Nuclear Reactors, BAU, First Semester, 2007-2008 (Saed Dababneh). 1 Nuclear Physics at BAU This course

Slides:



Advertisements
Similar presentations
I0 I Probability Neutron Attenuation (revisited) X Recall t = N t
Advertisements

Nuclear Reactor Theory, JU, Second Semester, (Saed Dababneh). 1 Course web or
Nuclear Reactor Theory, JU, First Semester, (Saed Dababneh). 1 1/ v 235 U thermal cross sections fission 584 b. scattering 9 b. radiative capture.
Neutron-induced Reactions
Nuclear Reactors, BAU, 1st Semester, (Saed Dababneh). 1 Review Test Consider thermal neutrons in natural uranium (19.04 g.cm -3 ), a)What is.
Nuclear Reactors, BAU, 1st Semester, (Saed Dababneh). 1 HW 14 More on Moderators Calculate the moderating power and ratio for pure D 2 O as well.
1 Controlled Fission 235 U + n X + Y + (~ 2.4) n Moderation of second generation neutrons Chain reaction. Water, D 2 O or graphite moderator. Ratio of.
I0 I Probability Neutron Attenuation X Recall t = N t
Compound Nucleus Reactions
? Nuclear Reactions Categorization of Nuclear Reactions
Accelerator Physics, JU, First Semester, (Saed Dababneh).
Nuclear Reactor Theory, JU, First Semester, (Saed Dababneh).
Nuclear Reactor Theory, JU, Second Semester, (Saed Dababneh). 1 1/ v 235 U thermal cross sections fission 584 b. scattering 9 b. radiative capture.
Nuclear Size Quite old!!! Not exactly for Au!!!
Nuclear Binding Energy
Accelerator Physics, JU, First Semester, (Saed Dababneh). 1 Course web or
phenomenological course.
Nuclear Reactors, BAU, 1st Semester, (Saed Dababneh). 1 Steady State Diffusion Equation HW 20 Study example 5.3 and solve problem 5.8 in Lamarsh.
Energy Consumption Fossil Fuel Contribution to Global Energy Demand Year.
Interaction of radiation with matter - 5
What have we learned last time? Q value Binding energy Semiempirical binding energy formula Stability.
RFSS: Lecture 9 Nuclear Reactions
Direct Reactions. Optical model Represent the target nucleus by a potential -- Attenuation length.
Neutral Particles. Neutrons Neutrons are like neutral protons. –Mass is 1% larger –Interacts strongly Neutral charge complicates detection Neutron lifetime.

