Kernfysica: quarks, nucleonen en kernen

Slides:



Advertisements
Similar presentations
BigBite K.Egiyan Probabilities of SRC in Nuclei Measured with A(e,e / ) Reactions K. Egiyan (Yerevan Physics Institute, Yerevan, Armenia and Jefferson.
Advertisements

CoulEx. W. Udo Schröder, 2012 Shell Models 2 Systematic Changes in Nuclear Shapes Møller, Nix, Myers, Swiatecki, Report LBL 1993: Calculations fit to.
HL-1 May 2, 2006Kernfysica: quarks, nucleonen en kernen1 Outline lecture (HL-1) Particle Production Particle production in e + e - collisions Detection.
Spectroscopy at the Particle Threshold H. Lenske 1.
Gamma-ray strength functions Also called in the literature: radiative strength functions photon strength functions Presentation OCL group meeting Ann-Cecilie.
HL-3 May 2006Kernfysica: quarks, nucleonen en kernen1 Outline lecture (HL-3) Structure of nuclei NN potential exchange force Terra incognita in nuclear.
HL-5 May 2005Kernfysica: quarks, nucleonen en kernen1 Outline lecture (HL-5) Collective excitations of nuclei photo-excitation of GDR particle-hole excitations.
Kernfysica: quarks, nucleonen en kernen
HL-2 April 2004Kernfysica: quarks, nucleonen en kernen1 Outline lecture (HL-2) Quarkonium Charmonium spectrum quark-antiquark potential chromomagnetic.
8-1 RFSS: Lecture 8 Nuclear Force, Structure and Models Readings: §Nuclear and Radiochemistry: Chapter 10 (Nuclear Models) §Modern Nuclear Chemistry: Chapter.
Lecture 25 Quantum Mechanics of Atoms and Atomic Systems Chapter  Outline Quantum Mechanics and Periodic Table Atomic Structure and Conductivity.
P461 - Nuclei I1 Properties of Nuclei Z protons and N neutrons held together with a short-ranged force  gives binding energy P and n made from quarks.
II. Spontaneous symmetry breaking. II.1 Weinberg’s chair Hamiltonian rotational invariant Why do we see the chair shape? States of different IM are so.
Course Title: Nuclear Physics Course Code: EEE-202
Lecture 3 Many - electron atoms. The orbital approximation Putting electrons into orbitals similar to those in the hydrogen atom gives a useful way of.
(and some things about the weak interaction)
Direct Reactions. Optical model Represent the target nucleus by a potential -- Attenuation length.
P461 - Nuclei II1 Nuclear Shell Model Potential between nucleons can be studied by studying bound states (pn, ppn, pnn, ppnn) or by scattering cross sections:
Nuclear models. Models we will consider… Independent particle shell model Look at data that motivates the model Construct a model Make and test predictions.
P461 - Nuclei I1 Properties of Nuclei Z protons and N neutrons held together with a short-ranged force  gives binding energy P and n made from quarks.
The Quantum Mechanical Picture of the Atom
NUCLEAR STRUCTURE PHENOMENOLOGICAL MODELS
The National Superconducting Cyclotron State University Betty Tsang, 2/24-26/2005 INFN Workshop on Reactions and Structure with Exotic.
8-1 RFSS: Lecture 8 Nuclear Force, Structure and Models Part 1 Readings: §Nuclear and Radiochemistry: Chapter 10 (Nuclear Models) §Modern Nuclear Chemistry:
Nuclear and Radiation Physics, BAU, First Semester, (Saed Dababneh). 1 Nuclear Force Spin dependent  difference in neutron scattering cross.
The Shell Model of the Nucleus 5. Nuclear moments
Nucleons & Nuclei a quick guide to the real essentials in the subject which particle and nuclear physicists won’t tell you.
Lecture 10: Inelastic Scattering from the Proton 7/10/2003
