Symmetries Galore “Not all is lost inside the triangle” (A. Leviatan, Seville, March, 2014) R. F. Casten Yale CERN, August, 2014.

Slides:



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

Shell Model and Collective Models in Nuclei Experimental and theoretical perspectives R. F. Casten WNSL, Yale Univ. RIKEN, January, 2010.
Valence shell excitations in even-even spherical nuclei within microscopic model Ch. Stoyanov Institute for Nuclear Research and Nuclear Energy Sofia,
Generalized pairing models, Saclay, June 2005 Generalized models of pairing in non-degenerate orbits J. Dukelsky, IEM, Madrid, Spain D.D. Warner, Daresbury,
Development of collective behavior in nuclei Results primarily from correlations among valence nucleons. Instead of pure “shell model” configurations,
More General IBA Calculations Spanning the triangle How to use the IBA in real life.
IBA – An Introduction and Overview Basic Ideas, underpinnings, Group Theory, basic predictions.
What is symmetry? Immunity (of aspects of a system) to a possible change.
Single Particle and Collective Modes in Nuclei R. F. Casten WNSL, Yale June, 2009 Wright Nuclear Structure Laboratory Surrey Mini-School Lecture Series.
Single Particle and Collective Modes in Nuclei Lecture Series R. F. Casten WNSL, Yale Sept., 2008.
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.
Review Short range force, Pauli Principle  Shell structure, magic numbers, concept of valence nucleons Residual interactions  favoring of 0 + coupling:
Shell Model and Collective Models in Nuclei Experimental and theoretical perspectives R. F. Casten WNSL, Yale Univ. RIKEN, January, 2010.
Lectures on Nuclear Structure – What nuclei do and why: An empirical overview from a simple perspective CERN, July 2013 Richard F. Casten Yale University.
The proton-neutron interaction and the emergence of collectivity in atomic nuclei R. F. Casten Yale University BNL Colloquium, April 15, 2014 The field.
Low energy Lagrangian and energy levels of deformed nuclei Eduardo A. Coello Perez.
Nuclear structure theory D. Bonatsos NuPECC, March 2015.
Nuclear Low-lying Spectrum and Quantum Phase Transition Zhipan Li School of Physical Science and Technology Southwest University 17th Nuclear Physics Workshop,
Before we did: p2p2 M L & M S Microstate Table States (S, P, D) Spin multiplicity Terms 3 P, 1 D, 1 S Ground state term 3 P.
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.
Assume valence fermions couple in pairs to bosons of spins 0+ and 2+
Nuclei with more than one valence nucleon Multi-particle systems.
Outline  Simple comments on regularities of many-body systems under random interactions  Number of spin I states for single-j configuration  J-pairing.
NSDD Workshop, Trieste, February 2006 Nuclear Structure (II) Collective models P. Van Isacker, GANIL, France.
Even-even nuclei odd-even nuclei odd-odd nuclei 3.1 The interacting boson-fermion model.
Odd nuclei and Shape Phase Transitions: the role of the unpaired fermion PRC 72, (2005); PRC 76, (2007); PRC 78, (2008); PRC 79,
5. Exotic modes of nuclear rotation Tilted Axis Cranking -TAC.
More on Collective models Microscopic drivers: Valence p-n interactions Simply estimating the properties of nuclei Exotic nuclei.
4. The rotating mean field. The mean field concept A nucleon moves in the mean field generated by all nucleons. The mean field is a functional of the.
