Renormalized Interactions for CI constrained by EDF methods Alex Brown, Angelo Signoracci and Morten Hjorth-Jensen.

Slides:



Advertisements
Similar presentations
The role of the isovector monopole state in Coulomb mixing. N.Auerbach TAU and MSU.
Advertisements

Spectroscopy at the Particle Threshold H. Lenske 1.
COUPLED-CLUSTER CALCULATIONS OF GROUND AND EXCITED STATES OF NUCLEI Marta Włoch, a Jeffrey R. Gour, a and Piotr Piecuch a,b a Department of Chemistry,Michigan.
Testing isospin-symmetry breaking and mapping the proton drip-line with Lanzhou facilities Yang Sun Shanghai Jiao Tong University, China SIAP, Jan.10,
Delta-hole effects on the shell evolution of neutron-rich exotic nuclei Takaharu Otsuka University of Tokyo / RIKEN / MSU Chiral07 Osaka November 12 -
Testing shell model on nuclei
Lawrence Livermore National Laboratory UCRL-XXXX Lawrence Livermore National Laboratory, P. O. Box 808, Livermore, CA This work performed under.
Molecular Quantum Mechanics
What are we doing? Large-scale ab initio No-core Shell Model calculations.
Structure of neutron rich calcium isotopes from coupled cluster theory Gaute Hagen (ORNL) Collaborators: Andreas Ekström (MSU) Christian Forrsen (Chalmers)
Shell Model with residual interactions – mostly 2-particle systems Simple forces, simple physical interpretation.
Semi-magic seniority isomers and the effective interactions
Single Particle Energies
Su Shi Chun. From experiments, we found that nuclei are more tightly bounded  number of protons or neutrons is 2, 8, 20, 28, 50, 82, 126 (Magic numbers).
Terminating states as a unique laboratory for testing nuclear energy density functional Maciej Zalewski, UW under supervision of W. Satuła Kazimierz Dolny,
Masses (Binding energies) and the IBA Extra structure-dependent binding: energy depression of the lowest collective state.
Renormalized Interactions with EDF Single-Particle Basis States
Nucleons & Nuclei a quick guide to the real essentials in the subject which particle and nuclear physicists won’t tell you.
IAEA Workshop on NSDD, Trieste, November 2003 The nuclear shell model P. Van Isacker, GANIL, France Context and assumptions of the model Symmetries of.
Spectroscopic factors and Asymptotic Normalization Coefficients from the Source Term Approach and from (d,p) reactions N.K. Timofeyuk University of Surrey.
Shell-model CI codes and applications Calvin Johnson (1) Plamen Krastev (1,2) * Erich Ormand (2) 1 San Diego State University 2 Lawrence Livermore National.
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,
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.
Alex Brown PREX Aug Neutron Radii and the Neutron Equation of State.
Alex Brown UNEDF Feb Strategies for extracting optimal effective Hamiltonians for CI and Skyrme EDF applications.
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/
Mean-Field Description of Heavy Neutron-Rich Nuclei P. D. Stevenson University of Surrey NUSTAR Neutron-Rich Minischool Surrey, 2005.
Nuclear Models Nuclear force is not yet fully understood.
Trento, Giessen-BUU: recent progress T. Gaitanos (JLU-Giessen) Model outline Relativistic transport (GiBUU) (briefly) The transport Eq. in relativistic.
We construct a relativistic framework which takes into pionic correlations(2p-2h) account seriously from both interests: 1. The role of pions on nuclei.
Auxiliary Field Diffusion Monte Carlo study of symmetric nuclear matter S. Gandolfi Dipartimento di Fisica and INFN, Università di Trento I Povo,
Nuclear Collective Excitation in a Femi-Liquid Model Bao-Xi SUN Beijing University of Technology KITPC, Beijing.
NSDD Workshop, Trieste, February 2006 Nuclear Structure (I) Single-particle models P. Van Isacker, GANIL, France.
Shell Model with residual interactions – mostly 2-particle systems Start with 2-particle system, that is a nucleus „doubly magic + 2“ Consider two identical.
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)
Shell Model with residual interactions – mostly 2-particle systems Simple forces, simple physical interpretation Lecture 2.
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.
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.
Furong Xu (许甫荣) Many-body calculations with realistic and phenomenological nuclear forces Outline I. Nuclear forces II. N 3 LO (LQCD): MBPT, BHF, GSM (resonance.
Effective interactions in shell-model calculations M. Honma (Univ. of Aizu) T. Mizusaki (Senshu Univ.) T. Otsuka (Univ. of Tokyo/RIKEN) B. A. Brown (MSU)
Evolution Of Shell Structure, Shapes & Collective Modes Dario Vretenar
Lawrence Livermore National Laboratory Lattice QCD and Nuclear physics From Pipe Dream to Reality June 22, 2009 Tom Luu Performance Measures x.x, x.x,
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)
PKU-CUSTIPEN 2015 Dirac Brueckner Hartree Fock and beyond Herbert Müther Institute of Theoretical Physics.
Nuclear density functional theory with a semi-contact 3-body interaction Denis Lacroix IPN Orsay Outline Infinite matter Results Energy density function.
Alex Brown, Pack Forest UNEDF 2009 Implementations of NuShellX.
Furong Xu (许甫荣) Nuclear forces and applications to nuclear structure calculations Outline I. Nuclear forces II. N 3 LO (LQCD): MBPT, BHF, GSM (resonance.
Nuclear and Radiation Physics, BAU, 1 st Semester, (Saed Dababneh). 1 The Deuteron Deuterium (atom). The only bound state of two nucleons  simplest.
Variational Multiparticle-Multihole Configuration Mixing Method with the D1S Gogny force INPC2007, Tokyo, 06/06/2007 Nathalie Pillet (CEA Bruyères-le-Châtel,
Cluster-Orbital Shell Model for neutron-lich nuclei Hiroshi MASUI Kitami Institute of Technology Collaborators: Kiyoshi KATO, Hokkaido Univ. Kiyomi IKEDA,
Furong Xu (许甫荣) Many-body correlations in ab-initio methods Outline I. Nuclear forces, Renormalizations (induced correlations) II. N 3 LO (LQCD) MBPT,
Congresso del Dipartimento di Fisica Highlights in Physics –14 October 2005, Dipartimento di Fisica, Università di Milano Contribution to nuclear.
Few-Body Models of Light Nuclei The 8th APCTP-BLTP JINR Joint Workshop June 29 – July 4, 2014, Jeju, Korea S. N. Ershov.
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.
Presented by Building Nuclei from the Ground Up: Nuclear Coupled-cluster Theory David J. Dean Oak Ridge National Laboratory Nuclear Coupled-cluster Collaboration:
Large-Scale Shell-Model Study of the Sn-isotopes
Structure and dynamics from the time-dependent Hartree-Fock model
Exotic nuclei beyond 132Sn: where do we stand?
Coulomb repulsion and Slater Integrals
Nuclear Physics, JU, Second Semester,
Superheavy nuclei: relativistic mean field outlook
UWC Beyond mean-field: present and future
The following slides show you how to treat the Coulomb interaction in a many particle Hamiltonian. As the Coulomb interaction diverges for the case where.
Department of Physics, Sichuan University
Presentation transcript:

Renormalized Interactions for CI constrained by EDF methods Alex Brown, Angelo Signoracci and Morten Hjorth-Jensen

Wick’s theorem for a Closed-shell vacuum filled orbitals

Closed-shell vacuum filled orbitals EDF (Skyrme Phenomenology)

Closed-shell vacuum filled orbitals EDF (Skyrme) phenomenology NN potential with V_lowk

Closed-shell vacuum filled orbitals EDF (Skyrme) phenomenology “tuned” valence two-body matrix elements

Closed-shell vacuum filled orbitals EDF (Skyrme) phenomenology Monopole from EDF

Closed-shell vacuum filled orbitals A 3 A 2 A 1 Monopole from EDF

Aspects of evaluating a microscopic two-body Hamiltonian (N3LO + V lowk + core-polarization) in a spherical EDF (energy- density functional) basis (i.e. Skyrme HF) 1)TBME (two-body matrix elements): Evaluate N3LO + V lowk with radial wave functions obtained with EDF. 2)TBME: Evaluate core-polarization with an underlying single-particle spectrum obtained from EDF. 3)TBME: Calculate monopole corrections from EDF that would implicitly include an effective three-body interaction of the valence nucleons with the core. 4)SPE for CI: Use EDF single-particle energies – unless something better is known experimentally.

Why use energy-density functionals (EDF)? 1)Parameters are global and can be extended to nuclear matter. 2)Effort by several groups to improve the understanding and reliability (predictability) of EDF – in particular the UNEDF SciDAC project in the US. 3)This will involve new and extended functionals. 4)With a goal to connect the values of the EDF parameters to the NN and NNN interactions. 5)At this time we have a reasonably good start with some global parameters – for now I will use Skxmb – Skxm from [ BAB, Phys. Rev. C58, 220 (1998)] with small adjustment for lowest single-particle states in 209 Bi and 209 Pb.

Calculations in a spherical basis with no correlations

What do we get out of (spherical) EDF? 1)Binding energy for the closed shell 2)Radial wave functions in a finite-well (expanded in terms of harmonic oscillator). 3) gives single-particle energies for the nucleons constrained to be in orbital (n l j) a where BE(A) is a doubly closed-shell nucleus. 4) gives the monopole two-body matrix element for nucleons constrained to be in orbitals (n l j) a and (n l j) b

EDF core energy and single- particle energy EDF two-body monopole

Theory (ham) from Skxmb with parameters adjusted to reproduce the energy for the 9/2 - state plus about 100 other global data.

218 U 208 Pb x = experiment CI (ham) N3LO with EDF constraint EDF (or CI) with no correlations CI with N3LO

Skyrme (Skxmb) + V low-k N 3 LO (second order) 210 Po

Skyrme (Skxmb) + V low-k N 3 LO (first order)

213 Fr Skyrme (Skxmb) + V low-k N 3 LO (second order)

214 Ra Skyrme (Skxmb) + V low-k N 3 LO (second order)

EDF core energy and single- particle energy EDF two-body monopole

Theory (ham) from Skxmb with parameters adjusted to reproduce the energy for the 9/2 + state plus about 100 other global data.

Skyrme (Skxmb) + V low-k N 3 LO (second order) 210 Pb

Skyrme (Skxmb) + V low-k N 3 LO (second order) 210 Bi

Skyrme (Skxmb) + V low-k N 3 LO (second order) 212 Po

Skyrme (Skxmb) + V low-k N 3 LO (second order) 210 Pb

Skyrme (Skxmb) + exp spe V low-k N 3 LO (second order) 210 Pb

Skyrme (Skxmb) for 208 Pb (closed shell) + V low-k N 3 LO (second order)

“ab-initio” calculation for absolute energies of 213 Fr

Energy of first excited 2 + states