ROLE OF THE NON-AXIAL OCTUPOLE DEFORMATION IN THE POTENTIAL ENERGY OF HEAVY AND SUPERHEAVY NUCLEI XVI NUCLEAR PHYSICS WORKSHOP Kazimierz Dolny 23. – 27.09.2009.

Slides:



Advertisements
Similar presentations
Description of heavy nuclei masses by macro-micro models 1. Coworkers: Yu. Litvinov, A. Parkhomenko 2. Introduction 3. Considered models 4. Accuracy of.
Advertisements

Properties of super-heavy elements in Hartree-Fock-Bogolubov model with the Gogny force. M. Warda Katedra Fizyki Teoretycznej, Uniwersytet Marii Curie-Skłodowskiej,
CoulEx. W. Udo Schröder, 2012 Shell Models 2 Systematic Changes in Nuclear Shapes Møller, Nix, Myers, Swiatecki, Report LBL 1993: Calculations fit to.
On Condensation Force of TSC Akito Takahashi and Norio Yabuuchi High Scientific Research Laboratory Tsu-city Japan.
Nuclear “Pasta” in Compact Stars Hidetaka Sonoda University of Tokyo Theoretical Astrophysics Group Collaborators (G. Watanabe, K. Sato, K. Yasuoka, T.
Pavel Stránský 29 th August 2011 W HAT DRIVES NUCLEI TO BE PROLATE? Instituto de Ciencias Nucleares, Universidad Nacional Autónoma de México Alejandro.
1.Introduction 2.Exotic properties of K nuclei 3.To go forward (Future plan) 4.Summary Dense K nuclei - To go forward - KEK Nuclear KEK, ’06.Aug.3.
The Dynamical Deformation in Heavy Ion Collisions Junqing Li Institute of Modern Physics, CAS School of Nuclear Science and Technology, Lanzhou University.
Search for Triaxial Deformation in Neutron-Rich Mo/Ru Nuclei Daryl Hartley US Naval Academy Support from the National Science Foundation is Gratefully.
IS THE NUCLEAR LARGE AMPLITUDE COLLECTIVE DYNAMICS ADIABATIC OR NON ADIABATIC ? W. Brodziński, M. Kowal, J. Skalski National Centre for Nuclear Research(Warsaw)
Tidal Waves and Spatial Symmetry Daniel Almehed Stefan Frauendorf Yongquin Gu.
Secondary Minima and Non-axial Saddles in Superheavy (Z around 120) Introduction Method ot the analysis Deformation space Results Summary P. Jachimowicz,
Fusion-Fission Dynamics for Super-Heavy Elements Bülent Yılmaz 1,2 and David Boilley 1,3 Fission of Atomic Nuclei Super-Heavy Elements (SHE) Measurement.
Superdeformed oblate superheavy nuclei - mean field results 1.Introduction – some features of exotic shapes 2.Decay modes & possibility of K-isomers 3.Selfconsistent.
9/28/ :01 (00) PAIRING PROPERTIES OF SUPERHEAVY NUCLEI A. Staszczak, J. Dobaczewski and W. Nazarewicz (KFT UMCS) (IFT UW) (ORNL & UT)
Description of α-decay of heavy and superheavy nuclei A. Sobiczewski and A. Parkhomenko Sołtan Institute for Nuclear Studies, Warsaw XII Nuclear Physics.
One-qusiparticle excitations of the heavy and superheavy nuclei A. Parkhomenko and and A.Sobiczewski Institute for Nuclear Studies, ul. Hoża 69, Warsaw.
Fission potential energy surfaces in ten-dimensional deformation space. Vitaly Pashkevich Joint Institute for Nuclear Research. Dubna, Russia Yuri Pyatkov.
Effect of non-axial deformations of higher multipolarity on the fission-barrier height of heavy and superheavy nuclei I. Introduction II. Method of the.
Fission barriers of heavy and superheavy nuclei analyzed in multidimensional deformation space I.Introduction II.Method III.Deformation space IV.Results.
University of Brighton 30 March 2004RISING stopped beam physics workshop Microsecond isomers in A~110 nuclei Few nuclei have oblate ground states (~86%
Single particle properties of heavy and superheavy nuclei. Aleksander Parkhomenko.
Oscillations in mass asymmetry in second and third minima in actinides 1. Second & third minima in actinides 2. Barrier calculations: Micro-macro vs. selfconsistent.
Nuclear Low-lying Spectrum and Quantum Phase Transition Zhipan Li School of Physical Science and Technology Southwest University 17th Nuclear Physics Workshop,
SH nuclei – structure, limits of stability & high-K ground-states/isomers 1.Equilibrium shapes 2.Fission barriers 3.Q alpha of Z= ( with odd and.
SUPERDEFORMED OBLATE SUPERHEAVY NUCLEI ? SDO minima Stability of SDO nuclei K-isomerism Discussion Summary P. Jachimowicz, M. Kowal, J. Skalski.
The National Superconducting Cyclotron State University Betty Tsang, 2/24-26/2005 INFN Workshop on Reactions and Structure with Exotic.