12C(p,g)13N g III. Nuclear Reaction Rates 12C 13N Nuclear reactions
Nuclear and Radiation Physics, BAU, 1 st Semester, (Saed Dababneh). 1 Nuclear Reactions Categorization of Nuclear Reactions According to: bombarding.
25 9. Direct reactions - for example direct capture: Direct transition from initial state |a+A> to final state B +  geometrical.
1 III. Nuclear Reaction Rates Nuclear reactions generate energy create new isotopes and elements Notation for stellar rates: p 12 C 13 N  12 C(p,  )
Nuclear and Radiation Physics, BAU, First Semester, (Saed Dababneh). 1 Nuclear Force Spin dependent  difference in neutron scattering cross.
Stopping Power The linear stopping power S for charged particles in a given absorber is simply defined as the differential energy loss for that particle.
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:
Radiation Protection III NUCP 2331
Nuclear and Radiation Physics, BAU, First Semester, (Saed Dababneh). 1 Nuclear Fission 1/ v 235 U thermal cross sections  fission  584 b. 
Nuclear and Radiation Physics, BAU, 1 st Semester, (Saed Dababneh). 1 Nuclear Binding Energy B tot (A,Z) = [ Zm H + Nm n - m(A,Z) ] c 2 B  m.
Nuclear and Radiation Physics, BAU, Second Semester, (Saed Dababneh) Nuclear and Radiation Physics Before we start, let us tackle.
Nuclear and Radiation Physics, BAU, First Semester, (Saed Dababneh). 1 Nuclear Reactions Sample.
1 PHYS 3313 – Section 001 Lecture #10 Monday, Feb. 17, 2014 Dr. Jaehoon Yu Photoelectric Effect Compton Effect Pair production/Pair annihilation Monday,
Nuclear Reactor Theory, JU, First Semester, (Saed Dababneh). 1 Course web or
A. Dokhane, PHYS487, KSU, 2008 Chapter1- Neutron Reactions 1 NEWS Lecture1: Chapter 0 is already on my Website.
PHYS-H406 – Nuclear Reactor Physics – Academic year CH.VII: NEUTRON SLOWING DOWN INTRODUCTION SLOWING DOWN VIA ELASTIC SCATTERING KINEMATICS.
Neutrons (Basic Concepts).  It is desirable to classify neutrons according to their kinetic energy into:
Artificial Radioactivity
Lecture 12: The neutron 14/10/ Particle Data Group entry: slightly heavier than the proton by 1.29 MeV (otherwise very similar) electrically.
1 Interaction Between Ionizing Radiation And Matter, Part 3 Neutrons Audun Sanderud Department of Physics University of Oslo.
Accelerator Physics, JU, First Semester, (Saed Dababneh). 1 Electron pick-up. ~1/E What about fission fragments????? Bragg curve stochastic energy.
Nuclear Reactors, BAU, 1st Semester, (Saed Dababneh). 1 Controlled Fission Note that  is greater than 2 at thermal energies and almost 3 at.
Chapter 5 Interactions of Ionizing Radiation. Ionization The process by which a neutral atom acquires a positive or a negative charge Directly ionizing.
Nuclear and Radiation Physics, BAU, 1 st Semester, (Saed Dababneh) Nuclear and Radiation Physics Why nuclear physics? Why radiation.
Nuclear Reactors, BAU, 1st Semester, (Saed Dababneh).
Nuclear and Radiation Physics, BAU, First Semester, (Saed Dababneh). 1 Extreme independent particle model!!! Does the core really remain inert?
NE Introduction to Nuclear Science Spring 2012 Classroom Session 4: Radioactive Decay Types Radioactive Decay and Growth Isotopes and Decay Diagrams.
Nuclear Reactors, BAU, 1st Semester, (Saed Dababneh). 1 Neutron Attenuation (revisited) Recall  t = N  t Probability per unit path length.
Collective model Vibrational States Average shape Instantaneous shape
1 Segrè Lost … ! Nuclear Fission How much is recoverable? How much is recoverable? What about capture gammas? (produced by -1 neutrons) What about capture.
Nuclear Reactors, BAU, 1st Semester, (Saed Dababneh).
Monday, Sept. 18, 2006PHYS 3446, Fall 2006 Jae Yu 1 PHYS 3446 – Lecture #5 Monday, Sept. 18, 2006 Dr. Jae Yu 1.Nuclear Phenomenology 2.Properties of Nuclei.
Nuclear and Radiation Physics, BAU, First Semester, (Saed Dababneh) Nuclear and Radiation Physics Before we start, let us tackle.
Nuclear and Radiation Physics, BAU, First Semester, (Saed Dababneh). 1.
Nuclear and Radiation Physics, BAU, 1 st Semester, (Saed Dababneh). 1 The Deuteron Deuterium (atom). The only bound state of two nucleons  simplest.
A. Dokhane, PHYS487, KSU, 2008 Chapter1- Neutron Reactions 1 NEWS Lecture1: Chapter 0 is already on my Website.
Nuclear and Radiation Physics, BAU, 1 st Semester, (Saed Dababneh). 1 Electromagnetic moments Electromagnetic interaction  information about.
PHYS-H406 – Nuclear Reactor Physics – Academic year CH.VII: NEUTRON SLOWING DOWN INTRODUCTION SLOWING DOWN VIA ELASTIC SCATTERING KINEMATICS.
Nuclear Reactors Nuclear Physics at BAU This course
Resonance Reactions HW 34 In the 19F(p,) reaction:
Nuclear Reactors, BAU, 1st Semester, (Saed Dababneh).
Chapter 4 Mechanisms and Models of Nuclear Reactions
Neutron Resonance Reactions
Presentation transcript:

Nuclear Reactors, BAU, First Semester, (Saed Dababneh). 1 Nuclear Physics at BAU This course Nuclear and Radiation Physics Advanced Statistical Mechanics Nuclear Reactors

Nuclear Reactors, BAU, 1 st Semester, (Saed Dababneh). 2 Review of relevant studied material in nuclear physics. Concepts in neutron physics. The relevant physics related to nuclear technology:  Fission chain reaction.  Neutron diffusion and moderation.  Heat removal from nuclear reactors.  Isotope separation.  … Components of nuclear reactors. Nuclear reactor fuels and fuel cycles. Nuclear reactor theory. Basic concepts of radiation protection and nuclear safety, shielding and waste disposal. Issues and prospects of nuclear power today and in the future. General subjects to be covered

Nuclear Reactors, BAU, 1 st Semester, (Saed Dababneh). 3 Grading Review Test05% Mid-term Exam20% Projects, quizzes and HWs25% Final Exam50% Homeworks are due after one week unless otherwise announced. Remarks or questions marked in red without being announced as homeworks should be also seriously considered! Some tasks can (or should) be sent by

Nuclear Reactors, BAU, 1 st Semester, (Saed Dababneh). 4 Review Test Review relevant material in 742. Read Lamarsh Chs 1, 2 and 3. Will do the test afterwards.

Nuclear Reactors, BAU, 1 st Semester, (Saed Dababneh). 5 Projects  Consider nuclear fuel cycles with emphasis on front ends. Work as a team. Divide and organize the job among you. Try to explore local applicability. Due date (for written version) : December 5 th. Presentation: Will be scheduled later.  Other small projects will be announced in class.

Nuclear Reactors, BAU, 1 st Semester, (Saed Dababneh). 6 Nuclear Reaction Energetics (revisited) Conservation Laws Charge, Baryon number, total energy, linear momentum, angular momentum, parity, (isospin??) …….   a papa X pYpY pbpb Y b +ve Q-value  exoergic reaction. -ve Q-value  endoergic reaction. +ve Q-value  reaction possible if T a  0. -ve Q-value  reaction not possible if T a  0. (Is T a > |Q| sufficient?). Conservation of momentum ……

Nuclear Reactors, BAU, 1 st Semester, (Saed Dababneh). 7 Conservation of momentum. We usually do not detect Y. Show that: The threshold energy (for T a ): (the condition occurs for  = 0º). +ve Q-value  reaction possible if T a  0. Coulomb barriers…….!!! -ve Q-value  reaction possible if T a > T Th. HW 1 Nuclear Reaction Energetics (revisited)

Nuclear Reactors, BAU, 1 st Semester, (Saed Dababneh). 8 Nuclear Reaction Energetics (revisited) The double valued situation occurs between T Th and the upper limit T a \. Double-valued in a forward cone. HW 1 (continued) elastic inelastic scattering neutrons Discuss the elastic and inelastic scattering of neutrons using these relations.

Nuclear Reactors, BAU, 1 st Semester, (Saed Dababneh). 9 Nuclear Reaction Energetics (revisited)

Nuclear Reactors, BAU, 1 st Semester, (Saed Dababneh). 10 Nuclear Reaction Energetics (revisited) What about neutron induced reactions?

Nuclear Reactors, BAU, 1 st Semester, (Saed Dababneh). 11 Nuclear Reaction Energetics (revisited) What about neutron induced reactions?

Nuclear Reactors, BAU, 1 st Semester, (Saed Dababneh). 12 Nuclear Reaction Energetics (revisited) What about neutron induced reactions?

Nuclear Reactors, BAU, 1 st Semester, (Saed Dababneh). 13 Nuclear Reaction Energetics (revisited) If the reaction reaches excited states of Y 58 Ni( ,p) 61 Cu Highest proton energy less proton energy even less …. See Figures 11.4 in Krane What about neutron induced reactions?