Themes and challenges of Modern Science Complexity out of simplicity -- Microscopic How the world, with all its apparent complexity and diversity can be.
Lecture 4 Quantum Phase Transitions and the microscopic drivers of structural evolution.
Symmetries in Nuclei, Tokyo, 2008 Symmetries in Nuclei Symmetry and its mathematical description The role of symmetry in physics Symmetries of the nuclear.
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.
原子核配对壳模型的相关研究 Yanan Luo( 罗延安 ), Lei Li( 李磊 ) School of Physics, Nankai University, Tianjin Yu Zhang( 张宇 ), Feng Pan( 潘峰 ) Department of Physics, Liaoning.
The Algebraic Approach 1.Introduction 2.The building blocks 3.Dynamical symmetries 4.Single nucleon description 5.Critical point symmetries 6.Symmetry.
Isospin and mixed symmetry structure in 26 Mg DONG Hong-Fei, BAI Hong-Bo LÜ Li-Jun, Department of Physics, Chifeng university.
Interpreting and predicting structure Useful interpretative models; p-n interaction Second Lecture.
Discovery of a Quasi Dynamical Symmetry and Study of a possible Giant Pairing Vibration R.F. Casten WNSL, Yale May 11,2011 Evidence for a Quasi Dynamical.
PHYS 773: Quantum Mechanics February 6th, 2012
Surrey Mini-School Lecture 2 R. F. Casten. Outline Introduction, survey of data – what nuclei do Independent particle model and residual interactions.
Partial dynamical symmetries in Bose-Fermi systems* Jan Jolie, Institute for Nuclear Physics, University of Cologne What are dynamical symmetries? Illustration.
Wright Nuclear Structure Laboratory, Yale Quantum Phase Transitions in Nuclear Physics R. F. Casten, WNSL, Yale.
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.
Partial Dynamical Symmetry in Odd-Mass Nuclei A. Leviatan Racah Institute of Physics The Hebrew University, Jerusalem, Israel P. Van Isacker, J. Jolie,
Q UANTUM CHAOS IN THE COLLECTIVE DYNAMICS OF NUCLEI Pavel Cejnar, Pavel Stránský, Michal Macek DPG Frühjahrstagung, Bochum 2009, Germany Institute.
Some (more) High(ish)-Spin Nuclear Structure Paddy Regan Department of Physics Univesity of Surrey Guildford, UK Lecture 2 Low-energy.
Correlations in Structure among Observables and Enhanced Proton-Neutron Interactions R.Burcu ÇAKIRLI Istanbul University International Workshop "Shapes.
Quantum phase transitions and structural evolution in nuclei.
Quantum Phase Transitions in Nuclei
Algebraic collective model and its applications Gabriela Thiamová Laboratoire de Physique Subatomique et de Cosmologie Institut National Polytechnique.
Quantum Phase Transition from Spherical to γ-unstable for Bose-Fermi System Mahmut Böyükata Kırıkkale University Turkey collabration with Padova–Sevilla.
How do nuclei rotate? 3. The rotating mean field.
Nuclear Low-lying Spectrum and Quantum Phase Transition 李志攀 西南大学物理科学与技术学院.
Pairing Evidence for pairing, what is pairing, why pairing exists, consequences of pairing – pairing gap, quasi-particles, etc. For now, until we see what.
Determining Reduced Transition Probabilities for 152 ≤ A ≤ 248 Nuclei using Interacting Boson Approximation (IBA-1) Model By Dr. Sardool Singh Ghumman.
R. F. Casten Yale and MSU-FRIB SSNET17, Paris, Nov.6-10, 2017
Surrey Mini-School Lecture 2 R. F. Casten
Stationary Perturbation Theory And Its Applications
Nuclear Chemistry CHEM 396 Chapter 4, Part B Dr. Ahmad Hamaed
Quantum Two.
Presentation transcript:

Symmetries Galore “Not all is lost inside the triangle” (A. Leviatan, Seville, March, 2014) R. F. Casten Yale CERN, August, 2014

Themes and challenges of Modern Science Complexity out of simplicity -- Microscopic How the world, with all its apparent complexity and diversity can be constructed out of a few elementary building blocks and their interactions Simplicity out of complexity – Macroscopic How the world of complex systems can display such remarkable regularity and simplicity What is the force that binds nuclei? Why do nuclei do what they do? What are the simple patterns that nuclei display and what is their origin ? We will look at a model that lives in both camps

The macroscopic perspective (many-body quantal system) often exploits the idea of symmetries These describe the basic structure of the object. Geometrical symmetries describe the shape. Symmetry descriptions are usually analytic and parameter-free ( except for scale). (Scary group theory comment.) One model, the Interacting Boson Approximation (IBA) model, is expressed directly in terms of symmetries. Unfortunately, very few physical systems, especially in atomic nuclei, manifest a symmetry very well. We will see that this statement is now being greatly modified and symmetries may play a much larger role than heretofore.

E (keV) JπJπ Simple Observables - Even-Even Nuclei Relative B(E2) values

E(J) Rot.  ( ħ 2 /2 I )J(J+1) R 4/2 = 3.33 Nuclei that are non-spherical can rotate (1952)! Rotational energies follow the quantum symmetric top: E(0) Rot.  0, E(2) Rot.  6, E(4) Rot.  20 Example of a geometrical symmetry – ellipsoidal, axially symmetric nuclei

J E (keV) ? Without rotor paradigm Paradigm Benchmark Rotor ( ħ 2 /2 I ) J(J + 1) Amplifies structural differences Centrifugal stretching Deviations Identify additional degrees of freedom Value of paradigms

Rotational states Vibrational excitations Rotational states built on (superposed on) vibrational modes Ground or equilibrium state Rotor E(I)  ( ħ 2 /2 I )I(I+1) R 4/2 = 3.33 So, identification of the characteristic predictions of a symmetry both tells us the basic nature of the system and can highlight specific deviations from the perfect symmetry which can point to additional degrees of freedom. Real life example

The IBA – A collective model built on a highly truncated shell model foundation (only configurations with pairs of nucleons coupled to states with angular momentum 0 (s bosons) or 2 (d bosons) Embodies the finite number of valence nucleons. Like the shell model but opposed to traditional collective models, the predictions depend on N and Z

Shell Model Configurations Fermion configurations Boson configurations (by considering only configurations of pairs of fermions with J = 0 or 2.) s bosons and d bosons as the basic building blocks of the collective states The IBA Roughly, gazillions !! Need to simplify Huge truncation of the shell model

Symmetries of the IBA U(5) vibrator SU(3) rotor O(6) γ-soft U(6) Magical group theory stuff happens here Sph. Def. R 4/2 = 2.0 R 4/2 = 3.33 R 4/2 = 2.5 s and d bosons: 6-Dim. problem Three Dynamic symmetries, nuclear shapes IBA Symmetry Triangle What are these symmetries? Idealized structures whose predictions follow analytic formulas, with states labeled by good quantum numbers.

Proliferation of Symmetries ENTER PDS,QDS: Recent work (Leviatan, Van Isacker, Alhassid, Bonatsos, Cejnar, Pietralla, Cakirli, rfc,..): symmetries not limited to vertices: triangle permeated by symmetry elements: AoR, QDS, PDS AoR PDS QDS O(6) PDS – SU(3) QDS However, most nuclei do not exhibit the idealized symmetries: So, is their role just as benchmarks? Most nuclei lie inside the triangle where chaos and disorder are thought to reign.

PDS, QDS: what are these things? They are various situations in which some of the features of a Dyn.Sym. persist even though there is considerable symmetry-breaking. PDS: Some of the levels have the pure symmetry [such as SU(3)] and others are severely mixed QDS: Some of the degeneracies characteristic of a symmetry persist and some of the wave function correlations persist.

SU(3) O(3) Characteristic signatures: Degenerate bands within a group Vanishing B(E2) values between groups....  Typical SU(3) Scheme (for N valence nucleons)  vibrations What do real nuclei look like – what are the data??

Totally typical example Similar in many ways to SU(3). But note that the excited  vibrational excitations are not degenerate as they should be in SU(3). Also there are collective B(E2) values from the  band to the ground band. Most deformed rotors are not SU(3).  vibrations

Clearly, SU(3) is severely broken Or so we thought

B(E2) values in deformed rotor nuclei (typical values) 300 Wu 12 Wu 2 Wu  So, “clearly”, this violates the predictions of SU(3). So, realistic calculations have broken the symmetries (mixed their basis states). The degeneracies, quantum numbers, selection rules of the symmetry no longer apply. …. Or so we thought

What is an SU(3)-PDS? A bit weird!! It is based on the IBA SU(3) symmetry BUT breaks it while retaining pure SU(3) symmetry ONLY the ground and  bands which preserve SU(3) exactly. All other states are severely mixed! Why would we need such a thing? We have excellent fits to the data with numerical IBA calculations that break SU(3). Why would we think  band preserves SU(3)?

