Shell model description of dipole strength at low energy
|
|
- Rosanna Wells
- 5 years ago
- Views:
Transcription
1 Shell model description of dipole strength at low energy Kamila Sieja Institut Pluridisciplinaire Hubert Curien, Strasbourg Kamila Sieja (IPHC) / 18
2 Overview & Motivation Low energy enhancement of γ-sf E. Litvinova and N. Belov, Phys. Rev. C88 (213) 3132R Thermal continuum QRPA calculations Enhancement due to transitions between thermally unblocked s.p. states and the continuum Note the difference between T = (ground state) and T > (excited state) E1 strength distribution R. Schwengner et al., PRL111 (213) Shell model transitions between a large amount of states Enhancement due to the M1 transitions between states in the region near the quasicontinuum A general mechanism to be found throughout the nuclear chart Kamila Sieja (IPHC) / 18
3 SM calculations in sd pf gds valence space s1/2 d3/2 d5/2 g7/2 g9/2 p1/2 p3/2 f5/2 f7/2 s1/2 d3/2 d5/2 Π 16 O fp 1p-1h 48 Cr Fe ν Full fp-calculations for positive parity states Full 1 hω calculations for negative parity states- all 1p-1h excitations from sd and to gds shells H SM = i ε i c i c i + i,j,k,l V ijkl c i c j c lc k + β c.m. H c.m. 6 states per spin and parity S M1/E1 = B(M1/E1) ρ(e i ) (6 5 iterations...) or Lanczos SF method with 5 iterations for upward S M1/E1 Kamila Sieja (IPHC) / 18
4 Downward and upward strength calculations γ-decay (RSF) calculate desired number of low lying states using standard SM diagonalization techniques obtain the averages and radiative strength functions from relations: photoabsorption (PSF) use Lanczos Strength Function method with a large number of iterations: S = Ô ψ i = ψ i Ô2 ψ i f M1/E1 (E γ )=16π/9( hc) 3 S M1/E1 (E γ ) S M1/E1 = B(M1/E1) ρ i (E i ) The operator Ô does not commute with H and Ô ψ i is not necessarily the eigenstate of the Hamiltonian. But it can be developed in the basis of energy eigenstates: Ô ψ i = S(E f ) E f, f where S(E f )= E f Ô ψ i is microscopic strength function. If we carry Lanczos procedure using O =Ô ψ i as initial vector then H is diagonalized to obtain eigenvalues E f and after N iterations we have also the strength distribution. Kamila Sieja (IPHC) / 18
5 Downward and upward strength calculations γ-decay (RSF) calculate desired number of low lying states using standard SM diagonalization techniques obtain the averages and radiative strength functions from relations: photoabsorption (PSF) use Lanczos Strength Function method with a large number of iterations: S = Ô ψ i = ψ i Ô2 ψ i f M1/E1 (E γ )=16π/9( hc) 3 S M1/E1 (E γ ) S M1/E1 = B(M1/E1) ρ i (E i ) The operator Ô does not commute with H and Ô ψ i is not necessarily the eigenstate of the Hamiltonian. But it can be developed in the basis of energy eigenstates: Ô ψ i = S(E f ) E f, f where S(E f )= E f Ô ψ i is microscopic strength function. If we carry Lanczos procedure using O =Ô ψ i as initial vector then H is diagonalized to obtain eigenvalues E f and after N iterations we have also the strength distribution. Kamila Sieja (IPHC) / 18
6 Large scale shell model framework define valence space H eff Ψ eff = EΨ eff INTERACTIONS CORE build and diagonalize Hamiltonian matrix CODES Strasbourg shell model codes (E. Caurier, RMP77, 25, 427) NATHAN j-coupled basis large number of non-zero ME smaller dimensions tractable good quantum number: J can get many states of the same J used in the present calculations ideal for description of γ-decay downward strength (RSF) ANTOINE m-scheme basis sparse matrices larger dimensions tractable good quantum number: M numerical problems to get many states of the same J used in the present calculations ideal for description of photoabsorption upward strength (PSF) Kamila Sieja (IPHC) / 18
