = z z Frank x z ' Mary x '

14 Linear Momentum Linear momentum p must be conserved in all collisions. v -v v p xi = 0 p xf = 0 -v v 2v 1 + v 2 /c 2 v p ' xi = 2mv 1 + v 2 /c 2 p ' xf = 2mv

15 Linear Momentum Linear momentum p must be conserved in all collisions. The relativistic value calculated for p must approach the classical value mu as u approaches zero. Please verify the momentum conservation in the previous example of collision. Newton's second law becomes

16 Relativistic Energy We generalize energy from the work-kinetic energy theorem. We assume that the particle is accelerated from rest to some final speed u.

17 Relativistic Total Energy Evaluating the integral We can define Rest energy E 0 = mc 2 Total energy E = γ mc 2

18 Relativistic Kinetic Energy We can define the relativistic kinetic energy K At low u/c,

19 A Comparison

20 Mass-Energy Equivalence A small mass corresponds to an enormous amount of energy. This is a concept fundamental to nuclear and elementary-particle physics. Together with m 2 c 2 = ( E/c) 2 p 2 another invariant

21 The Most Famous Equation The release of atomic energy has not created a new problem. Albert Einstein on Atomic War or Peace

22 Fission of Uranium How much energy is released by the fission of uranium-235 to form barium-142 and krypton-91? The particle masses are 235U ( u) 142Ba ( u) 91Kr ( u) 1n ( u) 1n U 142 Ba + 91 Kr n The discovery of nuclear fission by Otto Hahn and Fritz Strassmann opened up a new era in human history. It seems to me that what makes the science behind this discovery so remarkable is that it was achieved by purely chemical means. Lise Meitner

23 Fission of Uranium 1. Determine the change in mass for one U-235 atom: Δ m = u 2. This means that for each mole of U-235 atoms ( g), the corresponding energy by Einstein's equation is E = mc 2 = J = kwh (Note that 1 kwh» 0.5 RMB) The experimental apparatus with which Otto Hahn and Fritz Strassmann discovered nuclear fission in 1938.

24 Otto Hahn's Notebook

25 Chain Reaction Otto Hahn Farmhall n U 142 Ba + 91 Kr n...he had contemplated suicide, when he first recognized the possible military use of fission; now, with the blame of its realization drawn squarely upon his shoulders, suicide again seemed a way to escape his desolation... Never has social responsibility hit a scientist with such impact.

26 Fukushima Nuclear Disaster The plant comprised six separate boiling water reactors originally designed by General Electric and maintained by the Tokyo Electric Power Company. Units 2 through 6 were BWR-4, while Unit 1 was the slightly older BWR-3 design. The Fukushima Nuclear Accident Independent Investigation Commission found the nuclear disaster was "manmade" and that its direct causes were all foreseeable.

27 Light Water Reactors Two main varieties of light water reactors are: the pressurized water reactor (PWR) and the boiling water reactor (BWR). The main difference between a BWR and PWR is that in a BWR, the reactor core heats water, which turns to steam and then drives a steam turbine. In a PWR, the reactor core heats water, which does not boil. This hot water then exchanges heat with a lower pressure water system, which turns to steam and drives the turbine.

28 Pressurized Water Reactor 中国首台也是世界首台第三代先进压水堆 AP1000 型核电机组 浙江三门核电站 1 号机组, 计划于 2015 年年底并网发电

29 Fission Reactor Philippsburg Nuclear Power Plant, Germany

30 Heavy Water Reactor Qinshan Phase III Units 1 & 2, located in Zhejiang China ( N E): Two CANDU 6 reactors, designed by Atomic Energy of Canada Limited (AECL), owned and operated by the Third Qinshan Nuclear Power Company Limited.

31 Deuteron Binding Energy A deuteron, which is the nucleus of a deuterium atom, contains one proton and one neutron and has a mass of u. The mass of proton is u and the mass of neutron u. Note that 1 u = kg. This total deuteron mass is not equal to the sum of the masses of the proton and neutron. The mass difference is therefore u. The energy equivalence of the mass difference is called the binding energy of the nucleus

32 Fusion In the nuclear reaction called fusion, two atomic nuclei combine to form a single nucleus. The fusion reaction in which two deuterium nuclei fuse to form a helium nucleus is of major importance in the development of controlledfusion reactors. The decrease in mass that results from the creation of one helium nucleus from two deuterium nuclei is kg. Hence, the corresponding excess energy that results from one fusion reaction is J = 23.9 MeV. If 1 g of deuterium is converted to helium, the energy released is about J!

33 Sustainable Energy Technologies that promote sustainable energy include renewable energy sources, such as hydroelectricity, solar energy, wind energy, wave power, geothermal energy, bioenergy, tidal power and also technologies designed to improve energy efficiency.

