Nuclear and Radiation Physics, BAU, First Semester, 2007-2008 (Saed Dababneh). 1 Extreme independent particle model!!! Does the core really remain inert?

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
Neutron-induced Reactions
Nuclear Magnetic Moment
? Nuclear Reactions Categorization of Nuclear Reactions
Accelerator Physics, JU, First Semester, (Saed Dababneh).
Nuclear Size Quite old!!! Not exactly for Au!!!
Neutron Excess Asymmetry Remember HWc 1.
Nuclear Binding Energy
Basic Nuclear Properties
Isomer Spectroscopy in Near-Spherical Nuclei Lecture at the ‘School cum Workshop on Yrast and Near-Yrast Spectroscopy’ IIT Roorkee, October 2009 Paddy.
How do nuclei rotate? 5. Appearance of bands. Deformed mean field solutions This is clearly the case for a well deformed nucleus. Deformed nuclei show.
The Collective Model Aard Keimpema.
(taken from H-J. Wolesheima,
Monday, Feb. 14, 2005PHYS 3446, Spring 2005 Jae Yu 1 PHYS 3446 – Lecture #8 Monday, Feb. 14, 2005 Dr. Jae Yu 1.Nuclear Models Shell Model Predictions Collective.
Course Title: Nuclear Physics Course Code: EEE-202
Nuclear models. Models we will consider… Independent particle shell model Look at data that motivates the model Construct a model Make and test predictions.
Higher Order Multipole Transition Effects in the Coulomb Dissociation Reactions of Halo Nuclei Dr. Rajesh Kharab Department of Physics, Kurukshetra University,
Nuclear and Radiation Physics, BAU, 1 st Semester, (Saed Dababneh). 1 Nuclear Reactions Categorization of Nuclear Reactions According to: bombarding.
NUCLEAR STRUCTURE PHENOMENOLOGICAL MODELS
Nuclear and Radiation Physics, BAU, First Semester, (Saed Dababneh). 1 Nuclear Force Spin dependent  difference in neutron scattering cross.
Vibrational and Rotational Spectroscopy
The Shell Model of the Nucleus 5. Nuclear moments
Nuclei with more than one valence nucleon Multi-particle systems.
Radiation Detection and Measurement, JU, 1st Semester, (Saed Dababneh). 1 Radiation Sources Heavy nuclei are unstable against spontaneous emission.
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.
NSDD Workshop, Trieste, February 2006 Nuclear Structure (II) Collective models P. Van Isacker, GANIL, France.
NUCLEAR MODELS.
Lecture 24 Collective Excitations in nuclei Introduction: Over half the known nuclei have configurations (Z,N) even, J  = 0 + Recall that an empirical.
5. Exotic modes of nuclear rotation Tilted Axis Cranking -TAC.
Lecture 20: More on the deuteron 18/11/ Analysis so far: (N.B., see Krane, Chapter 4) Quantum numbers: (J , T) = (1 +, 0) favor a 3 S 1 configuration.
Nuclear and Radiation Physics, BAU, First Semester, (Saed Dababneh). 1 Nuclear Reactions Sample.
Collective Model. Nuclei Z N Character j Q obs. Q sp. Qobs/Qsp 17 O 8 9 doubly magic+1n 5/ K doubly magic -1p 3/
Shape phase transition in neutron-rich even-even light nuclei with Z=20-28 H.B.Bai X.W.Li H.F.Dong W.C.Cao Department of Physics, Chifeng University, Chifeng.
Experimental evidence for closed nuclear shells Neutron Proton Deviations from Bethe-Weizsäcker mass formula: mass number A B/A (MeV per nucleon)
Nuclear Reactor Theory, JU, First Semester, (Saed Dababneh). 1 Course web or
5-1 RDCH 702: Lecture 5 Nuclear Force, Structure and Models Readings: §Nuclear and Radiochemistry: Chapter 10 (Nuclear Models) §Modern Nuclear Chemistry:
Nuclear Models Nuclear force is not yet fully understood.
How do nuclei rotate? 1. The molecular picture.
10-1 Fission General Overview of Fission The Probability of Fission §The Liquid Drop Model §Shell Corrections §Spontaneous Fission §Spontaneously Fissioning.
Accelerator Physics, JU, First Semester, (Saed Dababneh). 1 Electron pick-up. ~1/E What about fission fragments????? Bragg curve stochastic energy.
How do nuclei rotate? The nucleus rotates as a whole.
Nuclear Reactors, BAU, First Semester, (Saed Dababneh). 1 Nuclear Physics at BAU This course
Nuclear and Radiation Physics, BAU, 1 st Semester, (Saed Dababneh) Nuclear and Radiation Physics Why nuclear physics? Why radiation.
Lecture 23: Applications of the Shell Model 27/11/ Generic pattern of single particle states solved in a Woods-Saxon (rounded square well)
Nuclear and Radiation Physics, BAU, 1 st Semester, (Saed Dababneh). 1 Shell model Notes: 1. The shell model is most useful when applied to closed-shell.
Nuclear Reactors, BAU, 1st Semester, (Saed Dababneh). 1 Neutron Attenuation (revisited) Recall  t = N  t Probability per unit path length.
Some (more) High(ish)-Spin Nuclear Structure Paddy Regan Department of Physics Univesity of Surrey Guildford, UK Lecture 2 Low-energy.
Collective model Vibrational States Average shape Instantaneous shape
The Semi-empirical Mass Formula
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.
Nuclear and Radiation Physics, BAU, 1 st Semester, (Saed Dababneh). 1 Electromagnetic moments Electromagnetic interaction  information about.
Nuclear Physics, JU, Second Semester,
Monday, Oct. 2, 2006PHYS 3446, Fall 2006 Jae Yu 1 PHYS 3446 – Lecture #8 Monday, Oct. 2, 2006 Dr. Jae Yu 1.Nuclear Models Shell Model Collective Model.
Congresso del Dipartimento di Fisica Highlights in Physics –14 October 2005, Dipartimento di Fisica, Università di Milano Contribution to nuclear.
Pairing Evidence for pairing, what is pairing, why pairing exists, consequences of pairing – pairing gap, quasi-particles, etc. For now, until we see what.
Rotational energy term in the empirical formula for the yrast energies in even-even nuclei Eunja Ha and S. W. Hong Department of Physics, Sungkyunkwan.
Nuclear Reactors Nuclear Physics at BAU This course
Determining Reduced Transition Probabilities for 152 ≤ A ≤ 248 Nuclei using Interacting Boson Approximation (IBA-1) Model By Dr. Sardool Singh Ghumman.
Nuclear Binding Energy
CHEM 312 Lecture 8: Nuclear Force, Structure and Models
PHL424: γ-decay γ-decay is an electromagnetic process where the nucleus decreases in excitation energy, but does not change proton or neutron numbers This.
Resonance Reactions HW 34 In the 19F(p,) reaction:
Nuclear Chemistry CHEM 396 Chapter 4, Part B Dr. Ahmad Hamaed
Nuclear Physics, JU, Second Semester,
Nuclear Size Depends on probe and relevant physics.
Neutron Resonance Reactions
How do nuclei rotate? 1. The molecular picture.
Presentation transcript:

Nuclear and Radiation Physics, BAU, First Semester, (Saed Dababneh). 1 Extreme independent particle model!!! Does the core really remain inert? Shell model 1d 5/2 2s 1/2 1d 3/2 1p 1/2 ? l  pairing 

Core Nuclear and Radiation Physics, BAU, First Semester, (Saed Dababneh). 2 Shell model Extreme independent particle model  only 23 rd neutron. More complete shell model  all three “valence” nucleons. 20

Nuclear and Radiation Physics, BAU, First Semester, (Saed Dababneh). 3 Shell model HW 26 and 43 Sc, 43 Ti. Discuss the energy levels of nuclei with odd number of nucleons in the 1f 7/2 shell.

Nuclear and Radiation Physics, BAU, First Semester, (Saed Dababneh). 4 Shell model Dipole Magnetic Moment HW 27 HW 27 Show that examine and examine Eqs. 5.9 in Krane. In addition, work out problem 5.8 in Krane  Conclusion? Proton: g s (free) = ?g l = 1 ? Neutron: g s (free) = ?g l = 0 ? What about  + and  - ?

Nuclear and Radiation Physics, BAU, First Semester, (Saed Dababneh). 5 Shell model Electric Quadrupole Moment Refined QM  for a uniformly charged sphere Number of protons in a subshell Extremes Single particle: n = 1  - ive Q Single hole: n = 2j  +ive Q Examine Table 5.1 and Fig.5.10 in Krane In the xy-plane: Q  -  r 2 .

Nuclear and Radiation Physics, BAU, First Semester, (Saed Dababneh). 6

7 Shell model Validity A < < A < 220 NuclideQ (b) 2 H (D) O Co Cu Cs Dy Lu Bi-0.37

Nuclear and Radiation Physics, BAU, First Semester, (Saed Dababneh). 8 Collective model Large quadrupole moments  nucleus as a collective body (Liquid drop model). Interactions between outer nucleons and closed shells cause permanent deformation. Single-particle state calculated in a non-spherical potential  complicated. Spacing between energy levels depends on size of distortion. Doubly magic  1 st excited state away from GS. Near closure  single-particle states. Further away from closure  collective motion of the core  excited states.

