Term 3 Week 2 Nuclear Fusion & Nuclear Fission

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

Nuclear Energy Learning Outcomes

Nuclear Energy Learning Outcomes. Nuclear Fission. Chain Reaction

Nuclear Fusion 1 of 24 Boardworks Ltd 2011

Atomic and Nuclear Physics. Topic 7.3 Nuclear Reactions

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

WELCOME TO PERIOD 18: CONSEQUENCES OF NUCLEAR ENERGY

Nuclear Chemistry Unit

The Physics of Nuclear Reactors. Heather King Physics 420

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

Isotopes. An isotope is an atom of the same element (same number of protons) that varies in the number of neutrons.

Isotopes. An isotope is an atoms of the same element (same number of protons) that vary in the number of neutrons.

Nuclear Chemistry. Transmutations and the Creation of Elements

Nuclear Physics and Nuclear Reactions

Write down the nuclear equation that represents the decay of neptunium 239 into plutonium 239.

Fission and Fusion Book pg cgrahamphysics.com 2016

NUCLEI. Atomic mass unit

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

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

2 Energy from the Nucleus

Nuclear power plants can generate large amounts of electricity.

Unit 3: Chemistry in Society Nuclear Chemistry Summary Notes

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

Episode 528: Controlling fission

Chapter 21

Chapter 10 Section 4 Notes

Physics 30 Modern Physics Unit: Fission and Fusion

Nuclear Energy; Effects and Uses of Radiation

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

FUSION NEUTRON DEUTERIUM HELIUM TRITIUM.

Chapter 12: Nuclear Reaction

Fission & Fusion Movie

Nuclear processes: Vocabulary: Radioactive decay Isotope Alpha particle Beta particle Transmutation Strong Nuclear Force Fusion fission

Introducing nuclear fission The Fizzics Organization

Fundamental Forces of the Universe

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

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

UNIT 13: NUCLEAR CHEMISTRY

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

Special!Area!of!Study!1! Energy!from!the!nucleus!

Nuclear Reactions. Fission Fusion

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

Chemistry: The Central Science. Chapter 21: Nuclear Chemistry

RADIOACTIVITY & HALF-LIFE Part 3

Nuclear Reactions A Z. Radioactivity, Spontaneous Decay: Nuclear Reaction, Induced Process: x + X Y + y + Q Q > 0. Exothermic Endothermic

Forces and Nuclear Processes

Chapter 10. Answers to examination-style questions. Answers Marks Examiner s tips. 1 (a) (i) 238. (ii) β particle(s) 1 Electron antineutrinos 1

Nuclear processes: Vocabulary: Radioactive decay Isotope Alpha particle Beta particle Transmutation Strong Nuclear Force Fusion Fission

UNIT 10 RADIOACTIVITY AND NUCLEAR CHEMISTRY

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

Fundamentals of Nuclear Power. Original slides provided by Dr. Daniel Holland

Nuclear Energy ECEG-4405

UNIT 10 RADIOACTIVITY AND NUCLEAR CHEMISTRY

10.4 Fission and Fusion

What colour is the insulation around the wire connected to the live pin inside the plug? ... (1) (1)

NJCTL.org 2015 AP Physics 2 Nuclear Physics

One nucleus splits into two smaller nuclei and typically a few neutrons by the bombardment of a neutron. U-235 is the only naturally occurring

Alta Chemistry CHAPTER 25. Nuclear Chemistry: Radiation, Radioactivity & its Applications

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

(b) The type of matter is irrelevant since the energy is directly proportional to mass only

Some stars will finish their life cycle as a black dwarf and other stars as a black hole.

u d Fig. 6.1 (i) Identify the anti-proton from the table of particles shown in Fig [1]

Lecture PowerPoint. Chapter 31 Physics: Principles with Applications, 6 th edition Giancoli

11.5 Nuclear Reactions: Fusion

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

Nuclear Chemistry. The nuclei of some unstable isotopes change by releasing energy and particles, collectively known as radiation

Card #1/28. Card #2/28. Science Revision P2. Science Revision P2. Science Revision P2. Card #4/28. Topic: F = ma. Topic: Resultant Forces

Carbon Dating. Principles of Radiometric Dating. 03 nuclear decay and the standard model June 05, 2013

NUCLEI 1. The nuclei having the same atomic number (Z), but different mass numbers (A) are called isotopes.