Non-axial hexadecapole deformations of heaviest nuclei M. Kowal, A. Sobiczewski Soltan Institute for Nuclear Studies, Warsaw, Poland Method of the calculations.
Description of experimental fission barriers of heavy nuclei I.Introduction II.Experimental barriers III.Method of description IV.Deformation space V.Results.
Saddle-point shapes of heavy and superheavy nuclei M. Kowal, L. Shvedov and A. Sobiczewski Sołtan Institute for Nuclear Studies, Warsaw XIV Nuclear Physics.
The stability of triaxial superdeformed shape in odd-odd Lu isotopes Tu Ya.
Structures of Exotic 131,133 Sn Isotopes for r-process nucleosynthesis Shisheng Zhang 1,2 ( 张时声 ) 1. School of Physics and Nuclear Energy Engineering,
Mean-Field Description of Heavy Neutron-Rich Nuclei P. D. Stevenson University of Surrey NUSTAR Neutron-Rich Minischool Surrey, 2005.
Kazimierz 2011 T. Cap, M. Kowal, K. Siwek-Wilczyńska, A. Sobiczewski, J. Wilczyński Predictions of the FBD model for the synthesis cross sections of Z.
Nuclear deformation in deep inelastic collisions of U + U.
Isospin mixing and parity- violating electron scattering O. Moreno, P. Sarriguren, E. Moya de Guerra and J. M. Udías (IEM-CSIC Madrid and UCM Madrid) T.
ESNT Saclay February 2, Structure properties of even-even actinides at normal- and super-deformed shapes J.P. Delaroche, M. Girod, H. Goutte, J.
Comparison of the energy levels of an infinite and finite potential well Infinite well number of bound states is infinite Finite well number of bound states.
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.
Ning Wang An improved nuclear mass formula Guangxi Normal University, Guilin, China KITPC , Beijing.
Quantum Phase Transitions (QPT) in Finite Nuclei R. F. Casten June 21, 2010, CERN/ISOLDE.
Shell structure: ~ 1 MeV Quantum phase transitions: ~ 100s keV Collective effects: ~ 100s keV Interaction filters: ~ keV Binding energies, Separation.
WHY ARE NUCLEI PROLATE:
Symmetries of the Cranked Mean Field S. Frauendorf Department of Physics University of Notre Dame USA IKH, Forschungszentrum Rossendorf, Dresden Germany.
F. C HAPPERT N. P ILLET, M. G IROD AND J.-F. B ERGER CEA, DAM, DIF THE D2 GOGNY INTERACTION F. C HAPPERT ET AL., P HYS. R EV. C 91, (2015)
Slide 1 of Woonyoung So International Workshop on e-Science for Physics 2008 Extended Optical Model Analyses for the 9 Be+ 144 Sm System.
Quantum phase transitions and structural evolution in nuclei.
Atomic Orbitals – Class Warmup Determine whether each of the following statements is true or false. If it is false, explain what is wrong with the statement.
Global fitting of pairing density functional; the isoscalar-density dependence revisited Masayuki YAMAGAMI (University of Aizu) Motivation Construction.
Quantum Phase Transition from Spherical to γ-unstable for Bose-Fermi System Mahmut Böyükata Kırıkkale University Turkey collabration with Padova–Sevilla.
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.
Pairing Correlation in neutron-rich nuclei
Nuclear structure of lowest 229Th states
Zao-Chun Gao(高早春) China Institute of Atomic Energy Mihai Horoi
Structure and dynamics from the time-dependent Hartree-Fock model
Emmanuel Clément IN2P3/GANIL – Caen France
An isospin-dependent global elastic nucleon-nucleus potential
Triple-Humped Fission Barrier and Clusterization in the Actinide Region A. Krasznahorkay Inst. of Nucl. Res. of the Hungarian Acad. of Sci. (ATOMKI) Debrecen,
Molecular Geometries and Bonding Theories
Introduction Calculations for the N=7 isotones Summary
Flerov Laboratory of Nuclear Reactions, JINR, Dubna, Russia
Single particle states
Symmetry energy coefficients and shell gaps from nuclear masses
Superheavy nuclei: relativistic mean field outlook
Flerov Laboratory of Nuclear Reactions, JINR, Dubna, Russia
Flerov Laboratory of Nuclear Reactions, JINR, Dubna, Russia
Multidimensional fission barriers for heavy and superheavy nuclei
An improved nuclear mass formula
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
Magnetic dipole excitation and its sum rule for valence nucleon pair
Presentation transcript:

ROLE OF THE NON-AXIAL OCTUPOLE DEFORMATION IN THE POTENTIAL ENERGY OF HEAVY AND SUPERHEAVY NUCLEI XVI NUCLEAR PHYSICS WORKSHOP Kazimierz Dolny 23. – PIOTR JACHIMOWICZ, MICHAŁ KOWAL, PIOTR ROZMEJ, JANUSZ SKALSKI, ADAM SOBICZEWSKI

● Introduction ● Introduction ● Method of calculations ● Method of calculations ● More about motivation ● More about motivation ● Results and discussion ● Results and discussion ○ Ground – state energy ○ Ground – state energy ○ Potential – energy surfaces ○ Potential – energy surfaces ● Conclusions ● Conclusions Plan of the presentation :

Motivation : a 32 (Y Y 3 -2 ) a 32 (Y Y 3 -2 ) ● The importance of nonaxial octupole (tetrahedral) deformation in atomic nuclei was (tetrahedral) deformation in atomic nuclei was suggested some time ago (J. Dudek et al.). suggested some time ago (J. Dudek et al.). ● One searches for local (global) minima with large (or sizable) a 32 on total energy surfaces. large (or sizable) a 32 on total energy surfaces.

Macroscopic-microscopic approach: Macroscopic-microscopic approach: E = E tot ( β λ µ ) – E MACRO ( β λ µ = 0) E = E tot ( β λ µ ) – E MACRO ( β λ µ = 0) E MACRO ( β λ µ )+ E MICRO ( β λ µ ) ○ E MACRO ( β λ µ ) = Yukawa + exp Method of the calculation : ○ E MICRO (β λ µ ) = Woods – Saxon + pairing BCS ○ E MICRO (β λ µ ) = Woods – Saxon + pairing BCS

○ We studied energy vs. a 32 (a one-dimensional calculation) ○ E def = E(0) – E(a 32 ) Our try from one year ago : (a 32 ) ○ values of deformation a 32

○ We studied energy vs. a 32 (a one-dimensional calculation) ○ E def = E(0) – E(a 32 ) (a 32 ) ○ values of deformation a 32 Our try from one year ago :

○ E def = E MICRO (0) – E MICRO (a 32 ) E def = E def + E def MICROMACRO MICRO ○ E def = E MACRO (0) – E MACRO (a 32 ) MACRO (a 32 )

Now we include many deformations trying to answer the following: ● Does a tetrahedral (a 32 ) effect survive competition with other deformations competition with other deformations in heavy and superheavy nuclei ? in heavy and superheavy nuclei ? ● How large is the effect of a 32 on the potential – energy surfaces on top potential – energy surfaces on top of the axial deformations β 2 … β 8 ? of the axial deformations β 2 … β 8 ?