General Physics I. Lecture 21: Relativistic Energy and Momentum. Prof. WAN, Xin ( 万歆 )

General Physics I. Lecture 21: Relativistic Energy and Momentum. Prof. WAN, Xin ( 万歆 ) General Physics I Lecture 21: Relativistic Energy and Momentum Prof. WAN, Xin ( 万歆 ) xinwan@zju.edu.cn http://zimp.zju.edu.cn/~xinwan/ Outline Relativistic velocity, momentum, and energy The mass-energy

More information

General Physics I. Lecture 20: Lorentz Transformation. Prof. WAN, Xin ( 万歆 )

General Physics I. Lecture 20: Lorentz Transformation. Prof. WAN, Xin ( 万歆 ) General Physics I Lecture 20: Lorentz Transformation Prof. WAN, Xin ( 万歆 ) xinwan@zju.edu.cn http://zimp.zju.edu.cn/~xinwan/ Outline Lorentz transformation The inariant interal Minkowski diagram; Geometrical

More information

Nuclear Fission. Conceptual Physics 11 th Edition. Nuclear Fission. Nuclear Fission. Nuclear Fission. This lecture will help you understand:

Nuclear Fission. Conceptual Physics 11 th Edition. Nuclear Fission. Nuclear Fission. Nuclear Fission. This lecture will help you understand: Conceptual Physics 11 th Edition A typical uranium fission reaction: Chapter 34: NUCLEAR FISSION AND FUSION Note the mass number as well as atomic numbers balance. This lecture will help you understand:

More information

turbine (a) (i) Which part of the power station provides thermal (heat) energy from a chain reaction?

turbine (a) (i) Which part of the power station provides thermal (heat) energy from a chain reaction? Nuclear fission and radiation 1 The diagram shows parts of a nuclear power station. control rods boiler steam generator electricity out turbine condenser nuclear reactor (a) (i) Which part of the power

More information

Chapter 10 Section 4 Notes

Chapter 10 Section 4 Notes Chapter 10 Section 4 Notes This painting of an alchemist s laboratory was made around 1570. For centuries, these early scientists, known as alchemists, tried to use chemical reactions to make gold. The

More information

Nuclear power plants can generate large amounts of electricity.

Nuclear power plants can generate large amounts of electricity. 7.3 Nuclear Reactions Nuclear fission and fusion are processes that involve extremely large amounts of energy. Fission = the splitting of nuclei Fusion = the joining of nuclei Nuclear power plants can

More information

Nuclear Energy Learning Outcomes

Nuclear Energy Learning Outcomes 1 Nuclear Energy Learning Outcomes Describe the principles underlying fission and fusion. Interpret nuclear reactions. Discuss nuclear weapons. Describe the structure and operation of a nuclear reactor.

More information

Nuclear Energy Learning Outcomes. Nuclear Fission. Chain Reaction

Nuclear Energy Learning Outcomes. Nuclear Fission. Chain Reaction by fastfission public domain by fastfission public domain 1 Nuclear Energy Learning Outcomes Describe the principles underlying fission and fusion. Interpret nuclear reactions. Discuss nuclear weapons.

More information

Nuclear 2. Fission and Fusion

Nuclear 2. Fission and Fusion Nuclear 2 Fission and Fusion History 1896: Becquerel discovers radioactivity 1898: Marie & Pierre Curie discover radium 1911: Rutherford discovers nucleus 1932: Chadwick discovers neutrons 1933: Hitler

More information

Preliminaries. Introduction to Nuclear Science. Simon Fraser University Spring NUCS 342 January 6, 2011

Preliminaries. Introduction to Nuclear Science. Simon Fraser University Spring NUCS 342 January 6, 2011 Preliminaries Introduction to Nuclear Science Simon Fraser University Spring 2011 NUCS 342 January 6, 2011 NUCS 342 (Lecture 0) January 6, 2011 1 / 21 Outline 1 Useful links NUCS 342 (Lecture 0) January

More information

Physics 30 Modern Physics Unit: Fission and Fusion

Physics 30 Modern Physics Unit: Fission and Fusion Physics 30 Modern Physics Unit: Fission and Fusion Nuclear Energy For years and years scientists struggled to describe where energy came from. They could see the uses of energy and the results of energy

More information

Introducing nuclear fission The Fizzics Organization

Introducing nuclear fission The Fizzics Organization Nuclear Fission is the splitting of the nucleus of an atom into two or more parts by hitting it with a small particle, almost always a neutron (a proton would be repelled from the positive nucleus and

More information

Term 3 Week 2 Nuclear Fusion & Nuclear Fission

Term 3 Week 2 Nuclear Fusion & Nuclear Fission Term 3 Week 2 Nuclear Fusion & Nuclear Fission Tuesday, November 04, 2014 Nuclear Fusion To understand nuclear fusion & fission Nuclear Fusion Why do stars shine? Stars release energy as a result of fusing

More information

Chapter 7.1. Q4 (a) In 1 s the energy is 500 MJ or (i) 5.0! 10 J, (ii) 5.0! 10 kw! hr " 140 kwh or (iii) MWh. (b) In one year the energy is

Chapter 7.1. Q4 (a) In 1 s the energy is 500 MJ or (i) 5.0! 10 J, (ii) 5.0! 10 kw! hr  140 kwh or (iii) MWh. (b) In one year the energy is Chapter 7.1 Q1 The thermal energy discarded must be returned to a reservoir that has a lower temperature from where the energy was extracted. In this case the temperatures are the same and so this will

More information

Physics 2D Lecture Slides Jan 21. Vivek Sharma UCSD Physics

Physics 2D Lecture Slides Jan 21. Vivek Sharma UCSD Physics Physics D Lecture Slides Jan 1 Vivek Sharma UCSD Physics Particle Accelerators as Testing ground for S. Relativity When Electron Goes Fast it Gets Fat E = γ mc v As 1, γ c Apparent Mass approaches Relativistic

More information

[2] State in what form the energy is released in such a reaction.... [1]

[2] State in what form the energy is released in such a reaction.... [1] (a) The following nuclear reaction occurs when a slow-moving neutron is absorbed by an isotope of uranium-35. 0n + 35 9 U 4 56 Ba + 9 36Kr + 3 0 n Explain how this reaction is able to produce energy....

