Radiation Protection III NUCP 2331

Slides:



Advertisements
Similar presentations
Radioactivity.
Advertisements

Nuclear Chemistry A Short Study.
Unit 2 Notes – Radioactivity
Unit 2 Notes – Radioactivity
3/2003 Rev 1 I.3.7 – slide 1 of 23 Part I Review of Fundamentals Module 3Interaction of Radiation with Matter Session 7Neutron Interactions Module I.3.7.
NE Introduction to Nuclear Science Spring 2012
Interaction of radiation with matter - 5
Basic of radiation Prof. Dr. Moustafa. M. Mohamed Vice Dean
The equation E = mc 2 is probably the most recognized symbol of physics. This equation tells us that matter and energy are really two forms of the same.
Transmutation (Objective 25
 Atoms tend to attain stable electron configurations  All atoms like to be happy (balanced or neutral)  A nuclear reaction deals with reactions in.
Prentice Hall © 2003Chapter 21 Chapter 21 Nuclear Chemistry CHEMISTRY The Central Science 9th Edition.
Nuclear Chemistry Chapter 21. Warm Up Astatine – 210 goes through alpha decay, beta decay and alpha decay in that order to become stable. Write the reactions.
When the nucleus of an atom breaks down to form a different element.
Nuclear / Subatomic Physics Physics – Chapter 25 (Holt)
Neutral Particles. Neutrons Neutrons are like neutral protons. –Mass is 1% larger –Interacts strongly Neutral charge complicates detection Neutron lifetime.
Chapter 4 Radioactivity and Medicine A CT scan (computed tomography) of the brain using X-ray beams.
Nuclear Chemistry Nuclear chemistry is the study of the changes of the nucleus of atoms. Nuclear Reactions involve changes within the nucleus where as.
Radiation, nuclear fusion and nuclear fission
Nuclear Fission and Fusion
NUCLEAR CHEMISTRY 2F-1 (of 15) NUCLEONS – The particles found in the nucleus Protons (+) Neutrons (0) ATOMIC NUMBER (Z) – The number of protons in the.
Nuclear Physics Year 13 Option 2006 Part 3 – Nuclear Fission.
Nuclear Fundamentals Part I Unleashing the Power of the Atom.
Nuclear and Radiation Physics, BAU, 1 st Semester, (Saed Dababneh). 1 Nuclear Fission Q for 235 U + n  236 U is MeV. Table 13.1 in Krane:
Nuclear and Radiation Physics, BAU, First Semester, (Saed Dababneh). 1 Nuclear Fission 1/ v 235 U thermal cross sections  fission  584 b. 
Ttp:// Nuclear Chemistry.
Chapter 21: Nuclear Chemistry The study of nuclear reactions with an emphasis on their uses in chemistry and their effects on biological systems.
Radioactivity and Nuclear Reactions. How Did It All Happen? Radioactivity 4.16.
Nuclear Chemistry. Radioactive Decay Spontaneous breakdown of an atom’s nucleus Breakdown results in a lighter nucleus Emits electromagnetic radiation.
Nuclear Chemistry.
Nuclear Chemistry.
Chapter 9 Nuclear Radiation
Radiation. Atomic Anatomy Atoms –electrons (e-) –protons (p+) –neutrons (n)
Unit 12 – Nuclear Chemistry. Part II Key Terms Alpha decay – spontaneous decay of a nucleus that emits a helium nucleus and energy Beta decay – spontaneous.
Neutrons (Basic Concepts).  It is desirable to classify neutrons according to their kinetic energy into:
Alpha and Beta Interactions
Radioactivity.
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.
Nuclear Chemistry Nuclear Reactions. Reactions Chemical Reactions- atoms want stable electron configuration Nuclear Reaction- unstable isotopes (radioisotope)
RADIATION *Penetrating rays emitted by a radioactive source *Ranges from Cosmic and Gamma Rays to Radio Waves.
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.
Basic Concepts of Nuclear Physics Part II By Benjamin Thayer PHY3091.
1 Interaction Between Ionizing Radiation And Matter, Part 3 Neutrons Audun Sanderud Department of Physics University of Oslo.
What is a Fission Reactor?What is a Fission Reactor?  The Principles of Fission Reactors are similar to that of an Atomic Reactor  Fission Reactors.
1 Atomic Structure Protons 1 1 p ( amu) Neutrons 1 0 n ( amu) Electrons ( amu) Neon Ne ( amu)
P. Sci. Unit 12 Nuclear Radiation Chapter 10. Essential Questions 1)Identify four types of nuclear radiations and compare and contrast their properties.
Review of Fundamentals
The atom orbiting electrons Nucleus (protons and neutrons)
Nuclear Chemistry. Radioactivity The process by which materials give off such rays radioactivity; the rays and particles emitted by a radioactive source.
Nuclear Fission And Nuclear Fusion
Interaction Ionizing Radiation with Matter BNEN Intro William D’haeseleer BNEN - Nuclear Energy Intro W. D'haeseleer
A. Dokhane, PHYS487, KSU, 2008 Chapter1- Neutron Reactions 1 NEWS Lecture1: Chapter 0 is already on my Website.
Energy Unit Learning Goal 3: Examine how changes in the nucleus of an atom result in emissions of radioactivity.
Ch. 28 Nuclear Chemistry C. Smith. I. Nuclear Radiation A. Radioactivity 1. Radioisotopes are unstable isotopes that have unstable nuclei. 2. They gain.
P. Sci. Unit 12 Nuclear Radiation Chapter 10. Nuclear Radiation Strong Nuclear force – the force that holds protons and neutrons together. Remember that.
All pure substances are made of atoms. All substances can be divided but not “ad infinitum” (forever) Atoms are the smallest part that cannot be divided.
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.
Chapter 25: Nuclear Chemistry
Nuclear Chemistry. Radioactivity  Nuclear Reactions – reactions in which the nuclei of unstable isotopes (radioisotopes) gain stability by undergoing.
Unstable Nuclei and Radioactive Decay. Radioactivity (Radioactive decay) The process by which some substances spontaneously emit radiation. Radioactive.
1) How is the mass number calculated (2).
Scattering Reactions Scattering reactions - the incident particle collides with the target nucleus Elastic scattering – a collision between a particle.
Nuclear Radiation.
E = mc2 If you can’t explain it simply, you haven’t learned it well enough. Einstein.
Outside the nucleus, the beta decay {image} will not occur because the neutron and electron have more total mass than the proton. This process can occur.
St. 9- Nuclear Chemistry 1st, let’s review the parts of the Atom:
Nuclear Energy Chapter 25 6/1/2019.
Presentation transcript:

Radiation Protection III NUCP 2331 Neutrons Radiation Protection III NUCP 2331

Neutrons No charge Very penetrating ~1 AMU -similar to proton Stable in the nucleus Free neutron T ½= about 12 min Interacts by collision Losses energy in multiple interactions High H content material is good shielding

Neutron Energies The energies of neutrons are important in how they react Neutrons that have too much energy will not interact with the atom Capture cross section of the atom is dependant on the energies of the neutron U-235 will not interact with a fast neutron, needs to be low energy

Golf Analogy Consider the uranium is a hole on a golf course and the neutron a golf ball on the putting green. If the ball is hit too hard, even if it hits the hole near perfectly, it will likely hit the rim and be rejected. Animation 1 click Ball does not fall in hole

Golf Analogy If the ball is moving slowly enough, it is more likely to fall in the hole. Animation 1 click Ball falls in hole

Neutron Energies Cold- 0-.025 eV Thermal .025 ev Epithermal .025-.4 eV Cd .4-.6 ev EpiCd .6-1 eV Slow 1-10 eV Intermediate 10ev -1MeV Fast 1-20 MeV Relativistic > 20 Mev

Neutron Production Only very heavy radionulcides emit neutrons as part of their normal decay Cf-252, Cm-254 Need to be created in a accelerator or a neutron generator Sources have to be a two part source Heavy alpha emitter Low Z metal Am-Be, Pu-Li, Pu-Be, Ra-Be

Neutron Production Heavy atom produces an alpha particle as part of its natural decay process The alpha particle interacts with the low Z metal This initiates and (alpha, n) reaction in the metal Neutron production is based on activity of the alpha emitter

Neutron Source Each source combo generates and number of neutrons /sec and of a certain energy Pu-Be 2.3 E 6 n/sec/Ci Am-Be 2.2 E 6 n/sec/Ci Compare this with Cf-252 4.3 E 9 n/sec/Ci

Neutron Interactions (Indirectly Ionizing Radiation) Inelastic and Elastic Collisions Nuclear Capture

Cross section Neutrons have to come in close proximity to another particle/nucleus in order to interact The area that the particle/nucleus can interact with the neutron is called the capture cross section of that particle/nucleus The cross section of interaction is expressed as barns 1 barn = 10-24 cm2

Cross Sections Capture cross section-probability of nuclear reaction with neutron Total cross section takes into account all reactions(scatter, capture, absorption, fission, etc) Can have specify cross sections for each interaction Probability determined by energy

Cross section Macroscopic cross section- ratio between neutron flux and reaction rate, property of the material reactions per volume Microscopic cross section- probability of interaction with individual atom property of the nucleus probability per area

Elastic Scattering This interaction is similar to the bouncing of a ball on the floor The amount of energy transferred to the other object depends on the size difference in the objects Neutron hitting a large nucleus will not loose too much energy Neutron hitting an object of similar size may transfer most or all energy to other object

Ping Pong Ball Analogy Consider the neutron as a fast ping pong ball. If the ping pong ball hits a larger more massive bowling ball, the bowling ball won’t budge and the ping pong ball will scatter off of it at roughly the same speed. Animation - 1 click Ping pong ball strikes bowling ball and bounces

Moderators If the ping pong ball hits another slower moving or stationary ping pong ball of the same size, both balls will scatter off at roughly ½ the speed of the initial ping pong ball. Materials used to slow down neutrons are called moderators. Animation - 1 click Ping pong ball strikes other ball and both bounce off

Elestic scatter of neutrons is similar to the way billiard balls bounce off of each other. how energy each neutron has and the angles involved determines how much energy is transferred to the other body, protons.

Ineleastic scattering Inelastic interactions are where one of the colliding particles is composed of smaller units The neutron will interact with the other nucleus and transfer energy and the other atom will become energized The atom will then emit and photon or other particle to return to a ground state

Nuclear capture Neutrons loose energy by elastic scattering through matter When the neutron losses enough energy it will interact differently with atoms If the neutron is the right energy it will be absorbed into the atom This will add a neutron to the atomic mass and possibly making the atom unstable

In this case the neutron is slowed down by an elastic scatter and absorbed into a nucleus byt a inelastic scastter

Neutrons that have the right energy can be absorbed into the nucleus of an atom, this will upset the ratio between neutrons and protons and therefore possibly make the atom unstable and hence radioactive. Neutron radiation is the only type of radiation that can make other non radioactive material radioactive.

Neutron Activation The process of a material becoming radioactive after being subjected to a field of neutrons Material such as magnets in accelerators get highly radioactive Material can be put in neutron field for elemental analysis Can be used in forensics

Activation N=Aφσt N= number of radioactive atoms produced in the reaction A= number of atoms in the sample φ = neutron flux of the system σ = capture cross section of the atom T= time in the neutron field Formula get s complicated if one need to take into account decay while activation and counting

