Nuclear Energy Nuclear fission is when a heavy nucleus splits into two smaller nuclei. The total mass of the products is less than the original mass. The.

Slides:



Advertisements
Similar presentations
Radioactivity.
Advertisements

Modern Physics By Neil Bronks Atoms C 12 6 Mass Number Mass Number - Number of protons + Neutrons. Atomic Number Atomic Number - Number of protons In.
Transmutations involve more than just the conversion of one element into another—they also involve the conversion of mass into energy. Nuclear energy released.
20th Century Discoveries
Nuclear Reactions, Transmutations, Fission and Fusion
7: Atomic and Nuclear Physics 7.3 Nuclear reactions, fission and fusion.
Lecture 14 Fission and Fusion. Elementary Particles. Nuclear Fission Nuclear Fusion Fundamental Interaction (Forces) Elementary Particles.
Fundamental Forces of the Universe
NUCLEAR FUSION & NUCLEAR FISSION Noadswood Science, 2012.
Chapter 25 Nuclear Chemistry 25.3 Fission and Fusion
Chapter 10 Nuclear Physics. Copyright © Houghton Mifflin Company 10-2 Section 10.1: Symbols of the Elements An element is the fundamental atom by which.
Nuclear Physics Notes CP Physics Ms. Morrison.
Prentice Hall © 2003Chapter 21 Chapter 21 Nuclear Chemistry CHEMISTRY The Central Science 9th Edition.
A nucleus can be specified By an atomic number and a Mass number.
Nuclear Physics Year 13 Option 2006 Part 2 – Nuclear Fusion.
Sub-Atomic Particles Another building block of matter?? Richard Lasky – Summer 2010.
Nuclear Physics Selected Topics 5 –Fission and Fusion.
Power of the Sun. Conditions at the Sun’s core are extreme –temperature is 15.6 million Kelvin –pressure is 250 billion atmospheres The Sun’s energy out.
8/5/2002Ulrich Heintz - Quarknet Particle Physics what do we know? Ulrich Heintz Boston University.
Nuclear Force and Particles
Modern Physics Introduction To examine the fundamental nuclear model To examine nuclear classification To examine nuclear fission and fusion.
Alternative Energy Sources
Particle Physics Intro. What’s Stuff Made Of…Really? All particles can be grouped into two categories: Fermions and Bosons Things to know about Fermions:
Nuclear Fission and Fusion
General Physics (PHY 2140) Lecture 20 Modern Physics
23.4 Nuclear energy NUCLEARNUCLEAR POWERPOWER Millstone Station.
23.4 Nuclear energy NUCLEARNUCLEAR POWERPOWER Millstone Station.
General, Organic, and Biological Chemistry Fourth Edition Karen Timberlake 4.6 Nuclear Fission and Fusion Chapter 4 Nuclear Chemistry © 2013 Pearson Education,
General, Organic, and Biological ChemistryCopyright © 2010 Pearson Education, Inc.1 Chapter 4 Nuclear Chemistry 4.6 Nuclear Fission and Fusion.
Nuclear Chemistry L. Scheffler. The Nucleus The nucleus is comprised of the two nucleons: protons and neutrons. The number of protons is the atomic number.
1 Chapter 9 Nuclear Radiation 9.6 Nuclear Fission and Fusion Copyright © 2009 by Pearson Education, Inc.
Ionizing Radiation, Nuclear Energy, & Elementary Particles
Nuclear Fission & Fusion Objectives: Describe what happens in a nuclear chain reaction. Explain the use of water in the storage of spent fuel rods. Distinguish.
Modern Physics. Atom Nucleons – subatomic particles in the atom’s nucleus (protons and neutrons). Ion – An atom with a net electric charge which is due.
My Chapter 30 Lecture.
Subatomic Physics Chapter Properties of the Nucleus The nucleus is the small, dense core of an atom. Atoms that have the same atomic number but.
Unit 12: Part 5 Nuclear Reactions and Elementary Particles
Fisica Generale - Alan Giambattista, Betty McCarty Richardson Copyright © 2008 – The McGraw-Hill Companies s.r.l. 1 Chapter 30: Particle Physics Fundamental.
Atoms Chapter 4.
Nuclear Fission is the process by which the nucleus of an atom splits into two or more nuclei and some by- products.
Aim: How can we explain the four fundamental forces and the standard model? Do Now: List all the subatomic particles that you can think of.
Ionizing radiation is made up of photons and/or moving particles that have sufficient energy to knock an electron out of an atom or molecule.
Particles and how they interact
Fusion in the Stars Nunez & Panogalinog. Nuclear Fusion in stars is one of the most important reasons which make life on Earth possible! ○ HOW IS THAT.
Basic Concepts of Nuclear Physics Part II By Benjamin Thayer PHY3091.
© John Parkinson 1 e+e+ e-e- ANNIHILATION © John Parkinson 2 Atom 1x m n n n n Nucleus 1x m U Quarks 1x m U D ? ? ?
The Nucleus Nucleons- the particles inside the nucleus: protons & neutrons Total charge of the nucleus: the # of protons (z) times the elementary charge.
NUCLEAR FISSION AND FUSION. Specification Radioactivity and particles Particles describe the results of Geiger and Marsden’s experiments with gold foil.
Chapter 30: Nuclear Energy and Elementary Particles
A photon with a wavelength of 2
Basic Chemistry Copyright © 2011 Pearson Education, Inc. 1 Chapter 16 Nuclear Radiation 16.6 Nuclear Fission and Fusion.
Controlled Nuclear Fusion The JET Project
Ch. 28 Nuclear Chemistry C. Smith. I. Nuclear Radiation A. Radioactivity 1. Radioisotopes are unstable isotopes that have unstable nuclei. 2. They gain.
NUCLEAR ENERGY. The daughter nuclei in the reaction above are highly unstable. They decay by beta emission until they reach stable nuclei.
Discovery of the nucleus Rutherford carried out experiments to see what happened when alpha particles (2 neutrons and 2 protons) were fired at metal foil.
Intro. Into Nuclear Energy And you. What are the fundamental forces of the Universe??? Gravitational Force (interaction of massive bodies) Electromagnetic.
Chapter 30 Nuclear Energy and Elementary Particles.
Chemistry - Unit 13.  Discovery of Radioactivity  In 1895 Wilhelm Roentgen found that invisible rays were emitted when electrons bombarded the surface.
25.3 Fission and Fusion > 1 Copyright © Pearson Education, Inc., or its affiliates. All Rights Reserved. Chapter 25 Nuclear Chemistry 25.1 Nuclear Radiation.
Nuclear Physics An Introduction. What does it mean when something is “Radioactive”? Atomic nuclei that emit particles and energy are said to be radioactive.
Chapter 9.2 Nuclear Radiation.
Fission and Fusion of Atomic Nuclei
Chapter 5 Energy Resources
Aim: How can we describe Fundamental Particles?
alpha beta gamma electron energy electron energy electron positive
ELEMENTARY PARTICLES.
Unit 5.4 Nuclear Fission and Fusion
Subatomic Particles and Quantum Theory
Intro. Into Nuclear Energy
Fission and Fusion.
Presentation transcript:

Nuclear Energy Nuclear fission is when a heavy nucleus splits into two smaller nuclei. The total mass of the products is less than the original mass. The mass difference results in an energy gain, about 200MeV for each fission event. 0 1 n U-----> Ba Kr n The intermediate stage, U, which is very unstable is when the nucleus elongates and compresses until finally splitting. The three neutrons are available to bombard other nuclei.

Nuclear Reactors When a nucleus undergoes neutron bombardment and fission occurs, the neutrons released bombard other nuclei and if not controlled result in a chain reaction releasing a large amount of energy in a chain reaction, an explosion. A nuclear reactor is a system designed to maintain a self sustained chain reaction releasing controlled energy.

Cont. The average number of neutrons produced per fission event is 2.5, defined as the reproduction constant K. In reality K is less than 2.5. Self sustain chain reaction occurs when K = 1, then the reactor is said to be critical. When K is less than 1 it is subcritical and the reaction dies out. If it is greater than 1 it is super critical and the reaction is runaway.

Cont. When neutrons are released they have high kinetic energy and need to be slowed down to be absorbed by 235 U. This is done by the use of a Moderator, originally Carbon later heavy water. The moderator absorbs the kinetic energy of the neutrons allowing it to be captured by the nucleus causing fission. Not all neutrons are captured some leak out of the core before capture. A large surface area to volume ratio in the reactor will reduce the leakage. To much leakage and the reaction will stop.