7 Dipole strength in 44 Sc: theory vs exp <B(M1)> (µ Ν 2 ) SM, π + (hω states) SM, π - (1hω states) 44 Sc f 1 (MeV -3 ) 1e-6 1e-7 1e-8 44 Sc EXP SM, E1 SM, M1 SM, E1+M1 <B(M1)> (µ N 2 ) No enhancement of the 1 hω M1 strength due to the complexity of wave functions (comparable to that of deformed nuclei) Ti 5 Ti 54 Ti 48 Cr e all states below S n 1MeV M1 matrix elements E1 matrix elements KS, submitted Kamila Sieja (IPHC) / 18
8 Dipole strength in 44 Sc: E1 part B(E1) (e 2.fm 2 ) J i =-12 +/- J i = Sc E exc (MeV) low energy part: 6567 E1 matrix elements higher energy part: LSF with 5 iterations (J i = 2 + 1,2,3 ) <B(E1)> (e 2.fm 2 ) f E1 (MeV -3 ).1.1 1e-5-5MeV 5-1MeV 44 Sc 8-1MeV -1MeV 1e e-8 2e-8 1e-8-5MeV 5-1MeV 44 Sc 8-1MeV -1MeV Behaviour of the E1 strength at low energy independent on spin range and energy cut-off Kamila Sieja (IPHC) / 18
9 Comparison to other models B(E1) (e 2.fm 2 ) J i =-12 +/- J i = Sc E exc (MeV) f E1 (MeV -3 ) 1e-5 1e-6 1e-7 44 Sc 1e-8 QRPA(Sly4) SM, 2 + SM, 2 +,6 + 1e e-8 Reasonable agreement between QRPA and SM PSF up to 15MeV for higher energies, 3 hω excitations should be included in SM Microscopic SM strength has a non-zero limit for E γ =. Consistent with EGLO model. f E1 (MeV -3 ) 1e-9 44 Sc SM EGLO GFL SLO 1e Kamila Sieja (IPHC) / 18
10 Low energy E1 strength in SM & QRPA models QRPA describes formally photoabsorption from the ground state correction term is added to take into account collisions of quasiparticles: QRPA from S. Goriely, priv. comm. Γ (E)=Γ(E)(1+α 4πT 2 EE GDR ) the upbend of QRPA strength is not consistent with low energy strength from shell model shell model is the only microscopic tool that gives the downward strength Kamila Sieja (IPHC) / 18
11 Downward vs upward strength: E1 RSF E1 (MeV -3 ) 1e-5 1e-6 1e-7 1e-8 1e-9 γ-decay (RSF) 1e photoabsorption (PSF) Ti 1e-5 Ti PSF E1 (MeV -3 ) 1e-6 1e-7 1e-8 1e-9 44 Ti 46 Ti 48 Ti 5 Ti 52 Ti 1e E exc = Decay to all available states adds a broad component to the strength function with a non-zero E γ = limit. 1e-5 upward downward 1e-6 f E1 (MeV -3 ) 1e-7 1e-8 48 Ti RSF=PSF of the g.s. only for higher transition energies 1e Kamila Sieja (IPHC) / 18
12 Downward vs upward strength: M1 RSF M1 (MeV -3 ) 6e-8 5e-8 4e-8 3e-8 2e-8 1e-8 γ-decay (RSF) 44 Ti 46 Ti photoabsorption (PSF) 6e-8 48 Ti PSF M1 (MeV -3 ) 5e-8 4e-8 3e-8 2e-8 1e-8 44 Ti 46 Ti 48 Ti 5 Ti 52 Ti E exc = Decay to all available states can produce an enhancement effect at low energy. Kamila Sieja (IPHC) / 18
13 Impact of the realistic M1 fragmentation on the neutron capture cross sections M1 microscopic strength functions in iron chain ( 53 Fe- 7 Fe) and impact on (n,γ) cross sections f M1 [1-8 MeV -3 ] f M1 [1-8 MeV -3 ] f M1 [1-8 MeV -3 ] J= J=2 + H.-P. Loens K. Langanke, G. Martinez-Pinedo and KS, EPJ A48 (212) 48 E γ [MeV] 68 Fe J=4 + E γ [MeV] 68 Fe E γ [MeV] 68 Fe σ [b] Fe(n,γ) 68 Fe J= + J=2 + J= E n [MeV] Using SF of excited states instead of that of + leads to larger cross sections Kamila Sieja (IPHC) / 18
