Basic Concepts of Nuclear Physics Part II By Benjamin Thayer PHY3091.

Slides:



Advertisements
Similar presentations
Nuclear Chemistry A Short Study.
Advertisements

Nuclear Fission and Fusion
20th Century Discoveries
7: Atomic and Nuclear Physics 7.3 Nuclear reactions, fission and fusion.
NUCLEAR FUSION & NUCLEAR FISSION Noadswood Science, 2012.
Nuclear Energy Nuclear Reactions Nuclear Fission / Nuclear Fusion Harnessing the Power of the Nucleus.
Chapter 25 Nuclear Chemistry 25.3 Fission and Fusion
Investigation IV: Subatomic World
Nuclear Physics Notes CP Physics Ms. Morrison.
Nuclear Chemistry Fusion and Fission
Transmutation (Objective 25
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.
PA 1140 Waves and Quanta Unit 4: Atoms and Nuclei l Lecture course slides can be seen at:
Nuclear / Subatomic Physics Physics – Chapter 25 (Holt)
Nuclear Physics Selected Topics 5 –Fission and Fusion.
1 Chapter 9 Nuclear Radiation 9.6 Nuclear Fission and Fusion Copyright © 2005 by Pearson Education, Inc. Publishing as Benjamin Cummings.
Nuclear Fission and Fusion
Nuclear Fission & Fusion. History: Hahn & Strassman (1939) Bombarded Uranium-235 samples with neutrons expecting the Uranium-235 to capture neutrons Instead,
Lesson 2: It’s Greek to Me
Section 7.3. The process in which the nucleus changes gains or releases particles and energy The stronger the bond the more energy associated with it.
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.
Unit 8 Section 2: Nuclear Reactions
Nuclear Fundamentals Part I Unleashing the Power of the Atom.
Ahmad Saeedi Graduate Student Department of Physics, Western Illinois University, Macomb, IL Nuclear reaction Fission and Fusion.
Alpha, Beta, and Gamma Decay
AP Physics B Montwood High School R. Casao
1 Chapter 9 Nuclear Radiation 9.6 Nuclear Fission and Fusion Copyright © 2009 by Pearson Education, Inc.
Nuclear Fusion D-T Fusion Reactions. Nuclear fusion Nuclear fusion occurs when two light nuclei merge to form a heavier nucleus. The binding energy curve.
Section 24-3 Nuclear Fission Stability of elements is best around a mass number of 60. Atoms with a mass number greater than 60 tend to gain stability.
Nuclear Chemistry.
Atomic Stability. Isotopes Isotopes are atoms of an element that have different numbers of neutrons in their nucleus. Cu Copper – 63 OR Copper.
Nuclear Power Reactors SEMINAR ON NUCLEAR POWER REACTOR.
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.
Fission Lise Meitner- Austrian physicist during time of WWII. Discovered that bombardment of uranium with neutrons can split the nucleus into two pieces.
Summative Assessment Review! Ms. Barlow’s HS PS Class.
Nuclear Radiation > Nuclear Radiation & Transformations.
Atoms Chapter 4.
Protons and neutrons are called nucleons. An atom is referred to as a nuclide. An atom is identified by the number of protons and neutrons in its nucleus.
Nuclear Fission is the process by which the nucleus of an atom splits into two or more nuclei and some by- products.
Physics 12 Mr. Jean January 18 th, The plan: Video clip of the day Chapter 18 & 19 – MC.
Nuclear Fission and Fusion Unit 8 – Part B. Nuclear Balance Delicate balance between attractive strong nuclear forces and repulsive electric forces. In.
Nuclear Energy Nuclear Structure and Radioactivity.
Nuclear Chemistry. Nuclear Chemistry looks at the number of protons and neutrons in an atom Radioactive Decay = Spontaneous disintegration of a nucleus.
Basic Chemistry Copyright © 2011 Pearson Education, Inc. 1 Chapter 16 Nuclear Radiation 16.6 Nuclear Fission and Fusion.
In your own words try to explain a radio active decay series
“Standard Model” of particles in the universe
Nuclear Fission And Nuclear Fusion
Chapter 21 Nuclear Chemistry. © 2009, Prentice-Hall, Inc. The Nucleus Remember that the nucleus is comprised of the two nucleons, protons and neutrons.
Ch. 28 Nuclear Chemistry C. Smith. I. Nuclear Radiation A. Radioactivity 1. Radioisotopes are unstable isotopes that have unstable nuclei. 2. They gain.
Nuclear Chemistry III. Fission & Fusion (Nuclear reactions that are NOT radioactive decay.) III. Fission & Fusion (Nuclear reactions that are NOT radioactive.
AQA A2 Physics A Nuclear Physics Section 15 Fission.
11 ELECTROMAGNETIC RADIATION. 22 EM RADIATION II ALSO CALLED RADIANT ENERGY ONLY A PORTION IS CALLED LIGHT TRAVELS IN WAVES TRAVELS THROUGH SPACE (VACUUM)
Fission and Fusion are both nuclear reactions that involve the particles in the nucleus of an atom.
Fission, the splitting of nuclei, and fusion, the combining of nuclei, release tremendous amounts of energy. Section 3: Nuclear Reactions K What I Know.
CLICK HERE TO BEGIN! Directions: Click the term that correctly matches the definition in each question.
Nuclear Physics An Introduction. What does it mean when something is “Radioactive”? Atomic nuclei that emit particles and energy are said to be radioactive.
Nuclear Chemistry. Radioactivity  Radioisotopes – isotopes that are unstable, who’s nucleus undergoes changes to gain stability  Radiation – the penetration.
Chapter 9.2 Nuclear Radiation.
Chapter 9 Nuclear Radiation
A. Nuclear Forces Do nuclei contain attractive or repulsive forces?
Nuclear Fission and Fusion
Fission and Fusion of Atomic Nuclei
Harnessing the Power of the Sun
Chemistry 25.3.
Harnessing the Power of the Sun
Unit 4 – Nuclear Reactions
Chemistry 25.3.
Chemistry 25.3.
Nuclear Energy Nuclear Structure and Radioactivity.
Presentation transcript:

Basic Concepts of Nuclear Physics Part II By Benjamin Thayer PHY3091

Topics Interactions involving neutrons Interactions involving neutrons Nuclear Fission Nuclear Fission Nuclear Reactors Nuclear Reactors Nuclear Fusion Nuclear Fusion

Interactions Involving Neutrons As neutrons are electrically neutral, they do not interact electrically with electrons As neutrons are electrically neutral, they do not interact electrically with electrons Rate of neutron induced reactions increase as the neutron KE increases Rate of neutron induced reactions increase as the neutron KE increases When a neutron is absorbed by atomic nuclei of matter - decays by nuclear forces When a neutron is absorbed by atomic nuclei of matter - decays by nuclear forces

Interactions involving Neutrons Neutron Capture Neutron Capture If a fast neutron (energy> 1MeV) travels through matter – collides with other nuclei If a fast neutron (energy> 1MeV) travels through matter – collides with other nuclei Loses KE with each collision Loses KE with each collision If this KE becomes low – neutron is absorbed by a nucleus If this KE becomes low – neutron is absorbed by a nucleus The nucleus becomes unstable (for a very short time) and emits gamma radiation to stabilize The nucleus becomes unstable (for a very short time) and emits gamma radiation to stabilize

Interactions Involving Neutrons Neutron Capture Neutron Capture The product nucleus is radioactive The product nucleus is radioactive Decays by beta emission Decays by beta emission Rate of capture depends on: Rate of capture depends on: Type of atoms in the target matter Type of atoms in the target matter Energy of the incident neutrons Energy of the incident neutrons

