1 Properties of hypernuclei in the Skyrme Hartree-Fock method Xian-Rong Zhou Department of physics, Xiamen University, Xiamen, China Present Status of.

Slides:



Advertisements
Similar presentations
CoulEx. W. Udo Schröder, 2012 Shell Models 2 Systematic Changes in Nuclear Shapes Møller, Nix, Myers, Swiatecki, Report LBL 1993: Calculations fit to.
Advertisements

Structure of  hypernuclei with the antisymmetrized molecular dynamics method Masahiro Isaka (RIKEN)
Testing isospin-symmetry breaking and mapping the proton drip-line with Lanzhou facilities Yang Sun Shanghai Jiao Tong University, China SIAP, Jan.10,
Isospin dependence and effective forces of the Relativistic Mean Field Model Georgios A. Lalazissis Aristotle University of Thessaloniki, Greece Georgios.
Possible existence of neutral hyper-nucleus with strangeness -2 and its production SPN 2014, Changsha, Dec , 2014 Institute of High Energy Physics.
12 June, 2006Istanbul, part I1 Mean Field Methods for Nuclear Structure Part 1: Ground State Properties: Hartree-Fock and Hartree-Fock- Bogoliubov Approaches.
Pavel Stránský 29 th August 2011 W HAT DRIVES NUCLEI TO BE PROLATE? Instituto de Ciencias Nucleares, Universidad Nacional Autónoma de México Alejandro.
Finite Nuclei and Nuclear Matter in Relativistic Hartree-Fock Approach Long Wenhui 1,2, Nguyen Van Giai 2, Meng Jie 1 1 School of Physics, Peking University,
F. Minato A, S. Chiba A, K. Hagino B A. Japan Atomic Energy Agency B. Tohoku Univ. Fission barrier of uranium including Λ hyperon Nucl.Phys.A831, 150 (2009)Nucl.
Projected-shell-model study for the structure of transfermium nuclei Yang Sun Shanghai Jiao Tong University Beijing, June 9, 2009.
Shan-Gui Zhou URL: 1.Institute of Theoretical Physics,
Single Particle Energies
The ground state structure and alpha decay of Hs super- heavy isotopes Junqing Li (Institute of Modern Physics, CAS,Lanzhou) KITPC-CAS Relativistic many-body.
Terminating states as a unique laboratory for testing nuclear energy density functional Maciej Zalewski, UW under supervision of W. Satuła Kazimierz Dolny,
NUCLEAR STRUCTURE PHENOMENOLOGICAL MODELS
Structure of Be hyper-isotopes Masahiro ISAKA (RIKEN) Collaborators: H. Homma and M. Kimura (Hokkaido University)
The stability of triaxial superdeformed shape in odd-odd Lu isotopes Tu Ya.
The first systematic study of the ground-state properties of finite nuclei in the relativistic mean field model Lisheng Geng Research Center for Nuclear.
Higher-Order Effects on the Incompressibility of Isospin Asymmetric Nuclear Matter Lie-Wen Chen ( 陈列文 ) (Institute of Nuclear, Particle, Astronomy, and.
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,
Ning Wang 1, Min Liu 1, Xi-Zhen Wu 2, Jie Meng 3 Isospin effects in nuclear mass models Nuclear Structure and Related Topics (NSRT15), , DUBNA.
L. R. Dai (Department of Physics, Liaoning Normal University) Z.Y. Zhang, Y.W. Yu (Institute of High Energy Physics, Beijing, China) Nucleon-nucleon interaction.
XII Nuclear Physics Workshop Maria and Pierre Curie: Nuclear Structure Physics and Low-Energy Reactions, Sept , Kazimierz Dolny, Poland Self-Consistent.
1 New formulation of the Interacting Boson Model and the structure of exotic nuclei 10 th International Spring Seminar on Nuclear Physics Vietri sul Mare,
Effects of self-consistence violations in HF based RPA calculations for giant resonances Shalom Shlomo Texas A&M University.
Three- and four-body structure of S=-2 hypernuclei E. Hiyama (Nara Women’s Univ.)
Alex Brown UNEDF Feb Strategies for extracting optimal effective Hamiltonians for CI and Skyrme EDF applications.
Chirality of Nuclear Rotation S. Frauendorf Department of Physics University of Notre Dame, USA IKH, Forschungszentrum Rossendorf Dresden, Germany.
HYPERNUCLEAR PHYSICS Hypernuclei are bound states of nucleons with a strange baryon (  hyperon). Extension of physics on N-N interaction to system with.
H. Lenske Institut für Theoretische Physik, U. Giessen Aspects of SU(3) Flavor Physics In-medium Baryon Interactions Covariant Density Functional Theory.