(  ) Partial Dynamical Symmetry (PDS) SU(3) So, expect PDS to predict vanishing B(E2) values between these bands as in SU(3). How can that possibly work since empirically these B(E2) values are collective !? BUT,  to ground B(E2)s CAN be finite in the PDS PDS: ONLY  and ground bands are pure SU(3).

SU(3) PDS :  B(E2) values , ground states pure SU(3), others mixed. Generalized T(E2) T(E2) PDS = e [ A (s + d + d + s) + B (d + d)] = e [T(E2) SU(3) + C (s + d + d + s) ] M(E2: J  – J gr ) eC = eC cancels M(E2: J  – J ’ gr ) eC Relative INTERband  to gr B(E2)’s are parameter-free! First term gives zero from SU(3) selection rules. But not second. Hence, relative  to ground B(E2) values: So, Leviatan: PDS works well for 168 Er (Leviatan, PRL, 1996). Accidental or a new paradigm? Tried extensive test for 47 Rare earth nuclei. Key data will be relative  to ground B(E2) values.

Illustrative results

Transitional nuclei

5:100:70 Alaga Lets look into these predictions and comparisons a little deeper. Compare to “Alaga Rules” – what you would get for a pure rotor for RATIOS of squares of transition matrix elements [B(E2) values] from one rotational band to another.

168-Er: The Alaga rules, valence space, and collectivity PDS has pure , gr band K, so why differ from Alaga? Ans: PDS (from IBA) is valence space model: predictions are N val – dep. PDS differs from Alaga solely due to N-Dep effects that arise from the fermion underpinning (Pauli Principle). Valence collective models that agree with the PDS have minimal mixing. Predictions deviating from the PDS signal configuration mixing.

Using the PDS to better understand collective model calculations (and collectivity in nuclei) PDS B(E2:  – gr): the sole reason they differ from the Alaga rules is that they take into account the finite number of valence nucleons. Therefore, IBA calculations (like WCD) that agree with the PDS differ from the Alaga rules purely because of finite valence nucleon number effects. Not heretofore recognized. IBA – CQF deviates further from the Alaga rules, agrees better with the data (and has one fewer parameter). IBA – CQF: The differences from the PDS are due to mixing Can use the PDS to disentangle valence space from mixing!

Again, as one enters the triangle expect vertex symmetries to be highly broken. Consider structures descending from O(6) Now a highly selective O(6) PDS



Calculate wave functions throughout triangle, expand in O(6) basis   good along a line descending from O(6) Remnants of pure O(6) (for the ground state band only) persist along a line in the triangle extending into the region of well-deformed rotational nuclei

Order, Chaos, and the Arc of regularity

Whelan, Alhassid, ca 1989 Order and chaos? What happens generally inside the triangle Arc of Regularity is a narrow zone in the triangle with high degree of order amidst regions of chaotic behavior. What is going on along the AoR? 6 +, 4 +, 3 +, 2 +, , 2 +, n d

Role of the arc as a “boundary” between two classes of structures  AoR – E(0 + 2 ) ~ E(2 + 2 ) Not just a theoretical curiosity: 8 nuclei in the rare earth region have been found to lie along the arc

The symmetry underlying the Arc of Regularity is an SU(3)-based Quasi Dynamical Symmetry QDS All SU(3) degeneracies and all analytic ratios of 0 + bandhead energies persist along the Arc.

Summary AoR PDS QDS O(6) PDS – SU(3) QDS Elements of structural symmetries abound throughout the triangle

Principal Collaborators: R. Burcu Cakirli D. Bonatsos Klaus Blaum Aaron Couture Thanks to Ami Leviatan, Piet Van Isacker, Michal Macek, Norbert Pietralla, C. Kremer for discussions.

