Electromagnetic Properties of

Slides:



Advertisements
Similar presentations
Lifetime measurements in 128 Cs and 132 La as a test of chirality Kazimierz Dolny September 2005 Julian Srebrny Nuclear Physics Division Institute of Experimental.
Advertisements

Nuclear structure in the A~50 region Roberto V. Ribas Instituto de Física – USP XXVII RTFNB – Santos, 2004.
How do nuclei rotate? 5. Appearance of bands. Deformed mean field solutions This is clearly the case for a well deformed nucleus. Deformed nuclei show.
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.
The Collective Model Aard Keimpema.
Structure of odd-odd nuclei in the interacting boson fermion-fermion model 3.
Projected-shell-model study for the structure of transfermium nuclei Yang Sun Shanghai Jiao Tong University Beijing, June 9, 2009.
High spin states in 136,137 La, 148 Ce and 105 Mo.
NPSC-2003Gabriela Popa Microscopic interpretation of the excited K  = 0 +, 2 + bands of deformed nuclei Gabriela Popa Rochester Institute of Technology.
Nuclear models. Models we will consider… Independent particle shell model Look at data that motivates the model Construct a model Make and test predictions.
W. Udo Schröder, 2005 Rotational Spectroscopy 1. W. Udo Schröder, 2005 Rotational Spectroscopy 2 Rigid-Body Rotations Axially symmetric nucleus 
Microwave Spectroscopy II
Rotational bands in the rare-earth proton emitters and neighboring nuclei Darek Seweryniak Argonne National Laboratory PROCON Rotational landscape.
The Shell Model of the Nucleus 5. Nuclear moments
NSDD Workshop, Trieste, February 2006 Nuclear Structure (II) Collective models P. Van Isacker, GANIL, France.
The stability of triaxial superdeformed shape in odd-odd Lu isotopes Tu Ya.
5. Exotic modes of nuclear rotation Tilted Axis Cranking -TAC.
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.
Symmetries in Nuclei, Tokyo, 2008 Symmetries in Nuclei Symmetry and its mathematical description The role of symmetry in physics Symmetries of the nuclear.
Chirality of Nuclear Rotation S. Frauendorf Department of Physics University of Notre Dame, USA IKH, Forschungszentrum Rossendorf Dresden, Germany.
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/
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.
ShuangQuan Zhang ( 张双全 ) School of Physics, Peking University Recent theoretical developments in chirality in atomic nuclei Beihang.
1 New symmetries of rotating nuclei S. Frauendorf Department of Physics University of Notre Dame.
Nuclear Models Nuclear force is not yet fully understood.
How do nuclei rotate? 1. The molecular picture.
Spontaneous symmetry breaking and rotational bands S. Frauendorf Department of Physics University of Notre Dame.
Shell Model with residual interactions – mostly 2-particle systems Start with 2-particle system, that is a nucleus „doubly magic + 2“ Consider two identical.
How do nuclei rotate? The nucleus rotates as a whole.
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.
Search for chiral doublet structures in odd-A 79 Kr with the Hyperball2 CYRIC CYRIC/Tohoku University J.Timar ATOMKI (Hungary) K. Starosta (MSU)
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?
A close up of the spinning nucleus S. Frauendorf Department of Physics University of Notre Dame, USA IKH, Forschungszentrum Rossendorf Dresden, Germany.
July 29-30, 2010, Dresden 1 Forbidden Beta Transitions in Neutrinoless Double Beta Decay Kazuo Muto Department of Physics, Tokyo Institute of Technology.
Some (more) High(ish)-Spin Nuclear Structure Paddy Regan Department of Physics Univesity of Surrey Guildford, UK Lecture 2 Low-energy.
The Semi-empirical Mass Formula
Shape evolution of highly deformed 75 Kr and projected shell model description Yang Yingchun Shanghai Jiao Tong University Shanghai, August 24, 2009.
Left-handed Nuclei S. Frauendorf Department of Physics University of Notre Dame, USA IKH, Forschungszentrum Rossendorf Dresden, Germany.
Symmetries of the Cranked Mean Field S. Frauendorf Department of Physics University of Notre Dame USA IKH, Forschungszentrum Rossendorf, Dresden Germany.
The i 13/2 Proton and j 15/2 Neutron Orbital and the SD Band in A~190 Region Xiao-tao He En-guang Zhao En-guang Zhao Institute of Theoretical Physics,
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.
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.
g-ray spectroscopy of the sd-shell hypernuclei
How do nuclei rotate? 3. The rotating mean field.
Nordita Workshop on chiral bands /04/2015 Multiple chiral bands associated with the same strongly asymmetric many- particle nucleon configuration.
Dimitar Tonev, Institute for Nuclear Research and Nuclear Energy, Bulgarian Academy of Sciences Lifetime measurements in mass regions A=100 and A=130 as.
Chiral Symmetry Symposium Beijing 2013 Uniwersytet Warszawski Phase transition into spontaneous chiral symmetry breaking Ernest Grodner The Seventh Symposium.
Rotational energy term in the empirical formula for the yrast energies in even-even nuclei Eunja Ha and S. W. Hong Department of Physics, Sungkyunkwan.
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.
A microscopic investigation on magnetic and antimagnetic rotations in 110 Cd Jing Peng Beijing Normal University Collaborators:P.W.Zhao, Jie Meng, and.
Determining Reduced Transition Probabilities for 152 ≤ A ≤ 248 Nuclei using Interacting Boson Approximation (IBA-1) Model By Dr. Sardool Singh Ghumman.
oblate prolate l=2 a20≠0, a2±1= a2±2= 0 Shape parameterization
20/30.
DSAM lifetime measurements in 194Tl
PHL424: Nuclear rotation.
CHEM 312 Lecture 8: Nuclear Force, Structure and Models
Nuclear Chemistry CHEM 396 Chapter 4, Part B Dr. Ahmad Hamaed
Lecture 5-6 xxxxxxx.
2Joint Institute for Nuclear Research, Dubna , Russia
Nuclear Physics, JU, Second Semester,
Rotational Spectroscopy
Quest for chirality in 107Ag
Nuclei at the Extremes of Spin: The Superdeformed Bands in 131,132Ce
20/30.
Shape-coexistence enhanced by multi-quasiparticle excitations in A~190 mass region 石跃 北京大学 导师:许甫荣教授
II. Spontaneous symmetry breaking
How do nuclei rotate? 1. The molecular picture.
Presentation transcript:

Electromagnetic Properties of Nuclear Chiral Partners

For triaxial odd-odd nuclei The Master Equation For triaxial odd-odd nuclei Chirality = Nilsson model + irrotational flow moment of inertia b E [MeV]

Valence nucleons behave as gyroscopes. Pairing interactions couple single particle states to Cooper pairs with no net angular momentum. Valence odd nucleons are unpaired. The properties of valence nucleons can be derived from the Nilsson model

HSM = V(r) +VLS (r) L  S  +L2 +L  S Nuclear single-particle shell model states. HSM = V(r) +VLS (r) L  S 2 8 20 40 70 112 50 82 126 Spher. Harm. Oscillator +L2 +L  S  N=0 N=1 N=2 N=3 N=4 N=5 h11/2 

Unique parity h11/2 state in quadrupole-deformed triaxial potential. HSM = Unique parity h11/2 state in quadrupole-deformed triaxial potential. H= HSM+ Hdef Triaxial shape for b = 0.3, g = 30º. Hdef= kb [ cos(g)Y20(q,f)+ 1/2sin (g){Y22(q,f)+ Y2-2(q,f)}] js =0.00  s =1.36 ji =0.00  i =2.01  jl =5.46  l =0.30 js =5.46  s =0.30 ji =0.00  i =2.01  jl =0.00  l =1.36

j2=jx2+jy2+jz2 E - EF = k ( jx2 - jy2) E < EF E > EF Semi classical analysis for single-particle Nilsson hamiltonian in a triaxial nucleus. j2=jx2+jy2+jz2 E - EF = k ( jx2 - jy2) E < EF E > EF

Collective nuclear rotation resembles that of irrotational liquid but is different than that of a rigid body. In particular moments of inertia differ significantly. laboratory intrinsic irrotational liquid rigid body

Angular momentum for rotating triaxial body with irrotational flow moment of inertia aligns along intermediate axis. J[ħ2/MeV]

Triaxial odd-odd nuclei result in three perpendicular angular momenta for particle-hole configurations built on high-j orbitals .

Results of the Gammasphere GS2K009 experiment. band 2 band 1 134Pr ph11/2 nh11/2

Systematics of partner bands in odd-odd A~130 nuclei. Spin [ħ] 134Pr 136Pm 138Eu 132La 130Cs 132Pr 130La 128Cs 134La 132Cs Energy [MeV] Systematics of partner bands in odd-odd A~130 nuclei.

Chirality is a general phenomenon in triaxial nuclei: two mass regions identified up to date, partner bands in odd-odd and odd-A nuclei.

General electromagnetic properties of chiral partners. long Int short jp jn R I+1 I+2 I

General particle plus triaxial rotor model H = Vsp + Hrot Vsp (b,g,q,f) Hrot Moment of inertia: k =1,2,3 Model for odd-odd nuclei follows the model developed for odd-A nuclei by J. Meyer-ter-Vehn in Nucl. Phys. A249 (1975) 111 The model discussion. The starting point is rather general. The total hamiltonian consists of single particle part and rotor part. The single particle term is quadrupole deformed mean field with its shape parameterized by beta and gamma. The rotor contribution can be expressed with moment of inertia and the core rotation which is the total minus the single particle angular momenta. For the moment of inertia we consider an irrotational-flow type. The formalism developed for odd-A nuclei is followed in the current study for odd-odd case, and details can be referred to the paper by Meyer-Ter-Vehn.