Ning Wang 1, Min Liu 1, Xi-Zhen Wu 2, Jie Meng 3 Isospin effect in Weizsaecker-Skyrme mass formula ISPUN14, , Ho Chi Minh City 1 Guangxi Normal.
1 Skyrme Hartree-Fock 理论 对奇异性原子核性质的研究 周先荣 厦门大学物理系 ,第十四届全国核结构大会,湖州.
1 11/20/ /10/2014 Jinniu Hu Stellar neutrino emission at finite temperature in relativistic mean field theory Jinniu Hu School of Physics, Nankai.
Mean-Field Description of Heavy Neutron-Rich Nuclei P. D. Stevenson University of Surrey NUSTAR Neutron-Rich Minischool Surrey, 2005.
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.
Cross section of elementally process [5] The  -ray spectroscopy of light hypernuclei at J-PARC (E13) K. Shirotori for the Hyperball-J collaboration Department.
Recent Studies of Hypernuclei Formation with Electron Beams at MAMI Patrick Achenbach U Mainz Sept. 2o13.
Coupling of (deformed) core and weakly bound neutron M. Kimura (Hokkaido Univ.)
Relativistic mean field and RPA with negative energy states for finite nuclei Akihiro Haga, Hiroshi Toki, Setsuo Tamenaga, Yoko Ogawa, Research Center.
Trento, Giessen-BUU: recent progress T. Gaitanos (JLU-Giessen) Model outline Relativistic transport (GiBUU) (briefly) The transport Eq. in relativistic.
M. Matsuo, PRC73(’06) Matter Calc. Two-particle density.
Structure of neutron-rich Λ hypernuclei E. Hiyama (RIKEN)
Auxiliary Field Diffusion Monte Carlo study of symmetric nuclear matter S. Gandolfi Dipartimento di Fisica and INFN, Università di Trento I Povo,
Erosion of N=28 Shell Gap and Triple Shape Coexistence in the vicinity of 44 S M. KIMURA (HOKKAIDO UNIV.) Y. TANIGUCHI (RIKEN), Y. KANADA-EN’YO(KYOTO UNIV.)
ShuangQuan Zhang School of Physics, Peking University Static chirality and chiral vibration of atomic nucleus in particle rotor model.
NEUTRON SKIN AND GIANT RESONANCES Shalom Shlomo Cyclotron Institute Texas A&M University.
Lecture 23: Applications of the Shell Model 27/11/ Generic pattern of single particle states solved in a Woods-Saxon (rounded square well)
Deformations of sd and pf shell  hypernuclei with antisymmetrized molecular dynamics Masahiro Isaka (RIKEN)
Studies of hypernuclei with the AMD method Masahiro ISAKA Institute of Physical and Chemical Research (RIKEN) Focusing on 25  Mg, based on M. Isaka, M.
Three-body force effect on the properties of asymmetric nuclear matter Wei Zuo Institute of Modern Physics, Lanzhou, China.
July 29-30, 2010, Dresden 1 Forbidden Beta Transitions in Neutrinoless Double Beta Decay Kazuo Muto Department of Physics, Tokyo Institute of Technology.
Effect of tensor on halo and subshell structure in Ne, O and Mg isotopes Chen Qiu Supervisor: Prof. Xian-rong Zhou Xiamen University April. 13, 2012.
Evolution Of Shell Structure, Shapes & Collective Modes Dario Vretenar
WHY ARE NUCLEI PROLATE:
第十四届全国核结构大会暨第十次全国核结构专题讨论会
Weak decay of  in nuclear medium FCPPL-2015, USTC, April 8-12, 2015 Institute of High Energy Physics Qiang Zhao Institute of High Energy Physics, CAS.
Left-handed Nuclei S. Frauendorf Department of Physics University of Notre Dame, USA IKH, Forschungszentrum Rossendorf Dresden, Germany.
PKU-CUSTIPEN 2015 Dirac Brueckner Hartree Fock and beyond Herbert Müther Institute of Theoretical Physics.
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,
Structure of light Λ hypernuclei Emiko Hiyama (RIKEN)
1 11/20/13 21/11/2015 Jinniu Hu School of Physics, Nankai University Workshop on “Chiral forces and ab initio calculations” Nov. 20- Nov. 22,
g-ray spectroscopy of the sd-shell hypernuclei
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.
Relativistic EOS for Supernova Simulations
Pairing Correlation in neutron-rich nuclei
LI ANG 李 昂 Shape evolution of Ne isotopes and Ne hypernuclei: The interplay of pairing and tensor interactions LI ANG 李 昂
Masahiro Isaka (RIKEN)
Zao-Chun Gao(高早春) China Institute of Atomic Energy Mihai Horoi
Impurity effects in p-sd shell and neutron-rich L hypernuclei
Effects of the φ-meson on the hyperon production in the hyperon star
Presentation transcript:

1 Properties of hypernuclei in the Skyrme Hartree-Fock method Xian-Rong Zhou Department of physics, Xiamen University, Xiamen, China Present Status of the Nuclear Interaction Theory, 08/25 -09/19,2014, Beijing, China

2 Outline  Introduction  Extended Skyrme Hartree-Fock  Properties of hypernuclei shapes of hypernuclei effects of hyperon enegery spetrum  Summary

3 N Z ,  Hypernuclei ,  Hypernuclei Strangeness D nuclear chart

4 Multistrange system: Ne utron star, … Why to study hypernuclei? Nucleon-nucleon interaction Hyperon-nucleon interaction Impurity of nuclear system

5 Theoretical studies about hypernuclei Energy spectrum Decay properties The effect of hyperon(s) Shapes …….

6 Studies based on spherical symmetry: 1. Relativistic mean-field model (RMF) 2. Skyrme Hartree-Fock model (SHF) 3. Woods-Saxon potential + YN interaction 4. Few-body theory Theoretical studies about the shapes of hypernuclei

7 Deformed HF with nonrealistic YN interaction: T. H. Ho and A.Volkov, Phys. Lett. B30, 303, W. H. Bassichis, A. Gal, Phys. Rev. C1, 28, J. Zofka, Czech, J. Phys. B30, 95, Nilsson Model: assume the same deformation for core and hypernuclei: K. Hagino, Phys. Rev. C63, , 2001 Calculations considering deformation:

8 Deformed SHF with Microscopic YN int. X.-R. Zhou, H.-J. Schulze, H. Sagawa,et al., Phys. Rev. C76, (2007) Relativistic mean-field model (RMF): Myaing Thi Win, H. Hagino, et al., Phys. Rev. C 78, (2008) Triaxial SHF with Skyrme-like YN interaction: Myaing Thi Win, H. Hagino, et al., Phys. Rev. C 83, (2011) Antisymmetrized molecular dynamics (AMD): M. Isaka,, et al., Phys. Rev. C 83, (2011) Triaxial RMF: Bing-Nan Lu ( 吕炳楠 ), S.-G.Zhou, Phys. Rev. C 84, (2011) Considering deformation self-consistently:

9 Bing-Nan Lu, E. Hiyama, H. Sagawa, and S.-G. Zhou, Phys. Rev. C 89, (2014) Superdeformation in hypernuclei

10 Why to study deformations of hypernuclei Many p-shell and sd-shell nuclei are deformed. For example, experimentally, 10 B and 11 C have large quadrupole moments. F. Ajzenberg-Selove, Nucl. Phys. A490, 1 (1988); A506, 1(1990). Also, 8 Be is known to be strongly deformed due to its double-α structure.