14 Outlook: A word on shell model calculations SM is a powerful tool that can be used in many mass regions. Nevertheless, to get the proper physics, large valence spaces and time-consuming calculations are necessary. A valence space can be adequate to describe some properties and completely wrong for others: 48 Cr (f 7/2 ) 8 (f 7/2 p 3/2 ) 8 (fp) 8 Q(2 + )(e.fm 2 ) E(4 + )/E(2 + ) B(E2;2 + )(e 2.fm 4 ) B(GT) The GT (magnetic) properties require model spaces that include all spin-orbit partners. Some effects can be incorporated via renormalization of the magnetic operator (quenching), but some other cannot... Kamila Sieja (IPHC) / 18
15 B(M1) in 87 Kr: model space dependence <B(M1)> (µ N 2 ) π +, fpgd (LNPS) π +, pf-gds 87 Kr from V. W. Ingeberg talk fpgd model space: full pf-shell for protons, 2p-2h excitations from p 3/2,f 5/2 to p 1/2,g 9/2,d 5/2 neutron orbits pf gds model space: full pf-shell for protons, 2p-2h excitations from g 9/2 to d 5/2,s 1/2,d 3/2,g 7/2 neutron orbits Kamila Sieja (IPHC) / 18
16 Outlook: M1 strengths and correlations within the model space <B(M1)> (µ N 2 ) full ν=4 46 Ti B(M1; + ->1 + ) (µ N 2 ) Fe, fpgd model space 2p-2h, q=1. 6p-6h, q=.75 8p-8h, q= Not enough correlations too much enhancement, not enough strength at low energy... Kamila Sieja (IPHC) / 18
17 Summary The large-scale shell model can describe both, upward and downward M1/E1/E2... strengths. Employed in model spaces encompassing the necessary degrees of freedom can give a valuable insight into physics mechanisms behind the low-energy behavior of calculated strengths. M1 dipole strength functions show an upbend for the low γ-energies. However, the mixing destroys the enhancement. No enhancement of the 1 hω M1 is present for the same reason. More complexity of the wave function less probability for the upbend. E1 dipole strength functions do not show the low energy upbend. Given the nature of the E1 operator, one can expect no much upbend throughout the nuclear chart to be verified in very neutron-rich nuclei. Shell model E1 strength at low energy exhibits different trend from QRPA approaches with a flat, non-zero E γ = limit. Consistent with EGLO model. Systematic, reliable SM calculations needed to characterize the regions where the enhancement should be present and the evolution of strengths in neutron-rich nuclei. Kamila Sieja (IPHC) / 18
18 Effective Hamiltonian Interaction from V lowk based on the CD-Bonn potential Monopole corrections to fix the s.p. and s.h. energies pf-shell TBME from the LNPS fit (PRC82, 5431, 21) Good reproduction of low lying levels in considered nuclei and accurate position of the first 1p-1h states Quenching of.75 on magnetic spin operator Accurate reproduction of known magnetic moments of f 7/2 -shell nuclei E exc (MeV) E exc (MeV) EXP SM 44 Sc *J 44 Ti EXP SM *J Kamila Sieja (IPHC) / 18
Recent developments in the nuclear shell model and their interest for astrophysics
Recent developments in the nuclear shell model and their interest for astrophysics Kamila Sieja Institut Pluridisciplinaire Hubert Curien, Strasbourg FUSTIPEN topical meeting "Recent Advances in the Nuclear
More informationRecent developments in the nuclear shell model and their interest for astrophysics
Recent developments in the nuclear shell model and their interest for astrophysics Kamila Sieja Institut Pluridisciplinaire Hubert Curien, Strasbourg Kamila Sieja (IPHC) 10-14.03.24 1 / 46 Atomic nucleus:
More informationAdvantages and Limitations Of The Shell Model
Advantages and Limitations Of The Shell Model F. Nowacki 1 Atelier de Structure Nucléaire Théorique April 7 th /11 th -2008 1 Strasbourg-Madrid-GSI Shell-Model collaboration What do we mean by SHELL MODEL