Nuclear Fission & Fusion

Nuclear Chemistry. Chapter 24

Lecture PowerPoints. Chapter 31 Physics: Principles with Applications, 7th edition Giancoli

nuclear chemical change CH4 + 2O2 CO2 + 2H2O carbon dating

LECTURE 25 NUCLEAR STRUCTURE AND STABILITY. Instructor: Kazumi Tolich

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

Radioactivity & Nuclear. Chemistry. Mr. Matthew Totaro Legacy High School. Chemistry

Chapter 16 Nuclear Chemistry. An Introduction to Chemistry by Mark Bishop



1. Four different processes are described in List A. The names of these processes are given in List B.

1ST SEM MT CHAP 22 REVIEW

MockTime.com. Ans: (b) Q6. Curie is a unit of [1989] (a) energy of gamma-rays (b) half-life (c) radioactivity (d) intensity of gamma-rays Ans: (c)

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

Nuclear Physics Questions. 1. What particles make up the nucleus? What is the general term for them? What are those particles composed of?

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

Ch Radioactivity. Henry Becquerel, using U-238, discovered the radioactive nature of elements in 1896.

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

Nuclear Physics

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

Energy Changes in Chemical and Nuclear Reactions

NUCLEAR PHYSICS: solutions to higher level questions

Energy. on this world and elsewhere. Visiting today: Prof. Paschke

Name Date Class NUCLEAR RADIATION. alpha particle beta particle gamma ray

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

Nuclear Physics. Nuclear Structure. Slide 1 / 87 Slide 2 / 87. Slide 4 / 87. Slide 3 / 87. Slide 6 / 87. Slide 5 / 87. Table of Contents.

Nuclear Physics

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

Chapter 7 Review. Block: Date:

Fission Reactors. Alternatives Inappropriate. Fission Reactors

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

Transcription:

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 small nuclei such as hydrogen to form larger nuclei The energy released by this process is vast water contains lots of hydrogen atoms If we could make a fusion reactor on Earth then a glass of water could provide the same amount of energy as a tanker full of petrol!

Fusion Reactions 2 small nuclei release energy when they are fused together to form a single, larger nucleus The process releases energy if the relative mass of the product nucleus is no more than about 55 (the same as an iron nucleus) Energy must be supplied to create bigger nuclei

Nuclear Fusion & Stars The Sun consists of about 75% hydrogen (H) and 25% helium (He) The core is so hot that it consists of a plasma of bare nuclei with no electrons these nuclei move about and fuse together when they collide When they fuse they release energy

Nuclear Fusion & Stars Nuclear fusion involves two atomic nuclei joining to make a large nucleus energy is released when this happens The Sun and other stars use nuclear fusion to release energy Complex Overall hydrogen nuclei join to form helium nuclei The Sun is changing its composition from hydrogen to helium: - Hydrogen-1 nuclei fuse with hydrogen-2 nuclei to make helium-3 nuclei 1 1 H + 2 1 H 3 2 He

Nuclear Fusion On Earth Technically very difficult to produce nuclear fusion on Earth Plasma of light nuclei must be heated to extremely high temperatures before the nuclei will fuse This temperature is needed because 2 nuclei approaching each other will try and repel each other (due to the positive charge) move them fast enough (i.e. with temperature) then they will overcome this force of repulsion, and fuse

Nuclear Fusion On Earth There are some experimental reactors, however the process is extremely complicated and currently they only work for a few minutes: - Plasma is heated by passing a very high electric current through Plasma is contained by a magnetic field (if it touched the reactor walls it would go cold, and fusion would cease)

Powerful Future Practical fusion reactions could meet all our energy needs: - The fuel for fusion reactors is readily available as heavy hydrogen, present in sea water The reaction product, helium, is a nonradioactive inert gas so is harmless The energy released could be used to then generate electricity