Nuclear and Radiation Physics, BAU, First Semester, (Saed Dababneh). 9 Collective model A net nuclear potential due to filled core shells exists. Collective model combines both liquid drop model and shell model. Two major types of collective motion:  Rotations: Rotation of a deformed shape.  Vibrations: Surface oscillations.

Nuclear and Radiation Physics, BAU, First Semester, (Saed Dababneh). 10 Collective model Rotational motion observed for non-spherical nuclei. Deformed nuclei are mainly Ellipsoid of surface: Difference between semimajor and semiminor axes. Deformation parameter. HW 28 Problems 5.11 and 5.12 in Krane. Discuss effect on quadrupole moment.  > 0  < 0 R av

Nuclear and Radiation Physics, BAU, First Semester, (Saed Dababneh). 11 Collective model Symmetry axis GS (even-even)  0 + Symmetry  only even I

Nuclear and Radiation Physics, BAU, First Semester, (Saed Dababneh). 12 Collective model HW 29 HW 29 compare measured energies of the states of the ground state rotational band to the calculations. Rigid body or liquid drop? Intermediate  Short range and saturation of nuclear force.

Nuclear and Radiation Physics, BAU, First Semester, (Saed Dababneh). 13 Collective model Spin parity E measured (keV) E/E(2 + )I(I + 1)/ Er Higher angular momentum  centrifugal stretching  higher moment of inertia  lower energy than expected  additional evidence for lack of rigidity. HW 29 (continued)

Nuclear and Radiation Physics, BAU, First Semester, (Saed Dababneh). 14 Collective model Odd-A

Nuclear and Radiation Physics, BAU, First Semester, (Saed Dababneh). 15 Collective model Average shape Instantaneous shape

Nuclear and Radiation Physics, BAU, First Semester, (Saed Dababneh). 16 Collective model Instantaneous coordinate Symmetry Amplitude Spherical harmonics r 0 A 1/3 = 0 monopole = 1 dipole = 2 quadrupole = 3 octupole.

Nuclear and Radiation Physics, BAU, First Semester, (Saed Dababneh). 17 Collective model Both monopole and dipole excitations require high energy. R(t) = R avr +  00 Y 00 = 0 monopole = 1 dipole

Nuclear and Radiation Physics, BAU, First Semester, (Saed Dababneh). 18 Collective model = 2 quadrupole Quantization of quadrupole vibration is called a quadrupole phonon. A phonon carries two units of angular momentum and even parity (-1 2 ). This mode is dominant. For most even-even nuclei, a low lying state with J π =2 + exists. Octupole phonon.

Nuclear and Radiation Physics, BAU, First Semester, (Saed Dababneh). 19 Collective model l = 4  = +4, +3, +2, +1, 0, -1, -2, -3, -4 l = 2  = +2, +1, 0, -1, -2 l = 0  = 0 Triplet 0 +, 2 +, 4 +

Nuclear and Radiation Physics, BAU, First Semester, (Saed Dababneh). 20 Collective model Two-phonon triplet at twice the energy of the single phonon state. HW 30 Krane 5.10

Nuclear and Radiation Physics, BAU, First Semester, (Saed Dababneh). 21 Nuclear Reactions X(a,b)Y First in 1919 by Rutherford: 4 He + 14 N  17 O + 1 H 14 N( ,p) 17 O Incident particle may: change direction, lose energy, completely be absorbed by the target…… Target may: transmute, recoil…… b =   Capture reaction. If B.E. permits  fission (comparable masses). Different exit channels a + X  Y 1 + b 1  Y 2 + b 2  Y 3 + b 3 …….

Nuclear and Radiation Physics, BAU, First Semester, (Saed Dababneh). 22 Nuclear Reactions Recoil nucleus Y could be unstable   or  emission. One should think about:  Reaction dynamics and conservation laws i.e. conditions necessary for the reaction to be energetically possible.  Reaction mechanism and theories which explain the reaction.  Reaction cross section i.e. rate or probability.

Nuclear and Radiation Physics, BAU, First Semester, (Saed Dababneh). 23 Nuclear Reactions 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 and Radiation Physics, BAU, First Semester, (Saed Dababneh). 24 Nuclear Reactions 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 31

Nuclear and Radiation Physics, BAU, First Semester, (Saed Dababneh). 25 Nuclear Reactions The double valued situation occurs between T Th and the upper limit T a \. Double-valued in a forward cone. HW 31 (continued)