More informationShell evolution and pairing in calcium isotopes with two- and three-body forces
Shell evolution and pairing in calcium isotopes with two- and three-body forces Javier Menéndez Institut für Kernphysik, TU Darmstadt ExtreMe Matter Institute (EMMI) with Jason D. Holt, Achim Schwenk and
More informationNeutrino-Nucleus Reactions Based on Recent Progress of Shell Model Calculations
Neutrino-Nucleus Reactions Based on Recent Progress of Shell Model Calculations Toshio Suzuki (Nihon University) New shell model calculations in p-shell modified shell model Hamiltonian (SFO) with improved
More informationProbing shell evolution with large scale shell model calculations
Probing shell evolution with large scale shell model calculations Yutaka Utsuno Advanced Science Research Center, Japan Atomic Energy Agency Center for Nuclear Study, University of Tokyo Nuclear structure
More informationBeyond mean-field study on collective vibrations and beta-decay
Advanced many-body and statistical methods in mesoscopic systems III September 4 th 8 th, 2017, Busteni, Romania Beyond mean-field study on collective vibrations and beta-decay Yifei Niu Collaborators:
More informationNuclear structure theory
Nuclear structure theory Thomas Papenbrock and Lecture 2: Traditional shell model National Nuclear Physics Summer School 2008 George Washington University Shell structure in nuclei Mass differences: Liquid
More informationCoexistence phenomena in neutron-rich A~100 nuclei within beyond-mean-field approach
Coexistence phenomena in neutron-rich A~100 nuclei within beyond-mean-field approach A. PETROVICI Horia Hulubei National Institute for Physics and Nuclear Engineering, Bucharest, Romania Outline complex
More informationNeutrinoless Double Beta Decay within the Interacting Shell Model
Neutrinoless Double Beta Decay within the Interacting Shell Model Institute for Nuclear Physics, Technical University Darmstadt (TUD) ExtreMe Matter Institute (EMMI), GSI EFN 2010, El Escorial, 27-29 September
More informationThree-nucleon forces and shell structure of neutron-rich Ca isotopes
Three-nucleon forces and shell structure of neutron-rich Ca isotopes Javier Menéndez Institut für Kernphysik (TU Darmstadt) and ExtreMe Matter Institute (EMMI) NUSTAR Week 3, Helsinki, 9 October 13 Outline
More informationQRPA Calculations of Charge Exchange Reactions and Weak Interaction Rates. N. Paar
Strong, Weak and Electromagnetic Interactions to probe Spin-Isospin Excitations ECT*, Trento, 28 September - 2 October 2009 QRPA Calculations of Charge Exchange Reactions and Weak Interaction Rates N.
More informationShape coexistence and beta decay in proton-rich A~70 nuclei within beyond-mean-field approach
Shape coexistence and beta decay in proton-rich A~ nuclei within beyond-mean-field approach A. PETROVICI Horia Hulubei National Institute for Physics and Nuclear Engineering, Bucharest, Romania Outline
More informationShell-model description for beta decays of pfg-shell nuclei
Shell-model description for beta decays of pfg-shell nuclei Workshop on New Era of Nuclear Physics in the Cosmos the r-process nucleosynthesis Sep. 25-26, 2008 @RIKEN M. Honma (Univ. of Aizu) T. Otsuka
More informationNEW ADVANCES IN SHELL MODEL CALCULATIONS: APPLICATIONS AROUND
NEW ADVANCES IN SHELL MODEL CALCULATIONS: APPLICATIONS AROUND DOUBLY MAGIC NUCLEI 40 Ca AND 132 Sn Houda NAÏDJA IPHC Strasbourg, France GSI Darmstadt, Germany. LPMS, Université Constantine 1, Algeria.