Control of Power Level If nuclear bombardment is not controlled the reactor becomes too hot and will melt and/or the chain reaction is too fast and an explosion may occur. Temperature if often controlled by cooling water that removes excess heat from the core. In addition it is necessary to use control rods that absorb excess neutrons before being captured by the fission process. These rods made of either graphite, boron or cadmium are inserted between the fuel rods and adjusted to control the amount of neutron absorption.

Cont. The heat from a nuclear reactor is used to produce steam that is used to run a turbine that in turn powers a generator. Power production whether by nuclear reactors, burning fossil fuel or some other means from the point of turning a turbine to powering a generator are virtually all the same.

Nuclear Fusion Fusion is the opposite to fission in that two smaller nuclei are combined to form a heavy nucleus which also results in the release of energy from the conversion of matter. The sun provides heat due to nuclear fusion of protons (hydrogen ions) to deuterium, then a hydrogen ion and deuterium to 3He and finally either hydrogen and 3He to 4He or two 3He to 4He and two hydrogen ions

Cont. First 1 1 H H---> 1 2 D + e + + v then 1 1 H D ---> 2 3 He +  then either 1 1 H He ---> 2 4 He + e + + v or 2 3 He He ---> 2 4 He + 2( 1 1 H) The energy liberated is carried by the gamma rays, positrons and neutrinos. The gamma rays are absorbed increasing the temperature, the positrons combine with electrons forming gamma rays and are absorbed, the neutrinos escape the star taking with them energy.

A Star Formation A star is formed by a shock wave from a supernova collapsing a cosmic dust cloud upon itself. As the particles collapse they accelerate and generate huge gravitation force and heat. As protons collide they repel and gravity continues to attract. The heat generated is in the order of 10 7 K. As fusion occurs the energy liberated prevents the star from collapsing under its own gravity and the cycle continues.

Fusion Power A large amount of energy is released in a thermonuclear reaction (fusion) and comparatively few radioactive by-products are formed. However proton-proton reaction are unrealistic due to the need of extremely high temperatures and pressures. The sun functions because of the extreme density of protons at its core. Reaction of deuterium with tritium seems promising but for the confinement of plasma at temperatures 10 8 K and the time required.

Magnetic Field Confinement It is the combination of two magnetic fields either helical or spiral in design used to confine plasma in a chamber and prevent it from touching the vessel walls. Temperatures 30 times hotter than the sun are produced by introduction of high kinetic energy neutral particles into the plasma or by the addition of energy from intense lasers

Elementary Particles Atom from ‘atomos’ indivisible remained until the early 20th century, the proton neutron and electron until 1937 and then collision of high energy particles discovered new particles. From 1960 on except for the electron, photon and a few others subatomic particles matter is made of quarks.

Forces of Nature Force relative range of mediating strength force field particle Strong 1 short 1fm Gluon electro long  1/r 2 Photon magnetic Weak 10 -(6) short fm nucleus Gravitational long  1/r 2 galaxy

Antiparticles For virtually every particle there is an antiparticle, having the same mass but opposite charge. Electron-positron, proton-antiproton, neutron-antineutron Exceptions are the photon and neutral pion which are their own antiparticles

Mesons Two mesons of slightly different mass, the muon (  ) has weak and electromagnetic interaction and plays no role in strong nuclear forces. Its life time around 2.2x10 -6 s decays to an electron, a neutrino and an antineutrino. The other, pi meson, pion (  ) comes in three varieties  -  +  o and decays into muon and an antineutrino in 2.6x10 -8 s. The pion is involved in transferring energy between nucleons

Particle Classification All particles except the photon can be classified into two group.1) Hadrons which include mesons and baryons are distinguished by mass and spin. All mesons decay to electrons, positrons neutrinos and photons. Baryons have masses equal to or larger than a proton and except for the proton all decay and produce a proton. Protons are composed of quarks.

Cont. 2) Leptons (meaning light), include electrons, muons and a tau and all have neutrinos associated with them. They have weak interaction and are considered truly elementary. Hadrons are composed of two or three fundamental constituents called quarks, (u,d,s). Quarks have fractional electronic charge and each have an antiquark of opposite charge.

Colored Quarks The three quarks are colored red blue and green. The antquarks are anti-red anti-blue and anti- green. Baryons consist of the three different colored quarks and mesons consist of one color and an anti quark of the anti-color. Both baryons and meson are colorless. The strong force between quarks is called color force and is carried by massless particles called gluons. Different colored quarks attract each other as opposites oppose. When gluon are absorbed or released the quarks color changes.