N-capture induced Fission Xenon-144 10n 10n 10n Neutron Fission is a process in which very heavy atoms, such as uranium and plutonium, after “absorbing” a neutron becomes so unstable that they literally split into two pieces accompanied by a large release of energy. The energy released per fission is approximately 200 megaelectronvolts, equivalent to about 3.2x10-11 J of energy, (a very small number). However this energy release is over two million times larger than that given up in most chemical reactions, for example in the burning of coal. If 1 gm of uranium-235 were to completely fission, it would require burning approximately 4900 pounds of coal to result in an equivalent energy release. To generate 1 J of energy 3.1x1010 fissions must occur. Most modern reactors operate at about 3800 megawatts of power which is 3,800,000,000 joules per second. To create this power level, 1.18x1020 fissions must occur in the reactor each second. Uranium-235 Plutonium-239 Strontium-90

Demonstration The neutron passes through water, slowing down and transferring its energy to the water molecules. Animation – 2 clicks Zoom out on neutron Neutron moves thru water and hits uranium The slow (thermalized) neutron is absorbed by a U-235 atom. We begin with a fast neutron

Demonstration The uranium becomes highly excited and begins to deform. Eventually, the nucleus splits into two fission products and releases 2 or 3 neutrons Fission Product Neutron Neutron Animation – 1 click Uranium gets excited and fissions Neutron Fission Product

Fission & Chain Reactions Neutron A chain reaction is the process where neutrons produced from fission go on to cause fissions in surrounding uranium atoms. Some of the neutrons produced will escape from the reactor core, while others will interact with other core materials other than fuel. These neutrons are “lost” and reduce the chain reaction process. If the number of fissions in the first generation equal the number of fissions in a second generation, the chain reaction is said to be “critical”. If the number of fissions is increasing between generations, the reaction is said to be supercritical, and the power level of the reactor will increase exponentially. If the number of fissions in decreasing between generations, the reaction is “subcritical” and the power will drop away dramatically. A nuclear reactor is operated so it is “critical” at some established power level, usually about 3800 megawatts thermal. To increase power the reactor is temporarily made supercritical, while to decrease power the reactor is made temporarily subcritical. Uranium-235 Plutonium-239

Neutron in reactor The amount of electricity that is produced is proportional to the amount of heat generated The amount of heat generated is proportional to the number of fissions taking place The number of fissions taking place is proportional to the free neutron population the change in the number of neutrons is related to the reactivity of the reactor

Reactivity Reactivity is defined as a reactor’s departure from criticality. It is a quantitative measure of the rate of change of fission neutron population. We can not detect the number of fissions occurring, but we can detect neutrons from fission to determine if they are increasing or decreasing in population. Mathematically, reactivity is described as the fractional change in neutron population.

Explanation Reactivity can be positive, negative or zero. A reactor with zero reactivity is critical by definition. A reactor with positive reactivity is supercritical. A reactor with negative reactivity is subcritical.

Neutrons In the fission process there can be two different types of neutrons Prompt Neutrons that are immediately released from the fission process Delayed Neutrons that are emitted from a high energy beta decay from one of the fission fragments Can be up to several minutes later Needs to be taken into account when calculating reactivity

Neutrons Flux- the number of neutrons passing through a space in a given time, Neutrons per area per time (n/cm2/sec) Fluence- number of neutrons passing through an area neutrons per area (n/cm2)

Neutron flux-density How many neutrons are passing through a square cm per second. in order to do this we need two pieces of info How many neutrons are being emitted by the source How far away from the source are we

Neutron flux-density Total number of neutrons divided by total surface area that is at certain distance from the source. Number of neutrons/4πr2 10 Ci-Pu-Be source generates 2.3 E 6 n/sec/Ci You are at 5 feet from source Neutron flux –density= ????

Neutron dose We need the neutron flux in order to determine the dose generated by those neutrons Dose from the neutrons is based on the energy of the neutrons Compare the flux-density of the neutrons to the number needed to generate 1 Rem

Neutron dose 0.5 MeV neutrons Flux density is 1.5 E 8 n/cm2 What is the dose?

Questions?