More information

10.4 Fission and Fusion

10.4 Fission and Fusion This painting of an alchemist s laboratory was made around 1570. For centuries, these early scientists, known as alchemists, tried to use chemical reactions to make gold. The alchemists failed in their

More information

Atomic and Nuclear Physics. Topic 7.3 Nuclear Reactions

Atomic and Nuclear Physics. Topic 7.3 Nuclear Reactions Atomic and Nuclear Physics Topic 7.3 Nuclear Reactions Nuclear Reactions Rutherford conducted experiments bombarding nitrogen gas with alpha particles from bismuth-214. He discovered that fast-moving particles

More information

RADIOACTIVITY & HALF-LIFE Part 3

RADIOACTIVITY & HALF-LIFE Part 3 RADIOACTIVITY & HALF-LIFE Part 3 Half-Life Half-life: is the rate of decay for a radioactive isotope. is the time required for half of an original quantity of an element to decay. is constant and independent

More information

Nobel prizes in nuclear and reactor physics. Szabolcs Czifrus Institute of Nuclear Techniques BME

Nobel prizes in nuclear and reactor physics. Szabolcs Czifrus Institute of Nuclear Techniques BME Nobel prizes in nuclear and reactor physics Szabolcs Czifrus Institute of Nuclear Techniques BME Nuclear physics in everyday life Electricity: production in nuclear power plants Sterilization by the application

More information

The Physics of Nuclear Reactors. Heather King Physics 420

The Physics of Nuclear Reactors. Heather King Physics 420 The Physics of Nuclear Reactors Heather King Physics 420 Nuclear Reactions A nuclear reaction is a reaction that involves atomic nuclei, or nuclear particles (protons, neutrons), producing products different

More information

Lecture 5 Nuclear Reactions

Lecture 5 Nuclear Reactions Objectives In this lecture you will learn the following We shall understand the concept of kinetic energy from the perspective of particle physics. We shall conclude that for all practical purposes, mass

More information

Radioactivity. L 38 Modern Physics [4] Hazards of radiation. Nuclear Reactions and E = mc 2 Einstein: a little mass goes a long way

Radioactivity. L 38 Modern Physics [4] Hazards of radiation. Nuclear Reactions and E = mc 2 Einstein: a little mass goes a long way L 38 Modern Physics [4] Nuclear physics what s inside the nucleus and what holds it together what is radioactivity, halflife carbon dating Nuclear energy nuclear fission nuclear fusion nuclear reactors

More information

POGIL: Fission Fusion

POGIL: Fission Fusion Name: Date: Period: Chemistry POGIL: Fission Fusion Why? Up until the 9 s, the only nuclear reactions that had been observed involved nuclei either capturing or emitting small particles such as alpha and

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

Final Review Prof. WAN, Xin

Final Review Prof. WAN, Xin General Physics I Final Review Prof. WAN, Xin xinwan@zju.edu.cn http://zimp.zju.edu.cn/~xinwan/ About the Final Exam Total 6 questions. 40% mechanics, 30% wave and relativity, 30% thermal physics. Pick

More information

Nuclear Energy ECEG-4405

Nuclear Energy ECEG-4405 Nuclear Energy ECEG-4405 Today s Discussion Technical History and Developments Atom Nuclear Energy concepts and Terms Features Fission Critical Mass Uranium Fission Nuclear Fusion and Fission Fusion Fission

More information

Nuclear Fusion 1 of 24 Boardworks Ltd 2011

Nuclear Fusion 1 of 24 Boardworks Ltd 2011 Nuclear Fusion 1 of 24 Boardworks Ltd 2011 2 of 24 Boardworks Ltd 2011 How do we get energy from atoms? 3 of 24 Boardworks Ltd 2011 Energy is produced from atoms in power stations using the process of

More information

Section 2: Nuclear Fission and Fusion. Preview Key Ideas Bellringer Nuclear Forces Nuclear Fission Chain Reaction Nuclear Fusion

Section 2: Nuclear Fission and Fusion. Preview Key Ideas Bellringer Nuclear Forces Nuclear Fission Chain Reaction Nuclear Fusion : Nuclear Fission and Fusion Preview Key Ideas Bellringer Nuclear Forces Nuclear Fission Chain Reaction Nuclear Fusion Key Ideas What holds the nuclei of atoms together? What is released when the nucleus

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

PHY492: Nuclear & Particle Physics. Lecture 3 Homework 1 Nuclear Phenomenology

PHY492: Nuclear & Particle Physics. Lecture 3 Homework 1 Nuclear Phenomenology PHY49: Nuclear & Particle Physics Lecture 3 Homework 1 Nuclear Phenomenology Measuring cross sections in thin targets beam particles/s n beam m T = ρts mass of target n moles = m T A n nuclei = n moles

More information

Nuclear Physics 3 8 O+ B. always take place and the proton will be emitted with kinetic energy.