E def is much larger than E def ○ One can suspect that the deformations {β λ }, will strongly decrase or even eliminate the effect of a 32. Results : ○ E def = E(0) – E GS (β λ ) ○ E def = E(0) – E min (a 32 ) (β2…β8)(β2…β8)(β2…β8)(β2…β8) (a 32 ) (β2…β8)(β2…β8)(β2…β8)(β2…β8)

○ E def = E(0) – E min (a 32 ) (a 32 ) ○ E def = E(0) – E GS (β λ ) (β2…β8)(β2…β8)(β2…β8)(β2…β8) (a 32 ) Results : (β2…β8)(β2…β8)(β2…β8)(β2…β8) E def is much larger than E def ○ One can suspect that the deformations {β λ }, will strongly decrase or even eliminate the effect of a 32.

○ The GS energies obtained from the minimization in the 8-dimensional deformation space {a 32,β 2, …, β 8 } ○ E def = E(0) – E GS (a 32, β λ ) (a 32, β 2 …β 8 ) ○ values of deformation a 32 Results :

○ E def = E(0) – E(a 32, β λ ) (a 32, β 2 …β 8 ) ○ values of deformation a 32 Results : ○ The GS energies obtained from the minimization in the 8-dimensional deformation space {a 32,β 2, …, β 8 }

Results : ○ The map from the 6-dimensional minimization over {β 3, …, β 8 } at each point

○ The map from the 6-dimensional minimization over {β 3, …, β 8 } at each point Results :

○ E def = E(0) – E(a 32 ) Preliminary results in the region Z ≥110, N ≥146 : (a 32 ) ○ values of deformation a 32 ○ first the one-dimensional calculation:

○ E def = E(0) – E(a 32 ) ○ values of deformation a 32 (a 32 ) Preliminary results in the region Z ≥110, N ≥146 : ○ first the one-dimensional calculation:

○ E def = E MICRO (0) – E MICRO (a 32 ) ○ E def = E MACRO (0) – E MACRO (a 32 ) MICROMACRO Energy decomposition into micro and macro parts: E def = E def + E def (a 32 ) MICROMACRO

E def is larger than E def (β2…β8)(β2…β8)(β2…β8)(β2…β8) ○ E def = E(0) – E GS (β λ ) (β2…β8)(β2…β8)(β2…β8)(β2…β8) ○ E def = E(0) – E min (a 32 ) (a 32 ) Comparison between effects of (β 2 … β 8 ) and a 32 alone (a 32 )

E def is larger than E def (β2…β8)(β2…β8)(β2…β8)(β2…β8) (a 32 ) ○ E def = E(0) – E min (a 32 ) (a 32 ) ○ E def = E(0) – E GS (β λ ) (β2…β8)(β2…β8)(β2…β8)(β2…β8) Comparison between effects of (β 2 … β 8 ) and a 32 alone

○ The map from the 6-dimensional minimization over {β 3, …, β 8 } at each point

Conclusions : ● Deformation a 32 significantly lowers energy of some heavy nuclei with respect to the energy at some heavy nuclei with respect to the energy at the spherical shape. the spherical shape. ● Since these nuclei are strongly deformed with E def ≈ 8 MeV, the a 32 efect manifests itself mostly as E def ≈ 8 MeV, the a 32 efect manifests itself mostly as a local minimum in the energy surface, appearing a local minimum in the energy surface, appearing high above the global minimum. high above the global minimum. ● Around 228 Fm we can find global minima with a 32, but those minima are very shallow. but those minima are very shallow. ● In the superheavy region we didn't find any global a 32 minimum, a 32 minimum, BUT: one has to note that a 32 was the only nonaxial BUT: one has to note that a 32 was the only nonaxial deformation included. deformation included.