Collective properties of even- even nuclei Vibrators and rotors With three Appendices.

Slides:



Advertisements
Similar presentations
Some (more) Nuclear Structure
Advertisements

Isomer Spectroscopy in Near-Spherical Nuclei Lecture at the ‘School cum Workshop on Yrast and Near-Yrast Spectroscopy’ IIT Roorkee, October 2009 Paddy.
Gamma-ray strength functions Also called in the literature: radiative strength functions photon strength functions Presentation OCL group meeting Ann-Cecilie.
Development of collective behavior in nuclei Results primarily from correlations among valence nucleons. Instead of pure “shell model” configurations,
With five Appendices at the end. Deformed nuclei So far, we have dealt with spherical nuclei only. How do we describe deformed nuclei? We need two parameters.
More General IBA Calculations Spanning the triangle How to use the IBA in real life.
Review Short range force, Pauli Principle  Shell structure, magic numbers, concept of valence nucleons Residual interactions  favoring of 0 + coupling:
The Collective Model Aard Keimpema.
Structure of odd-odd nuclei in the interacting boson fermion-fermion model 3.
Multipole Decomposition of Residual Interactions We have seen that the relative energies of 2-particle systems affected by a residual interaction depend.
NPSC-2003Gabriela Popa Microscopic interpretation of the excited K  = 0 +, 2 + bands of deformed nuclei Gabriela Popa Rochester Institute of Technology.
More General IBA Calculations Spanning the triangle.
How nuclei behave: a simple perspective based on symmetry and geometry (with a discussion of the microscopic drivers of structural evolution) R. F. Casten.
Masses (Binding energies) and the IBA Extra structure-dependent binding: energy depression of the lowest collective state.
(An outgrowth of our studies of shape/phase transitions and empirical signatures for them) A) An enhanced link between nuclear masses and structure B)
The IBA The Interacting Boson Approximation Model Preliminary review of collective behavior in nuclei Collective models, and why the IBA Basic ideas about.
IBA Lecture 3. Mapping the entire triangle Technique of orthogonal crossing contours (OCC)
IBA Lecture part 2. Most general IBA Hamiltonian in terms with up to four boson operators (given N) IBA Hamiltonian Mixes d and s components of the wave.
Nuclei with more than one valence nucleon Multi-particle systems.
PHYS 221 Recitation Kevin Ralphs Week 14. Overview Nuclear Physics – Structure of the Nucleus – Nuclear Reactions.
NSDD Workshop, Trieste, February 2006 Nuclear Structure (II) Collective models P. Van Isacker, GANIL, France.
The Physical Setting Chemistry.
1 The Physical Setting Chemistry Jerry Deutsch 2 New York State Education Department Core Curriculum
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 4 Quantum Phase Transitions and the microscopic drivers of structural evolution.
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/
1 In-Beam Observables Rauno Julin Department of Physics University of Jyväskylä JYFL Finland.
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.
The Algebraic Approach 1.Introduction 2.The building blocks 3.Dynamical symmetries 4.Single nucleon description 5.Critical point symmetries 6.Symmetry.
Interpreting and predicting structure Useful interpretative models; p-n interaction Second Lecture.
Nuclear Chemistry The Guide to types of Radioactive Decay and their Properties.
Surrey Mini-School Lecture 2 R. F. Casten. Outline Introduction, survey of data – what nuclei do Independent particle model and residual interactions.
Shell Model with residual interactions – mostly 2-particle systems Start with 2-particle system, that is a nucleus „doubly magic + 2“ Consider two identical.
Symmetries and collective Nuclear excitations PRESENT AND FUTURE EXOTICS IN NUCLEAR PHYSICS In honor of Geirr Sletten at his 70 th birthday Stefan Frauendorf,
ShuangQuan Zhang School of Physics, Peking University Static chirality and chiral vibration of atomic nucleus in particle rotor model.
Collective properties of even-even nuclei – Miscellaneous topics Vibrators and rotors.
TESTS OF PARTIAL DYNAMICAL SYMMETRIES AND THEIR IMPLICATIONS R. F. Casten Yale SDANCA, Oct. 9, 2015.
Lecture 23: Applications of the Shell Model 27/11/ Generic pattern of single particle states solved in a Woods-Saxon (rounded square well)
Shell Model with residual interactions – mostly 2-particle systems Simple forces, simple physical interpretation Lecture 2.
Quantum Phase Transitions (QPT) in Finite Nuclei R. F. Casten June 21, 2010, CERN/ISOLDE.
Testing Theories (What to do and what definitely not to do) R. F. Casten Yale August 2014.
A close up of the spinning nucleus S. Frauendorf Department of Physics University of Notre Dame, USA IKH, Forschungszentrum Rossendorf Dresden, Germany.
Some (more) High(ish)-Spin Nuclear Structure Paddy Regan Department of Physics Univesity of Surrey Guildford, UK Lecture 2 Low-energy.
1 The Physical Setting Chemistry Jerry Deutsch 2 New York State Education Department Core Curriculum
Quantum phase transitions and structural evolution in nuclei.
Quantum Phase Transitions in Nuclei
Chiral Symmetry Breaking in Nuclei J.H. Hamilton 1, S.J. Zhu 1,2,3, Y.X. Luo 1,4,, A.V. Ramayya 1, J.O. Rasmussen 4, J.K. Hwang 1, S. Frauendorf 5, V.
Aim: Why do fission and fusion reactions release so much energy? Essential Questions : Compare and contrast nuclear fission with fusion. Distinguish between.
W. Udo Schröder, 2005 Gamma Decay 1. W. Udo Schröder, 2005 Gamma Decay 2 Photons Photons: generated by moving charge distributions. Distributions can.
Pairing Evidence for pairing, what is pairing, why pairing exists, consequences of pairing – pairing gap, quasi-particles, etc. For now, until we see what.
超重原子核的结构 孙 扬 上海交通大学 合作者:清华大学 龙桂鲁, F. Al-Khudair 中国原子能研究院 陈永寿,高早春 济南,山东大学, 2008 年 9 月 20 日.
Large-Scale Shell-Model Study of the Sn-isotopes
Determining Reduced Transition Probabilities for 152 ≤ A ≤ 248 Nuclei using Interacting Boson Approximation (IBA-1) Model By Dr. Sardool Singh Ghumman.
The Physical Setting Chemistry Jerry Deutsch.
The role of isospin symmetry in medium-mass N ~ Z nuclei
Shape parameterization
Kazuo Muto Tokyo Institute of Technology (TokyoTech)
PHL424: Nuclear rotation.
Surrey Mini-School Lecture 2 R. F. Casten
Isospin Symmetry test on the semimagic 44Cr
Radioactive Decay.
Radioactive Decay.
Radioactive Decay.
a non-adiabatic microscopic description
individual excitations of nucleons
Nuclear Tidal Waves Daniel Almehed Stefan Frauendorf Yongquin Gu
High spin physics- achievements and perspectives
Nuclei at the Extremes of Spin: The Superdeformed Bands in 131,132Ce
Rotational Energy Levels for rigid rotor: Where Rotational Spectra of Rigid Diatomic molecule. BY G JANAKIRAMAN EGS A&S COLLAGE
Presentation transcript:

Collective properties of even- even nuclei Vibrators and rotors With three Appendices

What happens with both valence neutrons and protons? Case of few valence nucleons: Lowering of energies, development of multiplets. R 4/2  ~2 Vibrational modes, 1- and multi-phonon 2-particle spectra Intermediate

Lots of valence nucleons of both types R 4/2  ~3.33

B(E2; 2 +  0 + )

Broad perspective on structural evolution: R 4/2 Note the characteristic, repeated patterns

Development of collective behavior in nuclei Results primarily from correlations among valence nucleons. Instead of pure “shell model” configurations, the wave functions are mixed – linear combinations of many components. Leads to a lowering of the collective states and to enhanced transition rates as characteristic signatures. How does this happen? Consider mixing of states.

A illustrative special case of fundamental importance T Lowering of one state. Note that the components of its wave function are all equal and in phase Consequences of this: Lower energies for collective states, and enhanced transition rates. Lets look at the latter in a simple model.

W

Even-even Deformed Nuclei Rotations and vibrations

Rotational states Vibrational excitations Rotational states built on(superposed on) vibrational modes Ground or equilibirum state

Systematics and collectivity of the lowest vibrational modes in deformed nuclei

E2 transitions in deformed nuclei Intraband --- STRONG, typ. ~ 200 W.u. in heavy nuclei Interband --- Collective but much weaker, typ W.u. Which bands are connected? Alaga Rules for Branching ratios

0

Experimental B(E2) values in deformed nuclei

How to fix the model? Note: the Alaga rules assume that each band is pure – ground or gamma, in character. What about if they MIX ?? Bandmixing formalism

Mixing of gamma and ground state bands

Axially Asymmetric Nuclei Two types: “gamma” soft (or “unstable”), and rigid

First: Gamma soft E ~  (  + 3 ) ~ J max ( J max + 6 ) Note staggering in gamma band energies

E ~ J ( J + 6 ) E ~ J ~ J ( J + )  E ~ J ( J + 1 ) Overview of yrast energies

“Gamma” rigid or Davydov model Note opposite staggering in gamma band energies

Use staggering in gamma band energies as signature for the kind of axial asymmetry

Appendix A on Intruder States Another form of collective mode that sometimes appears in the low lying spectrum or can even become the ground state equilibrium cofiguration

The basic idea behind Intruder States: a 2- particle - 2-hole excitation that costs energy but gains it back by added collectivity which increases with increasing valence nucleon number.

Burcu Cakirli et al. Beta decay exp. + IBA calcs.

Appendix B on development of collectivity and lowering of collective energies by configuration mixing

Appendix C on energies and transition rates of 3- phonon states in terms of 2- phonon state anharmonicities