Hydrogen Bomb A hydrogen bomb is a uranium bomb, surrounded by the H isotope When the uranium bomb explodes it makes the surrounding hydrogen fuse and release even more energy a single hydrogen bomb would destroy Sydney 2 1

Nuclear Fission Energy is released in a nuclear reactor as a result of nuclear fission The nucleus of an atom of a fissionable substance splits into two smaller fragment nuclei This event can cause other fissionable nuclei to split, leading to a chain reaction of fission events Two isotopes in common use as nuclear fuels are uranium-235 and plutonium-239

Splitting Atoms Fission is another word for splitting (splitting a nucleus is called nuclear fission) Uranium or plutonium isotopes are normally used as the fuel in nuclear reactors, because their atoms have relatively large nuclei that are easy to split, especially when hit by neutrons When a uranium-235 or plutonium-239 nucleus is hit by a neutron, the following happens: - The nucleus splits into two smaller nuclei, which are radioactive Two or three more neutrons are released Some energy is released

Chain The additional neutrons released may also hit other uranium or plutonium nuclei and cause them to split even more neutrons are then released, which in turn can split more nuclei This is called a chain reaction in nuclear reactors the chain reaction is controlled, stopping it going too fast In a nuclear bomb the idea is the opposite to this!

Chain Reaction Krypton n n n More decays Uranium n Barium

Nuclear Reactors A nuclear reactor consists of uranium fuel rods, spaced evenly in the reactor core The reactor core is a thick steel vessel containing the fuel rods, control rods and water at high pressure The fission neutrons are slowed down by the collisions with the atoms in the water (the water acts as a moderator, slowing the fission neutrons down) Without a moderator the fast neutrons would not cause further fission of the nuclear fuel

Nuclear Reactors Nuclear reactors use the heat from nuclear reactions in the nuclear fuel to boil Steam from the boiling water in the (PWR) makes a turbine spin, which in turn makes the generator turn Control rods (cadmium / boron) absorb surplus neutrons, controlling the chain reaction

Safety The reactor core is a thick steel vessel which can withstand very high temperatures and pressures The core is enclosed by thick concrete walls, absorbing any radiation which escapes through the steel vessel - in an emergency the control rods are dropped completely into the core, reducing the reaction to almost zero

Enriched Fuel & Critical Mass The fuel in a nuclear reactor must contain fissionable isotopes Most reactors use enriched uranium which is ~97% non-fissionable U-238 and ~3% fissionable U-235 In comparison natural uranium is >99% non-fissionable U-238 *A nuclear bomb has two lumps of pure U-235 or Pu-239 (each lump cannot produce a chain reaction because it loses too many fission neutrons, but bringing them together enables the reaction to occur)

Summary: Fission Fission is a process in which a nucleus with a large mass number splits into two nuclei, which have smaller mass numbers. Neutrons are usually released when fission takes place Fission of a nucleus may be spontaneous, Can also be induced by bombarding a nucleus with a neutron. Induced fission is used to generate nuclear power and for weapons Products formed during fission gain kinetic energy. It is this energy that is harnessed in nuclear power stations

Summary: Fusion Fusion is a process in which two nuclei combine to form a nucleus of larger mass number. Fusion is the main nuclear process that occurs in the Sun and other stars. The products of fusion reactions also gain kinetic energy that can be harnessed.

BE, Fission and Fusion It takes energy, BE, to hold nucleons together as a nucleus. Iron has a mass number of 56 and is one of the most stable of all the elements. (high binding energy per nucleon). Elements with lower and higher mass numbers per nucleon are less stable. The total mass of a nucleus is less than the total mass of the nucleons that make up the nucleus. This difference is known as the mass defect and is equivalent to the binding energy of the nucleus, using E = mc 2. In fission, an unstable nucleus is converted into more stable nuclei with a smaller total mass. This mass defect is the binding energy that is released. In fusion, the mass of the nucleus that is created is slightly less than the total mass of the original nuclei. Again the mass defect is the binding energy that is released, since the nucleus that is formed is more stable.