NUCLEAR STRUCTURE PHENOMENOLOGICAL MODELS

Slides:



Advertisements
Similar presentations
Neutron Excess Asymmetry Remember HWc 1.
Advertisements

3224 Nuclear and Particle Physics Ruben Saakyan UCL
Gamma-ray strength functions Also called in the literature: radiative strength functions photon strength functions Presentation OCL group meeting Ann-Cecilie.
Energy Consumption Fossil Fuel Contribution to Global Energy Demand Year.
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.
Physics is fun!.
Nov 2006, Lecture 2 Nuclear Physics Lectures, Dr. Armin Reichold 1 Lecture 2 The Semi Empirical Mass Formula SEMF.
The Collective Model Aard Keimpema.
CHAPTER 12 The Atomic Nucleus
(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.
RADIOACTIVE DECAY NCCS 1.1.4
BASIC CONCEPTS.  Summary-1  The net nuclear charge in a nuclear species is equal to + Ze, where Z is the atomic number and e is the magnitude.
Brief History of Nuclear Physics 1896-Henri Becquerel ( ) discovered radioactivity 1911-Ernest Rutherford ( ), Hanz Geiger ( )
Happyphysics.com Physics Lecture Resources Prof. Mineesh Gulati Head-Physics Wing Happy Model Hr. Sec. School, Udhampur, J&K Website: happyphysics.com.
Nuclear Physics Nucleus: –nucleons (neutrons and protons) bound together. –Strong Force binds nucleons together over short range (~ m) –Nuclide:
The ground state structure and alpha decay of Hs super- heavy isotopes Junqing Li (Institute of Modern Physics, CAS,Lanzhou) KITPC-CAS Relativistic many-body.
Overview. Nucleus = Protons+ Neutrons nucleons A = nucleon number (atomic mass number) Gives you mass density of element Z = proton number (atomic number)
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.
Chapter 4 The Masses of Nuclei
Chapter 29 Nuclear Physics. General Physics Nuclear Physics Sections 1–4.
1 Chapter 31 Nuclear Physics and Radioactivity Nuclear Structure a)Proton - positive charge - mass x kg ≈ 1 u b) Neutron - discovered.
Nuclear Systematics and Rutherford scattering. Terminology Atomic number (Z) is the number of protons in the nucleus of an atom, and also the number of.
The Shell Model of the Nucleus 5. Nuclear moments
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 MODELS.
2-1 Nuclear Properties Systematic examination of general nuclear properties at the general §masses §matter distributions Size, shape, mass, and relative.
5. Exotic modes of nuclear rotation Tilted Axis Cranking -TAC.
Announcements Four circuits have the form shown in the diagram. The capacitor is initially uncharged and the switch S is open. The values of the emf,
Nuclear Physics Nucleus: –nucleons (neutrons and protons) bound together. –Strong Force binds nucleons together over short range (~ m) –Nuclide:
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/
Chapter 1 Structure of matter Chapter 2 Nuclear transformation
Experimental evidence for closed nuclear shells Neutron Proton Deviations from Bethe-Weizsäcker mass formula: mass number A B/A (MeV per nucleon)
The calculation of Fermi transitions allows a microscopic estimation (Fig. 3) of the isospin mixing amount in the parent ground state, defined as the probability.
THE NUCLEUS AND NUCLEAR REACTIONS. Nuclear descriptions Atomic number Atomic mass number Isotopes nucleons.
Nuclear Models Nuclear force is not yet fully understood.
Nuclear Physics PHY Outline  history  structure of the nucleus nuclear binding force liquid drop model shell model – magic numbers 
 Nature of nuclear forces, cont.  Nuclear Models lecture 3&4.
10-1 Fission General Overview of Fission The Probability of Fission §The Liquid Drop Model §Shell Corrections §Spontaneous Fission §Spontaneously Fissioning.
Radiochemistry Dr Nick Evans
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)
The Nuclear Shell Model A Review of The Nuclear Shell Model By Febdian Rusydi.
Phys 102 – Lecture 27 The strong & weak nuclear forces.
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.
12.3: The Deuteron The determination of how the neutron and proton are bound together in a deuteron. The deuteron mass = u The mass of a deuteron.
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?
July 29-30, 2010, Dresden 1 Forbidden Beta Transitions in Neutrinoless Double Beta Decay Kazuo Muto Department of Physics, Tokyo Institute of Technology.
The Semi-empirical Mass Formula
Happyphysics.com Physics Lecture Resources Prof. Mineesh Gulati Head-Physics Wing Happy Model Hr. Sec. School, Udhampur, J&K Website: happyphysics.com.
Physics 102: Lecture 27, Slide 1 Important announcements Check gradebook (EX/AB) Fill out online ICES evaluation Extra practice problems for final posted.
Nuclear and Radiation Physics, BAU, First Semester, (Saed Dababneh) Nuclear and Radiation Physics Before we start, let us tackle.
Physics 102: Lecture 27, Slide 1 Nuclear Binding, Radioactivity Physics 102: Lecture 28.
Gross Properties of Nuclei
Sizes. W. Udo Schröder, 2011 Nuclear Spins 2 Intrinsic Nuclear Spin Nuclei can be deformed  can rotate quantum mech.  collective spin and magnetic effects.
Nuclear and Radiation Physics, BAU, 1 st Semester, (Saed Dababneh). 1 Electromagnetic moments Electromagnetic interaction  information about.
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.
How do nuclei rotate? 3. The rotating mean field.
Nuclear Phenomenology 3C24 Nuclear and Particle Physics Tricia Vahle & Simon Dean (based on Lecture Notes from Ruben Saakyan) UCL.
Determining Reduced Transition Probabilities for 152 ≤ A ≤ 248 Nuclei using Interacting Boson Approximation (IBA-1) Model By Dr. Sardool Singh Ghumman.
What is the radius (in fm) of {image} ?
CHAPTER 12 The Atomic Nucleus
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 Stability Nuclear Changes
Nuclear Chemistry CHEM 396 Chapter 4, Part B Dr. Ahmad Hamaed
Nuclear Physics, JU, Second Semester,
Nuclear Physics PHY
Presentation transcript:

NUCLEAR STRUCTURE PHENOMENOLOGICAL MODELS From molecules to atomic nuclei. Standard model Basic concepts of nuclear physics. Units Properties of nucleons Liquid drop model Surface vibration and rotation MICROSCOPIC MODELS Nuclear force Nuclear mean field Shell model Second quantisation in the mean field Residual interaction. Collective excitations Collective model. Nilsson model

From molecules to atomic nuclei 10-15m=1fm

Standard model

Basic concepts of nuclear physics nucleon: proton or neutron nuclide: nucleus uniquely specified by number of protons (Z) and neutrons (N) mass number: A=Z+N isotopes: nuclides with the same Z ex: 235U and 238U isotones: nuclides with the same N ex: 2H, 3He isobars: nuclides with the same A atomic mass unit: 1u=1/12 m(12C) =1.66 10-27kg=931.5 MeV/c2

Basic physical observables in nuclei Electric quadrupole momentum Angular momentum Magnetic dipole momentum Parity Energy levels Decay rates

Electric quadrupole moment

Magnetic dipole moment

Units used in nuclear physics Length 1 fm =10-15 m Energy 1 MeV = 106 eV 1 eV = 1,6 10-19 J Basic constants MN=938,90 MeV/c2 ħc=197,33 MeV fm e2=ħc/137=1,44 MeV fm

Properties of nucleons proton neutron mass 1.007276= 938.280 MeV/c2 1.008665= 939.573 MeV/c2 charge +1 spin 1/2 magnetic moment +2.7928 μN -1.9128 μN parity

Nuclear chart stability of nuclei

Limits of stable nuclei exotic nuclei

Nuclear size from electron scattering experiments

Binding energy Mass defect

Example

Binding energy/nucleon: B/A

Liquid drop model Weizsäcker semiempirical formula (1935)

Symmetry energy

Liquid drop energy versus (Z,N)

Surface vibration and rotation Deformation parameters of the nuclear surface

Vibrational states

Rotational states

Total spin I and its projections to laboratory (M) and intrinsic (K) systems Ω

Parameters in the intrinsic system Ω is the rotation angle

β & γ vibrations of a deformed shape

Rotational-vibrational model Rotational bands built on top of the vibrational band head

Sakai-Sheline rule vibrational states → rotational bands

Nuclear force

Deuteron: the simplest nuclear system

Deuteron spin & magnetic moment

Electromagnetic versus strong field

Yukawa potential

Shell model

Nuclear mean field: the selfconsistent single particle potential created by all nucleons

Mean field potential for protons and neutrons

Spin-orbit interaction

Example

Shell model magic numbers appear due to the spin-orbit interaction

Spherical shell model scheme

The last nucleon of an odd-even (even-odd) nucleus determines the nuclear properties (spin, quadrupole and magnetic moments)

Schmidt limits for magnetic moments

Schmidt limits for quadupole moments

creation/annihilation Second quantisation in the mean field Each spherical level is filled by 2j+1 nucleons with different projections creation/annihilation operators for nucleons (fermions) Fermi level Ground state is a Slater determinant obeying the Pauli exclusion principle

Particle (croses) and hole (open circles) states p-h excitation:

(p,2p) reaction in the shell model

Residual interaction among nucleons in the mean field Multipole expansion l=0 : pairing l=2 : quadrupole-quadrupole

Quasiparticle Hamiltonian approximation Ground state =BCS vacuum Particle-particle (p-p) short-range interaction describes pairing correlations Quasiparticle approximation Hamiltonian Ground state =BCS vacuum

Occupation probabilities Gap parameter Normal system Superfluid system Fermi level

Proton gap versus Z

Particle-hole (p-h) long-range interaction describes collective excitations: 1) low-lying surface vibrations 2) giant resonance of protons against neutrons Hamiltonian p-h excitation p h

Distribution of collective excitations for various multipolarities versus energy Giant resonance Low-lying vibrational state

Collective model

Nilsson model of single particle states in the deformed intrinsic system Single particle energy versus deformation Deformed Hamiltonian

DECAY PROCESSES Alpha decay, cluster emission Beta decay Gamma decay Fission and fusion

Nuclear decay modes

Decay law Decay width Γ=ħλ

Narrow decaying resonance (Γ is small) is a quasi-stationary process

Decay rate (activity)

Alpha decay

The first probabilistic interpretation G. Gamow "Zur Quantentheorie des Atomkernes" (On the quantum theory of the atomic nucleus), Zeitschrift für Physik, vol. 51, 204-212 (1928). The first probabilistic interpretation of the wave function Rext ↓ Internal region External region

Quantum penetration explains Geiger-Nuttall law for α and cluster decays (C, O, Ne, Mg, Si) Coulomb parameter

Beta decay

Fermi & Gamow-Teller transitions

Gamma decay

Parity rules for gamma transitions

Decay operators in second quantisation: gamma transitions beta transitions

Fission & fusion

Fission - liquid drop model

Energy release for various processes

Strutinsky shell-model correction The double humped barrier determines the occurrence of superhevy nuclei Density of levels liquid drop shell model

Superheavy nuclei are formed by fusion and detected by alpha decay chains

Fusion energy

The Sun