Nuclear Physics 3 8 O+ B. always take place and the proton will be emitted with kinetic energy. Name: Date: Nuclear Physics 3. A student suggests that the following transformation may take place. Measurement of rest masses shows that 7 7 N+ He 8 O+ total rest mass( N 7 + He ) < total rest mass( O

More information

Chapter 12: Nuclear Reaction

Chapter 12: Nuclear Reaction Chapter 12: Nuclear Reaction A nuclear reaction occurs when a nucleus is unstable or is being bombarded by a nuclear particle. The product of a nuclear reaction is a new nuclide with an emission of a nuclear

More information

Science 10: Radioactivity! Comparing Fission and Fusion Notes (Ch 11)

Science 10: Radioactivity! Comparing Fission and Fusion Notes (Ch 11) http://www.atomicarchive.com/movies/index.shtml Science 10: Radioactivity! Comparing Fission and Fusion Notes (Ch 11) Nuclear Reactions: an atom s nucleus changes by gaining or releasing particles or energy.

More information

General Physics I. Lecture 6: Conservation of Momentum. Prof. WAN, Xin 万歆.

General Physics I. Lecture 6: Conservation of Momentum. Prof. WAN, Xin 万歆. General Physics I Lecture 6: Conservation of Momentum Prof. WAN, Xin 万歆 xinwan@zju.edu.cn http://zimp.zju.edu.cn/~xinwan/ Outline Importance of conservation laws in physics Applications of the conservation

More information

L 36 Modern Physics :006 FINAL EXAM. Nuclear reactions: E = mc 2. Radioactivity. Hazards of radiation. Biological effects of nuclear radiation

L 36 Modern Physics :006 FINAL EXAM. Nuclear reactions: E = mc 2. Radioactivity. Hazards of radiation. Biological effects of nuclear radiation 9:006 FINAL EXAM The final exam is on Monday MAY 7:30 AM - 9:30 AM in W90 CB The FE is not cumulative, and will cover lectures 3 through 36. (50 questions) The last regular lecture (Lec. 36) will be given

More information

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

PHYS 280 Midterm α Fall You may answer the questions in the space provided here, or if you prefer, on your own notebook paper. PHYS 280 Midterm α Fall 2014 Name: You may answer the questions in the space provided here, or if you prefer, on your own notebook paper. Short answers 1. If you are measuring an astrophysical phenomenon,

More information

Science A 52 Lecture 22 May 1, 2006 Nuclear Power. What is it? What are its problems and prospects?

Science A 52 Lecture 22 May 1, 2006 Nuclear Power. What is it? What are its problems and prospects? Science A 52 Lecture 22 May 1, 2006 Nuclear Power What is it? What are its problems and prospects? Lecture 22, 1 Nuclear Fission On of the most interesting accounts a fission and the discovery of the release

More information

LIGHT and SPECIAL RELATIVITY RELATIVISTIC MASS, MOMENTUM and ENERGY

LIGHT and SPECIAL RELATIVITY RELATIVISTIC MASS, MOMENTUM and ENERGY VISUAL PHYSICS ONLINE MODULE 7 NATURE OF LIGHT LIGHT and SPECIAL RELATIVITY RELATIVISTIC MASS, MOMENTUM and ENERGY Einstein s 1 st postulate states that the laws of physics are the same for all observers

More information

Chemistry 500: Chemistry in Modern Living. Topic 5: The Fires of Nuclear Fission. Atomic Structure, Nuclear Fission and Fusion, and Nuclear.

Chemistry 500: Chemistry in Modern Living. Topic 5: The Fires of Nuclear Fission. Atomic Structure, Nuclear Fission and Fusion, and Nuclear. Chemistry 500: Chemistry in Modern Living 1 Topic 5: The Fires of Nuclear Fission Atomic Structure, Nuclear Fission and Fusion, and Nuclear Weapons Chemistry in Context, 2 nd Edition: Chapter 8, Pages

More information

Nuclear Reactions and E = mc 2. L 38 Modern Physics [4] Hazards of radiation. Radiation sickness. Biological effects of nuclear radiation

Nuclear Reactions and E = mc 2. L 38 Modern Physics [4] Hazards of radiation. Radiation sickness. Biological effects of nuclear radiation L 38 Modern Physics [4] Nuclear physics what s s inside the nucleus and what holds it together what is radioactivity, halflife carbon dating Nuclear energy nuclear fission nuclear fusion nuclear reactors

More information

Chemistry 132 NT. Nuclear Chemistry. Review. You can t escape death and taxes. But, at least, death doesn t get worse. Will Rogers

Chemistry 132 NT. Nuclear Chemistry. Review. You can t escape death and taxes. But, at least, death doesn t get worse. Will Rogers Chemistry 3 NT You can t escape death and taxes. But, at least, death doesn t get worse. Will Rogers Chem 3 NT Nuclear Chemistry Module 3 Energy and Nuclear Reactions The core of a nuclear reactor used