Atomic Orbitals, Electron Configurations, and Atomic Spectra
Chapters 9, 11, 12 Concepts covered that will also be candidates for exam questions.
5. Exotic modes of nuclear rotation Tilted Axis Cranking -TAC.
The Shell Model of the Nucleus 2. The primitive model
Vector coupling of angular momentum. Total Angular Momentum L, L z, S, S z J and J z are quantized Orbital angular momentumSpin angular momentum Total.
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/
Lecture 16: Beta Decay Spectrum 29/10/2003 (and related processes...) Goals: understand the shape of the energy spectrum total decay rate sheds.
5-1 RDCH 702: Lecture 5 Nuclear Force, Structure and Models Readings: §Nuclear and Radiochemistry: Chapter 10 (Nuclear Models) §Modern Nuclear Chemistry:
Orbitals and energetics
Wolfram KORTEN 1 Euroschool Leuven – September 2009 Coulomb excitation with radioactive ion beams Motivation and introduction Theoretical aspects of Coulomb.
Nuclear Models Nuclear force is not yet fully understood.
Size and Structure Mikhail Bashkanov University of Edinburgh UK Nuclear Physics Summer School III.
Radiochemistry Dr Nick Evans
Lecture 23: Applications of the Shell Model 27/11/ Generic pattern of single particle states solved in a Woods-Saxon (rounded square well)
The nuclear mean field and its symmetries W. Udo Schröder, 2011 Mean Field 1.
The Nuclear Shell Model A Review of The Nuclear Shell Model By Febdian Rusydi.
Lecture 21: On to Finite Nuclei! 20/11/2003 Review: 1. Nuclear isotope chart: (lecture 1) 304 isotopes with t ½ > 10 9 yrs (age of the earth) 177.
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 and Radiation Physics, BAU, First Semester, (Saed Dababneh). 1 Extreme independent particle model!!! Does the core really remain inert?
Chapter 6 Electronic Structure Section 6.5 to End.
Nuclear and Radiation Physics, BAU, 1 st Semester, (Saed Dababneh). 1 The Deuteron Deuterium (atom). The only bound state of two nucleons  simplest.
Chapter 6 Section 2. Sec 6.5 Quantum Mechanics and Atomic Orbitals Wave functions – describes the behavior of the electron, denoted with the Greek letter,
Nuclear and Radiation Physics, BAU, 1 st Semester, (Saed Dababneh). 1 Electromagnetic moments Electromagnetic interaction  information about.
Nuclear Physics, JU, Second Semester,
Chapter 6 Section 2. Quantum Mechanics and Atomic Orbitals Wave functions – describes the behavior of the electron, denoted with the Greek letter, ψ The.
Semi-Empirical Mass Formula part II Quantum Terms
Pairing Evidence for pairing, what is pairing, why pairing exists, consequences of pairing – pairing gap, quasi-particles, etc. For now, until we see what.
Electric Dipole Response, Neutron Skin, and Symmetry Energy
CHEM 312 Lecture 7: Fission Readings: Modern Nuclear Chemistry, Chapter 11; Nuclear and Radiochemistry, Chapter 3 General Overview of Fission Energetics.
V. Nuclear Reactions Topics to be covered include:
The role of isospin symmetry in medium-mass N ~ Z nuclei
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.
Nuclear Chemistry CHEM 396 Chapter 4, Part B Dr. Ahmad Hamaed
Lecture 5-6 xxxxxxx.
Nuclear Physics, JU, Second Semester,
Kernfysica: quarks, nucleonen en kernen
Single particle states
Multielectron Atoms The quantum mechanics approach for treating multielectrom atoms is one of successive approximations The first approximation is to treat.
Aim: How is the electron organized in the atom?
Chapter 6 Section 2.
II. Spontaneous symmetry breaking
Presentation transcript:

Kernfysica: quarks, nucleonen en kernen Outline lecture (HL-4) HL-4 May 2004 Structure of nuclei Shell structure Deformation Nuclear reactions Stripping reaction DWBA Literature: PR 16, 17 HL-4 May 2004 Kernfysica: quarks, nucleonen en kernen Kernfysica: quarks, nukleonen en kernen

energy of 1. exc. state of even-even nuclei typ. JP=2+ shell and level structure determined by depth/shape of central potential, spin-orbit force, residual interaction (pairing correlations) j=l-1/2 j=l+1/2 HL-4 May 2004 Kernfysica: quarks, nucleonen en kernen

single-particle levels nlj shell gaps and intruder states HL-4 May 2004 Kernfysica: quarks, nucleonen en kernen

particle- and hole-states and excitations HL-4 May 2004 mirror pair, hole mirror pair, nucleon isospin independence of nuclear force HL-4 May 2004 Kernfysica: quarks, nucleonen en kernen Kernfysica: quarks, nukleonen en kernen

deformed nuclei: quadrupole moments prolate partially occupied p- and n-shells polarized the nucleus deformation oblate HL-4 May 2004 Kernfysica: quarks, nucleonen en kernen

regions of large deformation half-full shells  deformation Hund rule for atom shells: nl subshell filling: first different orbitals l next substates ml repulsive Coulomb force favours separate orbitals HL-4 May 2004 Kernfysica: quarks, nucleonen en kernen

pairing and polarization HL-4 May 2004 attractive NN force favours: pairing: l1 = l2; m1 = -m2; j = 0; JP = 0+ adjacent m-substate filling overlapping adjacent m-orbitals  deformation Nilsson Parameters:  = lz  = jz energy levels of deformed nuclei  ellipsoidal potential shape HL-4 May 2004 Kernfysica: quarks, nucleonen en kernen Kernfysica: quarks, nukleonen en kernen

extended SPSM: Nilsson model [Nn3] single-particle motion in anisotropic oscillator field: quantum numbers N = n3 + n   deformation   - 3 HL-4 May 2004 Kernfysica: quarks, nucleonen en kernen

deformation parameters: exp. and calc.  = exp. A even  = exp. A uneven  = calc. A uneven HL-4 May 2004 Kernfysica: quarks, nucleonen en kernen

spectroscopy through nuclear reactions stripping reaction 16O(d,p)17O Proton spectrum at 45 and Ed = 25.4 MeV (n-1d5/2)1 (n-1d3/2)1 (n-2s1/2)1 HL-4 May 2004 Kernfysica: quarks, nucleonen en kernen

single-particle levels nlj shell gaps, intruder states level sequence in sd shell (n-1d3/2)1 (n-2s1/2)1 (n-1d5/2)1 HL-4 May 2004 Kernfysica: quarks, nucleonen en kernen

stripping cross section for Ed (vd)  binding of d and binding of n in A+1 nucleus A A+1 Fermi´s Golden Rule for weak d-A and p-(A-1) interaction: Born approx.: likely final state with n in outer shell: with shell-model w.f. for n and short-range stripping interaction: q-transfer to nucleus! HL-4 May 2004 Kernfysica: quarks, nucleonen en kernen

DWBA for stripping reaction X(a,b)Y proton angular distribution for 16O(d,p)17O at Ed = 25.4 MeV l=2 plane waves  scattered waves: solutions for complex optical potential V(r) + iW(r) taking into account absorption by W(r) q=0 is Y=X+(a-b) a single-particle state ?? initial-state spin l=0 l=2 spectroscopic factors Sl,j measure single-particle character excellent agreement for small q HL-4 May 2004 Kernfysica: quarks, nucleonen en kernen

Kernfysica: quarks, nucleonen en kernen HL-4 May 2004 Summary lecture (HL-4) Nuclear structure Shell structure and shell gaps appear due to ls term Deformations in half-filled shells and polarization Nuclear reactions Stripping reactions study level structure DWBA approximation for transfer: spectroscopic factors Sl,j measure single-particle character HL-4 May 2004 Kernfysica: quarks, nucleonen en kernen Kernfysica: quarks, nukleonen en kernen