Continuing Influence of Shell Effects in the Nuclear

Slides:



Advertisements
Similar presentations
Basic Nuclear Properties
Advertisements

Various Polarization Processes
HIGS2 Workshop June 3-4, 2013 Nuclear Structure Studies at HI  S Henry R. Weller The HI  S Nuclear Physics Program.
Photo-Nuclear Physics Experiments by using an Intense Photon Beam Toshiyuki Shizuma Gamma-ray Nondestructive Detection Research Group Japan Atomic Energy.
Giant resonances, exotic modes & astrophysics
Gamma-ray strength functions Also called in the literature: radiative strength functions photon strength functions Presentation OCL group meeting Ann-Cecilie.
HL-5 May 2005Kernfysica: quarks, nucleonen en kernen1 Outline lecture (HL-5) Collective excitations of nuclei photo-excitation of GDR particle-hole excitations.
The Sum Over States model, although exact, requires a detailed knowledge of many parameters which are not generally available. Experience has shown that.
December 20, 2007, Sergey Bastrukov Elastic Vibrations of Atomic Nuclei and Neutron Stars Brief review of elastodynamical approach to the continuum mechanics.
 Lecture 3 .  Dielectric Materials  Dielectric materials are also called as insulators.  In dielectric materials, all the electrons are tightly bound.
Time dependence of SM parameters. Outline Dirac´s hypothesis SM parameters Experimental access to time dependence  laboratory measurements  Quasar absorption.
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 STRUCTURE PHENOMENOLOGICAL MODELS
Vibrational and Rotational Spectroscopy
The Shell Model of the Nucleus 5. Nuclear moments
Effects of self-consistence violations in HF based RPA calculations for giant resonances Shalom Shlomo Texas A&M University.
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.
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.
Ch ; Lecture 26 – Quantum description of absorption.
Pygmy Dipole Resonance in 64Fe
Magnetism and ElectroMagnetism
 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.
Anomalous two-neutron transfer in neutron-rich Ni and Sn isotopes studied with continuum QRPA H.Shimoyama, M.Matsuo Niigata University 1 Dynamics and Correlations.
NUCLEAR LEVEL DENSITIES NEAR Z=50 FROM NEUTRON EVAPORATION SPECTRA IN (p,n) REACTION B.V.Zhuravlev, A.A.Lychagin, N.N.Titarenko State Scientific Center.
Lecture X Magnetism and Matter Learning Objective: to examine some aspects of magnetic properties of materials.
Nuclear Structure SnSn P,n p n (  )‏ ( ,Xn)‏ M1E1 p,nn X λ ?E1 ExEx  Study of the pygmy dipole resonance as a function of deformation.
NEUTRON SKIN AND GIANT RESONANCES Shalom Shlomo Cyclotron Institute Texas A&M University.
Landau diamagnetism and de Hass van Alphen effect by Enas Hamasha Stastical mechanics ph 761 Dr. Abdulla Obeidat.
Total photoabsorption on quasi free nucleons at 600 – 1500 MeV N.Rudnev, A.Ignatov, A.Lapik, A.Mushkarenkov, V.Nedorezov, A.Turinge for the GRAAL collaboratiion.
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 and Radiation Physics, BAU, First Semester, (Saed Dababneh). 1 Extreme independent particle model!!! Does the core really remain inert?
R. Machleidt, University of Idaho Recent advances in the theory of nuclear forces and its relevance for the microscopic approach to dense matter.
July 29-30, 2010, Dresden 1 Forbidden Beta Transitions in Neutrinoless Double Beta Decay Kazuo Muto Department of Physics, Tokyo Institute of Technology.
DIRECT AND SEMIDIRECT NEUTRON RADIATIVE CAPTURE BY MEDIUM-HEAVY MASS NUCLEI: A NEW VERSION OF THE SEMIMICROSCOPIC DESCRIPTION B.A. Tulupov 1, M.H. Urin.
CEBAF - Continuous Electron Beam Accelerator Facility.
Pion-Induced Fission- A Review Zafar Yasin Pakistan Institute of Engineering and Applied Sciences (PIEAS) Islamabad, Pakistan.
Chapter 6 Magnetostatic Fields in Matter 6.1 Magnetization 6.2 The Field of a Magnetized Object 6.3 The Auxiliary Field 6.4 Linear and Nonlinear Media.
PROPERTIES OF HIGH-ENERGY ISOSCALAR MONOPOLE EXCITATIONS IN MEDIUM-HEAVY MASS SPHERICAL NUCLEI M. L. Gorelik 1), S. Shlomo 2), B. A. Tulupov 3), M. H.
Simultaneous photo-production measurement of the  and  mesons on the nucleons at the range 680 – 1500 MeV N.Rudnev, V.Nedorezov, A.Turinge for the GRAAL.
Systematical Analysis of Fast Neutron Induced Alpha Particle Emission Reaction Cross Sections Jigmeddorj Badamsambuu, Nuclear Research Center, National.
Cytomechanics of Osteoblasts and Osteoblast-like cells Dept. of Experimental Orthopaedics and Biomechanics Prof. Dr.David B.Jones.
Few-Body Models of Light Nuclei The 8th APCTP-BLTP JINR Joint Workshop June 29 – July 4, 2014, Jeju, Korea S. N. Ershov.
Laboratory system and center of mass system
Electromagnetic (gamma) decay
Determining Reduced Transition Probabilities for 152 ≤ A ≤ 248 Nuclei using Interacting Boson Approximation (IBA-1) Model By Dr. Sardool Singh Ghumman.
Generation of Magnetic Field
Structure and dynamics from the time-dependent Hartree-Fock model
What is the radius (in fm) of {image} ?
Chapter 10 Magnetic Properties Introduction 10
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.
Isospin Symmetry test on the semimagic 44Cr
AP Physics C: Electricity & Magnetism – Charges & Electric Field
Nuclear Chemistry CHEM 396 Chapter 4, Part B Dr. Ahmad Hamaed
all Cooper pairs must behave in the same way
Intermediate-mass-fragment Production in Spallation Reactions
Nuclear excitations in relativistic nuclear models
Nuclear Magnetic Resonance (NMR) Spectroscopy
Parametrisation of Binding Energies
10.3 NMR Fundamentals nuclear spin calculations and examples
Lecture 12 Optical Properties Md Arafat Hossain Outlines.
Chapter 4 Mechanisms and Models of Nuclear Reactions
From Atoms, to Nucleons, to Quarks
Nuclear Decays Unstable nuclei can change N,Z.A to a nuclei at a lower energy (mass) If there is a mass difference such that energy is released, pretty.
Quantum Mechanical Treatment of The Optical Properties
PHYS 3446 – Review Review Note Test deferred until Weds.
Ginzburg-Landau theory
Presentation transcript:

Continuing Influence of Shell Effects in the Nuclear  Quasi-Continuum 45Sc Cebo Ngwetsheni Nico orce 51V 153Sm 50V 56Fe

Outline Nuclear Polarizability​ Low energy enhancement (LEE)​ Systematics & Results​ Conclusion & Work Ahead

Nuclear Polarizability  Nuclei polarize in presence of an external electromagnetic field. Polarizability is driven by the dynamics of the giant dipole resonance (GDR) [1]. Inter-penetration motion of proton and neutron fluids, out of phase. The GDR motion is induced by the nuclear symmetry  energy, acting as a restoring force  [1]. from the Bethe-Weizsacker semi-empirical mass formula:  Ground state Figure: 1a

Nuclear Polarizability  Polarizability can be described macro- and microscopically:​ Hydrodynamic model [1] ​ ​                                 ​    ​ assuming a well-defined nuclear surface:  2.   Second order perturbation theory [1]:              where,  Figure 1b

Nuclear Polarizability Naturally, total cross section values should include both electric and magnetic polarizability contributions, IPM: diamagnetism is dominant for nuclei with A > 60 and paramagnetism dominates in light nuclei with the rise of permanent magnetic dipole moments and can contribute substantially to σ−2 values for nuclei with A < 20 [2]. where the magnetic polarizability is dependent on paramagnetic and diamagnetic susceptibilities,

Polarizability & Symmetry Energy Mass dependence of the symmetry energy yields [3][4] :      Figure 2

Low-Energy-Enhancement LEE is observed as an up-bend at low energies of measured photon strength function (PSF) for medium and heavy-mass nuclei. LEE observed in medium and heavy mass nuclei starting   at ~ 3 MeV & ~ 2 MeV, respectively. The physical origin of the LEE remains ambiguous, observed in A ≈ 50 and 90 mass region. Interpreted as: TCQRPA, predicts E1 transitions from the hot quasi-continuum to continuum region produces the up-bend [4]​. Shell model  calculations predict LEE has a predominant M1 character, resulting from active high-j proton & neutron orbits with magnetic moments adding up coherently [5].        ​ Figure 3

LEE & GDR   In order to combine the cross-section contributions from the LEE and GDR , we use the relation: The similar features suggest a common physical origin for all GDR's in concordance with the Brink-Axel hypothesis, which also posits that a GDR can be built on every state in a nucleus. Henceforth, we assume similar resonance strengths for GDR s built on the ground and excited states. where, 238Np

LEE Extrapolation Setting up the low-energy cut off is not obvious.    LEE Extrapolation Setting up the low-energy cut off is not obvious. Recent SM calculations support the continuaation of the LEE to 0 MeV. We investigated two cases; extrapolation down to 0.8 MeV and 0.1 MeV

The semi-magic nuclei present smaller polarizability parameters, less than unity. The polarizability accunts for deviations from actual GDR effects  to that predicted by the hydrodynamic model These observations support continuation of shell effects in the quasi-continuum region where LEE occurs

CONCLUSION The sudden σ−2  values and k<1 for nuclei with neutron magic numbers N = 28, 50 and 82 supports the M1 nature of the LEE predicted by SM calculations. And validity of the Brink-Axel hypothesis, which seems to allow for structural changes. This work emphasizes the need for additional f(Eγ) measurements at low energies below 1 MeV and photo-proton  cross sections, particularly for low mass nuclei.

Other Work ... Implications of κ: κ > 1 may strongly affect the determination of reduced transition probabilities, or B(E2)'s and Qs values.    κ < 1 indicates shell effects. The polarization potential, proportional to α, tends to reduce the effective quadrupole potential, , to be corrected !!

Other Work ... Only three favorable Coulomb-excitation measurements provide unambiguous information on κ values of excited states; namely 6Li (J=3) , 7Li (J=½), 17O (J=½) shown as green diamonds NB: Qs = 0 for J=0, ½ allowing reliable measurements of κ values. Shell model κ values are represented by red squares in the Figure. Nucleus Ex (MeV) Jπ κSM κCoulex 7Li 0.478 ½- 3.4 4.4 (10) 12C 4.439 21+ 2.2 (2) 2.2+0.2 17O 0.871 ½+ 3.8 8.3 (6) Figure 3

Thank You !!