More information

L 36 Atomic and Nuclear Physics-4. Radioactivity. Nuclear reactions: E = mc 2. Hazards of radiation. Biological effects of nuclear radiation

L 36 Atomic and Nuclear Physics-4. Radioactivity. Nuclear reactions: E = mc 2. Hazards of radiation. Biological effects of nuclear radiation L 36 Atomic and Nuclear Physics- Nuclear physics what s inside the nucleus and what holds it together what is radioactivity, half-life carbon dating Nuclear energy nuclear fission nuclear fusion nuclear

More information

Nuclear Physics 2. D. atomic energy levels. (1) D. scattered back along the original direction. (1)

Nuclear Physics 2. D. atomic energy levels. (1) D. scattered back along the original direction. (1) Name: Date: Nuclear Physics 2. Which of the following gives the correct number of protons and number of neutrons in the nucleus of B? 5 Number of protons Number of neutrons A. 5 6 B. 5 C. 6 5 D. 5 2. The

More information

Lecture 14, 8/9/2017. Nuclear Reactions and the Transmutation of Elements Nuclear Fission; Nuclear Reactors Nuclear Fusion

Lecture 14, 8/9/2017. Nuclear Reactions and the Transmutation of Elements Nuclear Fission; Nuclear Reactors Nuclear Fusion Lecture 14, 8/9/2017 Nuclear Reactions and the Transmutation of Elements Nuclear Fission; Nuclear Reactors Nuclear Fusion Nuclear Reactions and the Transmutation of Elements A nuclear reaction takes place

More information

Unpressurized steam reactor. Controlled Fission Reactors. The Moderator. Global energy production 2000

Unpressurized steam reactor. Controlled Fission Reactors. The Moderator. Global energy production 2000 From last time Fission of heavy elements produces energy Only works with 235 U, 239 Pu Fission initiated by neutron absorption. Fission products are two lighter nuclei, plus individual neutrons. These

More information

Nuclear Chemistry. The Nucleus. Isotopes. Slide 1 / 43. Slide 2 / 43. Slide 3 / 43

Nuclear Chemistry. The Nucleus. Isotopes. Slide 1 / 43. Slide 2 / 43. Slide 3 / 43 Slide 1 / 43 Nuclear Chemistry The Nucleus Slide 2 / 43 Remember that the nucleus is comprised of the two nucleons, protons and neutrons. The number of protons is the atomic number. The number of protons

More information

The Electromagnetic Spectrum. 7.1 Atomic Theory and Radioactive Decay. Isotopes. 19K, 19K, 19K Representing Isotopes

The Electromagnetic Spectrum. 7.1 Atomic Theory and Radioactive Decay. Isotopes. 19K, 19K, 19K Representing Isotopes 7.1 Atomic Theory and Radioactive Decay Natural background radiation exists all around us. Radioactivity is the release of high energy particles or waves When atoms lose high energy particles and waves,

More information

Step 2: Calculate the total amount of U-238 present at time=0. Step 4: Calculate the rate constant for the decay process.

Step 2: Calculate the total amount of U-238 present at time=0. Step 4: Calculate the rate constant for the decay process. LP#9. A meteor contains 0.556 g of Pb-206 to every 1.00g U-238. Determine the age of the meteor. Step 1: Calculate the moles of each nuclide present. 0.566g Pb-206 x 1.00g U-238 x Step 2: Calculate the

More information

LECTURE 25 NUCLEAR STRUCTURE AND STABILITY. Instructor: Kazumi Tolich

LECTURE 25 NUCLEAR STRUCTURE AND STABILITY. Instructor: Kazumi Tolich LECTURE 25 NUCLEAR STRUCTURE AND STABILITY Instructor: Kazumi Tolich Lecture 25 2 30.1 Nuclear structure Isotopes Atomic mass 30.2 Nuclear stability Biding energy 30.3 Forces and energy in the nucleus

More information

Nuclear fission and fusion are processes that involve extremely large amounts of energy.

Nuclear fission and fusion are processes that involve extremely large amounts of energy. Nuclear Reactions & Energy Nuclear fission and fusion are processes that involve extremely large amounts of energy. Fission = the splitting of a large nucleus into two smaller nuclei, subatomic particles

More information

A is called the mass number gives, roughly, the mass of the nucleus or atom in atomic mass units = amu = u

A is called the mass number gives, roughly, the mass of the nucleus or atom in atomic mass units = amu = u 5/5 A is called the mass number gives, roughly, the mass of the nucleus or atom in atomic mass units = amu = u The number of neutrons in the nucleus is given by the symbol N. Clearly, N = A Z. Isotope:

More information

By Tim, John, Shane, Owen

By Tim, John, Shane, Owen By Tim, John, Shane, Owen A few refreshers Atoms of the same element, which always have an identical number of protons, that have different numbers of neutrons, is an isotope. Protons and neutrons are

More information

Module II: Relativity and Electrodynamics

Module II: Relativity and Electrodynamics Module II: Relativity and Electrodynamics Lecture 2: Lorentz transformations of observables Amol Dighe TIFR, Mumbai Outline Length, time, velocity, acceleration Transformations of electric and magnetic