BACKUPS

States labelled by quantum numbers Degenerate bands within irrep (  ) T(E2) = eQ = e[(s † d + d † s) - (d † d ) (2) ] (  ) SU(3)

Creation and destruction operators as Example: Consider the case we have just discussed – the spherical vibrator ,2,0 0 E 2E 1 2 Why is the B(E2: 4 – 2) = 2 x B(E2: 2– 0) ?? Difficult to see with Shell Model wave functions with 1000’s of components However, as we have seen, it is trivial using destruction operators WITHOUT EVER KNOWING ANYTHING ABOUT THE DETAILED STRUCTURE OF THESE VIBRATIONS !!!! These operators give the relationships between states. “Ignorance operators”

Finite Valence Space effects on Collectivity Note: 5 N’s up, 5 N’s down: 1 with N Alaga Most dramatic, direct evidence for explicit valence space size in emerging collectivity PDS B(E2: g to Gr) R.F. Casten, D.D. Warner and A. Aprahamian, Phys. Rev. C 28, 894 (1983).

~ 0.03 ~ 0.1 x ~0.03 ~ 0.003

Concepts of group theory Generators, Casimirs, Representations, conserved quantum numbers, degeneracy splitting Generators of a group: Set of operators, O i that close on commutation. [ O i, O j ] = O i O j - O j O i = O k i.e., their commutator gives back 0 or a member of the set For IBA, the 36 operators s † s, d † s, s † d, d † d are generators of the group U(6). Generators : define and conserve some quantum number. Ex.: 36 Ops of IBA all conserve total boson number = n s + n d N = s † s + d † Casimir: Operator that commutes with all the generators of a group. Therefore, its eigenstates have a specific value of the q.# of that group. The energies are defined solely in terms of that q. #. N is Casimir of U(6). Representations of a group: The set of degenerate states with that value of the q. #. A Hamiltonian written solely in terms of Casimirs can be solved analytically

Let’s illustrate group chains and degeneracy- breaking. Consider a Hamiltonian that is a function ONLY of: s † s + d † d That is: H = a(s † s + d † d) = a (n s + n d ) = aN In H, the energies depend ONLY on the total number of bosons, that is, on the total number of valence nucleons. ALL the states with a given N are degenerate. That is, since a given nucleus has a given number of bosons, if H were the total Hamiltonian, then all the levels of the nucleus would be degenerate. This is not very realistic (!!!) and suggests that we should add more terms to the Hamiltonian. I use this example though to illustrate the idea of successive steps of degeneracy breaking being related to different groups and the quantum numbers they conserve. The states with given N are a “representation” of the group U(6) with the quantum number N. U(6) has OTHER representations, corresponding to OTHER values of N, but THOSE states are in DIFFERENT NUCLEI (numbers of valence nucleons).

H’ = H + b d † d = aN + b n d Now, add a term to this Hamiltonian: Now the energies depend not only on N but also on n d States of a given n d are now degenerate. They are “representations” of the group U(5). States with different n d are not degenerate

N N + 1 N + 2 ndnd a 2a E 00 b 2b H’ = aN + b d † d = a N + b n d U(6) U(5) H’ = aN + b d † d Etc. with further terms

Concept of a Dynamical Symmetry N Spectrum generating algebra !! Each successive term: Introduces a new sub-group A new quantum number to label the states described by that group Adds an eigenvalue term that is a function of the new quantum number, hence Breaks a previous degeneracy

Now, WHY are spin increasing transitions so small in Alaga rules and so much larger in the data than in the PDS? 2 J int, R J tot J int, ~R 0, 0 0, 2 0, 4 2, 0  R = 4 !! ~ Forbidden Deviations from Alaga:  – gr. band mixing. E2 matrix element : ME(E2) = [  unpert +  mix ] Can be larger or smaller than the unperturbed. BUT, if unperturbed is forbidden, then ME(E2) = [  mix ] > unpert (which is zero). So mixing always increases forbidden/weak transitions.

Review of phonon creation and destruction operators is a b-phonon number operator. For the IBA a boson is the same as a phonon – think of it as a collective excitation with ang. mom. 0 (s) or 2 (d). What is a creation operator? Why useful? A)Bookkeeping – makes calculations very simple. B) “Ignorance operator”: We don’t know the structure of a phonon but, for many predictions, we don’t need to know its microscopic basis.