11 Several models for deformed nuclei Alpha-model Projected shell model (PSM) Deformed Skyrme Hartree-Fock (DSHF) Relativistic mean-field model (RMF) Antisymmetrized molecular dynamics (AMD) ……

12 Microscopic hyperon-nucleon interaction for deformed hypernuclei B Y, Hypernuclear Structure Effective YN interaction BHF cal. for asymmetric matter Free YN interaction MF cal. YN: Nijmegen soft-core hyperon-nucleon potential NSC89,NSC97 a,NSC97f,ESC08 NN: Argonne v18 nucleon-nucleon interaction

Comparison of different hyperon-nucleon potential

14 Extended DSHF including hyperon-nucleon interaction Total energy of a hypernucleus in extended DSHF: where the energy density SHF Due to the YN force, DSHF + YN interaction:

The energy density functional ε NΛ is obtained from a fit to the binding energy per baryon, B/A(ρ n, ρ p, ρ), of asymmetric hypermatter, as generated by BHF calculations. Effective mass of hyperon

16 In practice we use the following parametrizations:

17 Extended SHF equation Minimizing the total energy of the hypernucleus, one arrives with extended SHF equation with the modified mean field by hyperon:

18 For light nuclei, For medium-mass and heavy nuclei, Pairing interaction Nucl. Phys. A722, c183, 2003 Euro. Phys. J. A8, 59, 2000 We take a density-dependent delta pairing Nucl. Phys. A551, 434 (1993)

19 1. Hypernuclei is deformed or not?

X.-R. Zhou, H.-J. Schulze, H. sagawa et.al, PRC76, (2007) Binding energies vs deformations

21 Binding energies vs deformations X.-R. Zhou, H.-J. Schulze, H. sagawa et.al, PRC76, (2007)

22 2. The effect of hyperon on nuclear structure?

23 The effect of hyperon in neutron-rich nuclei X.-R. Zhou,A.Polls,H.-J.Schulze, et al.,PRC78,054306(2008)

24 The Oxygen isotopes exp.

25 3. Energy spectrum of hypernulcei

The SHF models can just give the single-particle energies and ground state of Λ hypernuclei in intrinsic frame of reference. The conservation of particle number is destroyed by BCS method. The study of the gamma spectra and electromagnetic transitions needs symmetry restoration. Limitations of extended SHF+BCS method: Angular momentum and particle-number projection (AMP&PNP) are needed !

Projected SHF+BCS Model The projected mean-field state The projection operator Energies with angular momentum and E2 transitions

Energy potential surface of 12 C and Ji-Wei Cui, X.-R. Zhou, in preparation

Energy potential surface of 20 Ne and

Energy potential surface of 24 Mg and

Energy potential surface of 26 Mg and

Energy potential surface of 26 Si and

Energy potential surface of 28 Si and

Comparison of NSC89(upper) and Skyrme-type(lower) ΛN Interactions

Comparison of different Skyrme parameters

Energy spectrum of 12 C and cal1 and cal2 label energy levels with or without the Λ spin-orbit term.

cal1 and cal2 label energy levels with or without the Λ spin-orbit term. Energy spectrum of 20 Ne and

cal1 and cal2 label energy levels with or without the Λ spin-orbit term. Energy spectrum of 24 Mg and

Energy spectrum of 28 Si and cal1 and cal2 label energy levels with or without the Λ spin-orbit term.

Exp data in W.u. from: The B(E2) transitions of hypernuclei become a little smaller due to the shrinkage of the quadruple shape. B(E2) transition probabilities

41 Summary 1.The DSHF was extended to hypernuclei by including a microscopically derived hyperon- nucleon interaction. 3. Due to the effect of hyperons, the nuclei close to the drip line are stabilized and new isotopes are potentially made available. 2.The calculated core nuclei and the corresponding hypernuclei have similar deformations with the same sign when the core nuclei are well deformed. 4. The projected SHF+BCS model gives reasonable initial results of energy spectra and E2 transition rates for well-deformed sd-shell nuclei and hypernuclei.

42 Cooperators H. Sagawa University of Aizu, Japan H.-J. Schulze, University of Catania, Italy En-Guang Zhao Institute of Theoretical Physics, CAS, China Ji-Wei Cui Xiamen University, China

43 Thank you for your attention! Furong Lake Xiamen Univ.