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

PhysicsAndMathsTutor.com 1

PhysicsAndMathsTutor.com 1 PhysicsAndMathsTutor.com 1 1. Describe briefly one scattering experiment to investigate the size of the nucleus of the atom. Include a description of the properties of the incident radiation which makes

More information

Masses and binding energies

Masses and binding energies Masses and binding energies Introduction to Nuclear Science Simon Fraser University Spring 2011 NUCS 342 January 10, 2011 NUCS 342 (Lecture 1) January 10, 2011 1 / 23 Outline 1 Notation NUCS 342 (Lecture

More information

Mechanical Engineering Introduction to Nuclear Engineering /12

Mechanical Engineering Introduction to Nuclear Engineering /12 Mechanical Engineering Objectives In this lecture you will learn the following In this lecture the population and energy scenario in India are reviewed. The imminent rapid growth of nuclear power is brought

More information

Forces and Nuclear Processes

Forces and Nuclear Processes Forces and Nuclear Processes To understand how stars generate the enormous amounts of light they produce will require us to delve into a wee bit of physics. First we will examine the forces that act at

More information

Nuclear Physics and Nuclear Reactions

Nuclear Physics and Nuclear Reactions Slide 1 / 33 Nuclear Physics and Nuclear Reactions The Nucleus Slide 2 / 33 Proton: The charge on a proton is +1.6x10-19 C. The mass of a proton is 1.6726x10-27 kg. Neutron: The neutron is neutral. The

More information

Answers to test yourself questions

Answers to test yourself questions Answers to test yourself questions Topic 8 8. Energy sources a pecific energy is the energy that can be extracted from a unit mass of a fuel while energy density is the energy that can be extracted from

More information

Module 01 Basics of Nuclear Fission

Module 01 Basics of Nuclear Fission Prof.Dr. Böck Technical University Vienna Atominstitut Stadionallee 2 A-1020 Vienna, Austria ph: ++43-1-58801 141368 boeck@ati.ac.at Module 01 Basics of Nuclear Fission 1.3.2016 Structure of an Atom Fission

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

AN OVERVIEW OF NUCLEAR ENERGY. Prof. Mushtaq Ahmad, MS, PhD, MIT, USA

AN OVERVIEW OF NUCLEAR ENERGY. Prof. Mushtaq Ahmad, MS, PhD, MIT, USA AN OVERVIEW OF NUCLEAR ENERGY Prof. Mushtaq Ahmad, MS, PhD, MIT, USA Outline of the Seminar 2 Motivation and Importance of Nuclear Energy Future Energy Planning in the Kingdom Current Status of Nuclear

More information

Chemistry: The Central Science. Chapter 21: Nuclear Chemistry

Chemistry: The Central Science. Chapter 21: Nuclear Chemistry Chemistry: The Central Science Chapter 21: Nuclear Chemistry A nuclear reaction involves changes in the nucleus of an atom Nuclear chemistry the study of nuclear reactions, with an emphasis in their uses

More information

Aim: What are the two types of Nuclear. Reactions? Do Now: 1. Get into your groups and compare your answers to your homework.

Aim: What are the two types of Nuclear. Reactions? Do Now: 1. Get into your groups and compare your answers to your homework. Aim: What are the two types of Nuclear Reactions? Do Now: 1. Get into your groups and compare your answers to your homework. Nuclear Energy In nuclear reaction, mass is converted into energy; there is

More information

Nuclear Chemistry. Chapter 24

Nuclear Chemistry. Chapter 24 Nuclear Chemistry Chapter 24 Radioactivity Radioisotopes are isotopes that have an unstable nucleus. They emit radiation to attain more stable atomic configurations in a process called radioactive decay.

More information

PHYS 3313 Section 001 Lecture #7

PHYS 3313 Section 001 Lecture #7 PHYS 3313 Section 001 Lecture #7 Wednesday, Feb. 11, 2015 Invariant Quantities The Doppler Effect Relativistic Momentum and Energy Relationship Between Relativistic Quantities Quantization 1 Announcements

More information

Thinking Like a Chemist About Nuclear Change!

Thinking Like a Chemist About Nuclear Change! Thinking Like a Chemist About Nuclear Change! What are we going to learn today? Nuclear Changes REACTIONS ENERGY RELEASED DECAY Poll: Clicker Question There was a nuclear emergency in Japan. The emergency

More information

Lecture 11. Half-Lives of Various Nuclides. Radioactive decays are all first order processes. Professor Hicks Inorganic Chemistry (CHE152)

Lecture 11. Half-Lives of Various Nuclides. Radioactive decays are all first order processes. Professor Hicks Inorganic Chemistry (CHE152) Lecture 11 Professor Hicks Inorganic Chemistry (CHE152) Radioactive decays are all first order processes Half-Lives of Various Nuclides Nuclide Half-Life Type of Decay Th-232 1.4 x 10 10 yr alpha U-238

More information

General Physics I. Lecture 6: Conservation of Momentum. Prof. WAN, Xin 万歆.