A useful limit of the particle rotor model for triaxial nuclei For irrotational flow moment of inertia there are two special cases for which two out of three moments are equal: axial symmetry for g=0º (prolate shapes) Js=Ji=J0 Jl=0 for g=60º (oblate shapes) Jl=Ji=J0 Js=0 triaxiality for g=30º (triaxial shapes) Jl=Js=J0 Ji=4J0. J[ħ2/MeV]

Symmetric rotor with a triaxial shape at g=90 o l2<l3<l1, but J1=J2=1/4J3 , Q20=0, Q22 =Q2-2 ~b at g=90 o Intermediate axis is an effective symmetry axis of the core, a good choice for the quantization axis. Core rotation orients along the intermediate axis to minimize the rotational energy. g=30 3 1 2 g=90

Calculated Level Scheme B2 B1

Energy vs Spin: two pairs of degenerate bands

Calculated B(M1) and B(E2)

Particle-rotor Hamiltonian for triaxial odd-odd nuclei Core Single proton-particle in j (=h11/2 ) shell Single neutron-particle in j (=h11/2 ) shell

Quantum Number A: invariance properties of H=Hrot+V p+V n D2 symmetry → R3 = 0,±2,±4,±6,….. Invariant under the operation A consisting of Rotation or R3(p/2) [1→2,2→-1,3→3], R3(3p/2) [1→-2,2→-1,3→3] Exchange symmetry between valence proton and neutron C: p↔n C= +1 symmetric C= -1 anti-symmetric

Quantum number A and selection rules for transition rates [H,A]=0 A2=1 Quantum number A=±1 A=+1 R3=0,±4,±8,… & C=+1 R3=±2,±6,±10 …& C=-1 A=-1 R3=0,±4,±8,… & C=-1 R3=±2,±6,±10 …& C=+1 B(E2;Ii→If )≠0 for Ai ≠ Af Core contribution only ⇔ ΔC=0 Q20=0 for γ=90º [B(M1;Ii→If ) with Ai≠Af ] >> [B(M1;Ii→If ) with Ai=Af ] |ΔR3 |≤1 B(M1;Ii→If ) ≈0 for Ci=Cf due to the isovector character of M1 operator gl+gR =0.5 (-0.5) gseff-gR=2.848 (-2.792) for p (n)

Electromagnetic properties of chiral partners with A symmetry where +1 -1 I+4 I+3 I+2 I+1 I

Chiral fingerprints in triaxial odd-odd nuclei: near degenerate doublet D I=1 bands for a range of spin I ; S(I)=[E(I)-E(I-1)]/2I independent of spin I; chiral symmetry restoration selection rules for M1 and E2 transitions vs. spin resulting in staggering of the absolute and relative transition strengths.

Based on the above fingerprints 104Rh provides the best example of chiral bands observed up to date. doubling of states S(I) independent of I B(M1), B(E2) staggering C. Vaman et al. PRL 92(2004)032501

Electromagnetic properties – pronounced staggering in experimental B(M1)/B(E2) and B(M1)in / B(M1)out ratios as a function of spin [T.Koike et al. PRC 67 (2003) 044319 ].

Electromagnetic properties – unexpected B(M1)/B(E2) behavior for 134Pr and heavier N=75 isotones.

Absolute transition rates measurements in A~130 nuclei J. Srebrny et al, Acta Phys. Polonica B46(2005)1063 E. Grodner et al, Int. J. Mod. Phys. E14(2005) 347

Conclusions and future Electromagnetic properties of nuclear chiral partners in triaxial odd-odd nuclei have been identified from a symmetry of a particle-rotor Hamiltonian. A simple ( but limited ) model has been developed which describes uniquely triaxial features with a new quantum number A: Chiral doublet bands, Selection rules for electromagnetic transitions, Chiral wobbling mode. Model predictions are not consistent with the experimental absolute transition rate measurements reported in the mass 130 region. Absolute lifetime measurements are of crucial importance for chiral partner identification and investigation of doublet bands in odd-odd nuclei.

Credits T. Koike I. Hamamoto C.Vaman for 128Cs and 130La DSAM results Tohoku University, Sendai, Japan I. Hamamoto LTH, University of Lund, Sweden and NBI, Copenhagen, Denmark C.Vaman National Superconducting Cyclotron Laboratory Michigan State University, USA for 128Cs and 130La DSAM results E. Groedner, J. Srebrny et. al. Institute of Experimental Physics Warsaw University, Poland