Nuclear Reactors, BAU, 1 st Semester, (Saed Dababneh). 14 Neutron Interactions (revisited) Chadwick’s discovery. Neutrons interact with nuclei, not with atoms. (Exceptions). Recall from Nuclear Physics 742: o Inelastic scattering ( n,n \ ). Q = -E*  Inelastic gammas. Threshold? o Elastic scattering ( n,n ). Q = ?? (Potential and CN). Neutron moderation? o Radiative capture ( n,  ). Q = ??  Capture gammas. o ( n,  ), ( n,p ). Q = ?? Absorption Reactions. o ( n,2n ), ( n,3n ) Q = ?? Energetic neutrons on heavy water can easily eject the loosely bound neutron. o Fission. (n,f). HW 2 HW 2 Examples of such exo- and endo-thermic reactions with Q calculations.

Nuclear Reactors, BAU, 1 st Semester, (Saed Dababneh). 15 Elastic or inelastic. Analogous to diffraction. Alternating maxima and minima. First maximum at Minimum not at zero (sharp edge of the nucleus??) Clear for neutrons. Protons? High energy, large angles. Why? Inelastic  Excited states, energy, X-section and spin-parity. Neutron Scattering (revisited)

Nuclear Reactors, BAU, 1 st Semester, (Saed Dababneh). 16 Probability. Projectile a will more probably hit target X if area is larger. Classically:  =  (R a + R X ) 2. Classical  = ??? (in b) n + 1 H, n U, 238 U U Quantum mechanically:  =   2. Coulomb and centrifugal barriers  energy dependence of . What about neutrons? Nature of force: Strong: 15 N(p,  ) 12 C  ~ 0.5 b at E p = 2 MeV. Electromagnetic: 3 He( ,  ) 7 Be  ~ b at E  = 2 MeV. Weak: p(p,e + )D  ~ b at E p = 2 MeV. Experimental challenges to measure low X-sections.. Reaction Cross Section (revisited)

Nuclear Reactors, BAU, 1 st Semester, (Saed Dababneh). 17 Reaction Cross Section (Simple terms) X A (Area of the beam!!) Monoenergetic neutrons of speed v (cm.s -1 ) and density n (cm -3 ) Target with N atoms.cm -3 or NAX atoms. Position of a neutron 1 s before arriving at target |v| Volume = vA containing nvA neutrons that hit the “whole” target in 1 s. Beam Intensity I  nvA/A = nv (cm -2 s -1 ) Number of neutrons interacting with target per second  I, A, X and N =  t I N A X

Nuclear Reactors, BAU, 1 st Semester, (Saed Dababneh). 18 Reaction Cross Section (Simple terms) Number of neutrons interacting with target per second =  t I N A X Number of interactions with a single nucleus per second =  t I Interpretation and units of . nvA = IA neutrons strike the target per second, of these  t I neutrons interact with any single nucleus. Thus, measures the probability for a neutron to hit a nucleus. Total cross section Total number of nuclei in the target Effective cross-sectional area of the nucleus. Study examples in Lamarsh

Nuclear Reactors, BAU, 1 st Semester, (Saed Dababneh). 19 Reaction Cross Section (Simple terms) Number of neutrons interacting with target per second =  t I N A X Number of interactions per cm 3 per second (Collision Density) F t =  t I N = I  t  t = N  t Total cross section Volume of the target Macroscopic total cross section. Probability per unit path length. Mean free path Study examples in Lamarsh

Nuclear Reactors, BAU, 1 st Semester, (Saed Dababneh). 20 Reaction Cross Section (Simple terms) Homogeneous Mixture Molecule x m y n N x =mN, N y =nN given that events at x and y are independent. Study examples in Lamarsh

Nuclear Reactors, BAU, 1 st Semester, (Saed Dababneh). 21 Reaction Cross Section (revisited) dd ,, IaIa Detector for particle “b” “X“ target Nuclei / cm 2 “a” particles / s “b” particles / s cm 2 Typical nucleus (R=6 fm): geometrical  R 2  1 b. Typical  : 10 6 b.