Moderators Materials in which the elastic collision between the atoms and neutrons dominate Materials in which the elastic collision between the atoms and neutrons dominate They slow down the neutrons effectively They slow down the neutrons effectively As the rate of capture increases with decrease in the neutron energy, the material should have low capture tendency As the rate of capture increases with decrease in the neutron energy, the material should have low capture tendency Moderator nuclei should have low mass Moderator nuclei should have low mass ……which have abundance of hydrogen (paraffin & water are 2 examples) ……which have abundance of hydrogen (paraffin & water are 2 examples)

Moderators Fermi discovered that when some elements were bombarded by neutrons, new radioactive elements were produced. Fermi discovered that when some elements were bombarded by neutrons, new radioactive elements were produced. He predicted that neutron would be a good projectile. As it is uncharged, it would not experience Coulomb’s force while approaching the nucleus He predicted that neutron would be a good projectile. As it is uncharged, it would not experience Coulomb’s force while approaching the nucleus Neutrons become thermal neutrons Neutrons become thermal neutrons They are in thermal equilibrium with the moderator material They are in thermal equilibrium with the moderator material As the RMS speed of the thermal neutrons is 2800 m/s, they have a high probability of being captured As the RMS speed of the thermal neutrons is 2800 m/s, they have a high probability of being captured Compare that speed with the speed of the incident neutron whose kinetic energy is of the order of several MeV Compare that speed with the speed of the incident neutron whose kinetic energy is of the order of several MeV The process is called thermalistation The process is called thermalistation

Nuclear Fission

When a U-235 nucleus absorbs a thermal neutron, it produces a compound nucleus of U- 236 When a U-235 nucleus absorbs a thermal neutron, it produces a compound nucleus of U- 236 This nucleus undergoes fission, splitting into two fragments This nucleus undergoes fission, splitting into two fragments

Nuclear Fission

Nuclear Fission ( Chain Reaction ) If an least one neutron from U-235 fission strikes another nucleus and causes it to fission, then the chain reaction will continue If the reaction will sustain itself, it is said to be "critical", and the mass of U-235 required to produced the critical condition is said to be a "critical mass” A fission chain reaction produces intermediate mass fragments which are highly radioactive and produce further energy by their radioactive decay

Nuclear Fission ( Chain Reaction ) Some of them produce neutrons, called delayed neutrons, which contribute to the fission chain reaction. The probability for fission with slow neutrons is greater If the neutrons from fission are moderated to lower their speed, a critical chain reaction can be achieved at low concentrations of U-235

Nuclear Reactors

Reproduction Constant K: Average number of neutrons from each fission event that causes another fission event For normal fission reaction, K = 2.5 Less because of several factors K = 1 gives a self-sustained chain reaction – reactor is called critical K < 1, the reactor is sub critical – reaction dies out K>1, the reactor is supercritical and a un-stoppable reaction occurs

Nuclear Reactors

Current uses of nuclear energy must rely on nuclear fission, a less-than- ideal energy source, since nuclear fusion has yet to be harnessed for electricity generation. The heat from the nuclear fission is used to: Current uses of nuclear energy must rely on nuclear fission, a less-than- ideal energy source, since nuclear fusion has yet to be harnessed for electricity generation. The heat from the nuclear fission is used to: This usually done in a Boiling Water Reactor (BWR) or a Pressurized Water Reactor (PWR), but there are other options such as the fast breeder reactor This usually done in a Boiling Water Reactor (BWR) or a Pressurized Water Reactor (PWR), but there are other options such as the fast breeder reactor

Nuclear Fusion Opposite of nuclear fission Opposite of nuclear fission Energy will be released if two lighter nuclei combine to form a larger nucleus, a process is called nuclear fusion Energy will be released if two lighter nuclei combine to form a larger nucleus, a process is called nuclear fusion This process is hindered by Coulomb repulsive forces This process is hindered by Coulomb repulsive forces The Coulomb barrier is broken by raising the temperature of the material until the particles have enough energy (Sun…) The Coulomb barrier is broken by raising the temperature of the material until the particles have enough energy (Sun…)