General Physics I. Lecture 6: Conservation of Momentum. Prof. WAN, Xin 万歆. General Physics I Lecture 6: Conservation of Momentum Prof. WAN, Xin 万歆 xinwan@zju.edu.cn http://zimp.zju.edu.cn/~xinwan/ Outline Importance of conservation laws in physics Applications of the conservation

More information

Fission Reactors. Alternatives Inappropriate. Fission Reactors

Fission Reactors. Alternatives Inappropriate. Fission Reactors Page 1 of 5 Fission Reactors The Polywell Reactor Nuclear Reactions Alternatives Inappropriate Hidden Costs of Carbon Web Site Home Page Fission Reactors There are about 438 Neutron Fission Power Reactors

More information

Nuclear Reactions. Fission Fusion

Nuclear Reactions. Fission Fusion Nuclear Reactions Fission Fusion Nuclear Reactions and the Transmutation of Elements A nuclear reaction takes place when a nucleus is struck by another nucleus or particle. Compare with chemical reactions!

More information

Nuclear fission is used in nuclear power stations to generate electricity. Nuclear fusion happens naturally in stars.

Nuclear fission is used in nuclear power stations to generate electricity. Nuclear fusion happens naturally in stars. 1 (a) Nuclear fission is used in nuclear power stations to generate electricity. Nuclear fusion happens naturally in stars. (i) Explain briefly the difference between nuclear fission and nuclear fusion.

More information

PHYS:1200 LECTURE 36 ATOMIC AND NUCLEAR PHYSICS (4)

PHYS:1200 LECTURE 36 ATOMIC AND NUCLEAR PHYSICS (4) 1 PHYS:1200 LECTURE 36 ATOMIC AND NUCLEAR PHYSICS (4) This last lecture of the course will focus on nuclear energy. There is an enormous reservoir of energy in the nucleus and it can be released either

More information

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

PHYS 280 Midterm α Fall You may answer the questions in the space provided here, or if you prefer, on your own notebook paper. PHYS 280 Midterm α Fall 2014 Name: You may answer the questions in the space provided here, or if you prefer, on your own notebook paper. Short answers 1. If you are measuring an astrophysical phenomenon,

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

Physics 2D Lecture Slides Oct 13. Vivek Sharma UCSD Physics

Physics 2D Lecture Slides Oct 13. Vivek Sharma UCSD Physics Physics D Lecture Slides Oct 13 Vivek Sharma UCSD Physics Quiz : Wild Wild West got a Bit too wild 50m/s x ScarFace MadBull In the old west, a sheriff riding on a train traveling 50m/s sees a shootout

More information

Nuclear Reactions. Thornton and Rex, Ch. 13. Otto Hahn and Lise Meitner

Nuclear Reactions. Thornton and Rex, Ch. 13. Otto Hahn and Lise Meitner Nuclear Reactions Thornton and Rex, Ch. 13 Otto Hahn and Lise Meitner Reaction Kinematics Consider a general reaction, A (x, y) B or A + x Æ y + B with target A at rest. Ex. 9 Be 4 + 4 a 2 Æ 1 n 0 + 12

More information

Chapter 13 Nuclear physics

Chapter 13 Nuclear physics OCR (A) specifications: 5.4.11i,j,k,l Chapter 13 Nuclear physics Worksheet Worked examples Practical: Simulation (applet) websites nuclear physics End-of-chapter test Marking scheme: Worksheet Marking

More information

THE NUCLEUS OF AN ATOM

THE NUCLEUS OF AN ATOM VISUAL PHYSICS ONLINE THE NUCLEUS OF AN ATOM Models of the atom positive charge uniformly distributed over a sphere J. J. Thomson model of the atom (1907) ~2x10-10 m plum-pudding model: positive charge

More information

Fission and Fusion Book pg cgrahamphysics.com 2016

Fission and Fusion Book pg cgrahamphysics.com 2016 Fission and Fusion Book pg 286-287 cgrahamphysics.com 2016 Review BE is the energy that holds a nucleus together. This is equal to the mass defect of the nucleus. Also called separation energy. The energy

More information

Energy, Work, and Power

Energy, Work, and Power Matthew W. Milligan, Work, and Power Conservation Laws an Alternative to Newton s Laws Matthew W. Milligan, Work, and Power I. - kinetic and potential - conservation II. Work - dot product - work-energy

More information

Chapter 10 - Nuclear Physics

Chapter 10 - Nuclear Physics The release of atomic energy has not created a new problem. It has merely made more urgent the necessity of solving an existing one. -Albert Einstein David J. Starling Penn State Hazleton PHYS 214 Ernest

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

Preview. Subatomic Physics Section 1. Section 1 The Nucleus. Section 2 Nuclear Decay. Section 3 Nuclear Reactions. Section 4 Particle Physics

Preview. Subatomic Physics Section 1. Section 1 The Nucleus. Section 2 Nuclear Decay. Section 3 Nuclear Reactions. Section 4 Particle Physics Subatomic Physics Section 1 Preview Section 1 The Nucleus Section 2 Nuclear Decay Section 3 Nuclear Reactions Section 4 Particle Physics Subatomic Physics Section 1 TEKS The student is expected to: 5A

More information

Chapter 22. Preview. Objectives Properties of the Nucleus Nuclear Stability Binding Energy Sample Problem. Section 1 The Nucleus