Nuclear Reactors, BAU, 1 st Semester, (Saed Dababneh). 22 Reaction Cross Section (revisited) Many different quantities are called “cross section”. Krane Table 11.1 Angular distribution “Differential” cross section  ( ,  ) or  (  ) or “cross section” …!! Units … ! Doubly differential Energy state in “Y”  t for all “b” particles.

Nuclear Reactors, BAU, 1 st Semester, (Saed Dababneh). 23

Nuclear Reactors, BAU, 1 st Semester, (Saed Dababneh). 24n-TOFCERN

Nuclear Reactors, BAU, 1 st Semester, (Saed Dababneh). 25

Nuclear Reactors, BAU, 1 st Semester, (Saed Dababneh). 26 1/ v 235 U thermal cross sections  fission  584 b.  scattering  9 b.  radiative capture  97 b. Fast neutrons should be moderated. Fission Barriers Different Features (revisited)

Nuclear Reactors, BAU, 1 st Semester, (Saed Dababneh). 27 Neutron Induced Reactions (revisited) X ( n,b ) Y n(En)n(En) b(Q+En)b(Q+En) For thermal neutrons Q >> E n  b ( Q )  constant Probability to penetrate the potential barrier P o ( E thermal ) = 1 P > o ( E thermal ) = 0 Non-resonant

Nuclear Reactors, BAU, 1 st Semester, (Saed Dababneh). 28 Neutron Induced Reactions (revisited)

Nuclear Reactors, BAU, 1 st Semester, (Saed Dababneh). 29 HW 3  Statistical Factor (revisited)

Nuclear Reactors, BAU, 1 st Semester, (Saed Dababneh). 30 Resonance Reactions (revisited) Entrance Channel a + X Exit Channel b + Y Compound Nucleus C* Excited State ExEx JJ a + X  Y + bQ > 0 b + Y  X + aQ < 0 Inverse Reaction QM Statistical Factor (  ) Identical particles Nature of force(s). Time-reversal invariance. HW 4

Nuclear Reactors, BAU, 1 st Semester, (Saed Dababneh). 31 Projectile Target Q-value Projectile Q-value Target Direct Capture (all energies) Resonant Capture (selected energies with large X-section) E  = E + Q - E ex Q + E R = E r Resonance Reactions (revisited)

Nuclear Reactors, BAU, 1 st Semester, (Saed Dababneh). 32

Nuclear Reactors, BAU, 1 st Semester, (Saed Dababneh). 33 Resonance Reactions (revisited) Damped Oscillator eigenfrequency Damping factor Oscillator strength

Nuclear Reactors, BAU, 1 st Semester, (Saed Dababneh). 34 Resonance Reactions (revisited) Breit-Wigner formula All quantities in CM system Only for isolated resonances. Reaction Elastic scattering HW 5 HW 5 When does  R take its maximum value? Usually  a >>  b.

Nuclear Reactors, BAU, 1 st Semester, (Saed Dababneh). 35 Resonance Reactions (revisited) J a + J X + l = J (-1) l  (J a )  (J X ) =  (J) (-1) l =  (J) Natural parity. Exit Channel b + Y Compound Nucleus C* Excited State ExEx JJ Entrance Channel a + X

Nuclear Reactors, BAU, 1 st Semester, (Saed Dababneh). 36 Resonance Reactions (revisited) Cross section ECEC    a     Energy What is the “Resonance Strength” …? What is its significance? In what units is it measured? Charged particle radiative capture ( a,  ) (What about neutrons?)

Nuclear Reactors, BAU, 1 st Semester, (Saed Dababneh). 37 Neutron Resonance Reactions (revisited)

Nuclear Reactors, BAU, 1 st Semester, (Saed Dababneh). 38 Neutron Activation Analysis (revisited) ( Z,A ) + n  ( Z, A+1 ) -- ( Z+1, A+1 )  (  -delayed  -ray) ! Project 1