Chapter 22. Preview. Objectives Properties of the Nucleus Nuclear Stability Binding Energy Sample Problem. Section 1 The Nucleus Section 1 The Nucleus Preview Objectives Properties of the Nucleus Nuclear Stability Binding Energy Sample Problem Section 1 The Nucleus Objectives Identify the properties of the nucleus of an atom. Explain

More information

Chapter 21 Nuclear Chemistry

Chapter 21 Nuclear Chemistry Chapter 21 Nuclear Chemistry The Nucleus Remember that the nucleus is comprised of the two nucleons, protons and neutrons. The number of protons is the atomic number. The number of protons and neutrons

More information

1897 J.J. Thompson discovers the electron

1897 J.J. Thompson discovers the electron CHAPTER 1 BASIC CONCEPTS OF NUCLEAR PHYSICS 1.1 Historical survey: The origin of nuclear physics and the progress after can be understand from the historical review as follow: 1895 The discovery of X-Ray

More information

DEVIL PHYSICS THE BADDEST CLASS ON CAMPUS IB PHYSICS

DEVIL PHYSICS THE BADDEST CLASS ON CAMPUS IB PHYSICS DEVIL PHYSICS THE BADDEST CLASS ON CAMPUS IB PHYSICS TSOKOS LESSON 7-2 NUCLEAR REACTIONS Review Videos-Radioactivity2 Review Videos - Strong and Weak Nuclear Forces Essential Idea: Energy can be released

More information

Nuclear Properties. Thornton and Rex, Ch. 12

Nuclear Properties. Thornton and Rex, Ch. 12 Nuclear Properties Thornton and Rex, Ch. 12 A pre-history 1896 Radioactivity discovered - Becquerel a rays + (Helium) b rays - (electrons) g rays 0 (EM waves) 1902 Transmutation observed - Rutherford and

More information

Nuclear Physics and Radioactivity

Nuclear Physics and Radioactivity Nuclear Physics and Radioactivity Structure and Properties of the Nucleus Nucleus is made of protons and neutrons Proton has positive charge: Neutron is electrically neutral: Neutrons and protons are collectively

More information

NUCLEAR ENERGY! DAY 1: (RADIATION, FISSION, FUSION)

NUCLEAR ENERGY! DAY 1: (RADIATION, FISSION, FUSION) NUCLEAR ENERGY! DAY 1: (RADIATION, FISSION, FUSION) Nucleus Stability Stability of the nucleus depends on the nuclear forces that act between protons and neutrons Protons repel each other Protons attract

More information

Nuclear Physics. Slide 1 / 87. Slide 2 / 87. Slide 3 / 87. Table of Contents.

Nuclear Physics. Slide 1 / 87. Slide 2 / 87. Slide 3 / 87. Table of Contents. Slide 1 / 87 Slide 2 / 87 Nuclear Physics www.njctl.org Table of Contents Slide 3 / 87 Click on the topic to go to that section Nuclear Structure Binding Energy and Mass Defect Radioactivity Nuclear Half-life

More information

Nuclear Physics

Nuclear Physics Slide 1 / 87 Slide 2 / 87 Nuclear Physics www.njctl.org Slide 3 / 87 Table of Contents Click on the topic to go to that section Nuclear Structure Binding Energy and Mass Defect Radioactivity Nuclear Half-life

More information

Ch 17 Radioactivity & Nuc. Chemistry Study Guide Accelerated Chemistry SCANTRON

Ch 17 Radioactivity & Nuc. Chemistry Study Guide Accelerated Chemistry SCANTRON Ch 17 Radioactivity & Nuc. Chemistry Study Guide Accelerated Chemistry SCANTRON Name No-Calculators Allowed /65 MULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers

More information

Chapter 21. Chemistry, The Central Science, 10th edition Theodore L. Brown; H. Eugene LeMay, Jr.; and Bruce E. Bursten

Chapter 21. Chemistry, The Central Science, 10th edition Theodore L. Brown; H. Eugene LeMay, Jr.; and Bruce E. Bursten , The Central Science, 10th edition Theodore L. Brown; H. Eugene LeMay, Jr.; and Bruce E. Bursten Chapter 21 John D. Bookstaver St. Charles Community College St. Peters, MO 2006, Prentice Hall, Inc. The

More information

PHYSICS CET-2014 MODEL QUESTIONS AND ANSWERS NUCLEAR PHYSICS

PHYSICS CET-2014 MODEL QUESTIONS AND ANSWERS NUCLEAR PHYSICS PHYSICS CET-2014 MODEL QUESTIONS AND ANSWERS NUCLEAR PHYSICS IMPORTANT FORMULE TO BE REMEMBERED IMPORTANT FORMULE TO BE REMEMBERED 1. Identify the correct statement with regards to nuclear density a) It

More information

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

Name: New Document 1. Class: Date: 54 minutes. Time: 54 marks. Marks: Comments: Page 1 of 22

Name: New Document 1. Class: Date: 54 minutes. Time: 54 marks. Marks: Comments: Page 1 of 22 New Document Name: Class: Date: Time: 54 minutes Marks: 54 marks Comments: Page of 22 (a) Uranium has two natural isotopes, uranium-235 and uranium-238. Use the correct answer from the box to complete

More information