More informationLarge scale shell model calculations for neutron rich fp-shell nuclei
Large scale shell model calculations for neutron rich fp-shell nuclei Physical Research Laboratory, Ahmedabad-380 009, India Collaborators: I. Mehrotra (Allahabad) P.Van Isacker (GANIL, France) V.K.B.
More informationComparison of Nuclear Configuration Interaction Calculations and Coupled Cluster Calculations
Comparison of Nuclear Configuration Interaction Calculations and Coupled Cluster Calculations Mihai Horoi Department of Physics, Central Michigan University, Mount Pleasant, Michigan 48859, USA Support
More informationAccurate Description of the Spinand Parity-Dependent Nuclear Level Densities
Accurate Description of the Spinand Parity-Dependent Nuclear Level Densities Mihai Horoi Department of Physics, Central Michigan University, Mount Pleasant, Michigan 48859, USA Nuclear Level Densities
More informationLecture #3 a) Nuclear structure - nuclear shell model b) Nuclear structure -quasiparticle random phase approximation c) Exactly solvable model d)
Lecture #3 a) Nuclear structure - nuclear shell model b) Nuclear structure -quasiparticle random phase approximation c) Exactly solvable model d) Dependence on the distance between neutrons (or protons)
More informationThe nuclear shell-model: from single-particle motion to collective effects
The nuclear shell-model: from single-particle motion to collective effects 1. Nuclear forces and very light nuclei 2. Independent-particle shell model and few nucleon correlations 3. Many-nucleon correlations:
More informationTEST OF CLOSED-FORM GAMMA-STRENGTH FUNCTIONS. Vladimir Plujko. Taras Shevchenko National University; Institute for Nuclear Research, Kyiv, Ukraine
TEST OF CLOSED-FORM GAMMA-STRENGTH FUNCTIONS Vladimir Plujko Taras Shevchenko National University; Institute for Nuclear Research, Kyiv, Ukraine 1. Radiative (photon, gamma) strength functions (RSF)- definitions.
More informationSilvia M. Lenzi University of Padova and INFN. Silvia Lenzi, 10th Int. Spring Seminar on Nuclear Physics, Vietri sul Mare, May 21-25, 2010
Structure of Neutron-Rich Nuclei near N=40 Silvia M. Lenzi University of Padova and INFN 10th International Spring Seminar on Nuclear Physics Vietri sul Mare, May 21-25, 2010 Collaboration Theory: F. Nowacki,
More informationThe No-Core Shell Model
The No-Core Shell Model New Perspectives on P-shell Nuclei - The Shell Model and Beyond Erich Ormand Petr Navratil Christian Forssen Vesselin Gueorguiev Lawrence Livermore National Laboratory Collaborators:
More informationApplication of Equation of Motion Phonon Method to Nuclear and Exotic Nuclear Systems
Application of Equation of Motion Phonon Method to Nuclear and Exotic Nuclear Systems Petr Veselý Nuclear Physics Institute, Czech Academy of Sciences gemma.ujf.cas.cz/~p.vesely/ seminar at UTEF ČVUT,
More informationSHELL-MODEL RESULTS IN fp AND fpg 9/2 SPACES FOR
SHELL-MODEL RESULTS IN fp AND fpg 9/2 SPACES FOR 61,63,65 Co ISOTOPES P.C. Srivastava 1, * 1, ** and V.K.B. Kota 1 Physical Research Laboratory, Ahmedabad, India arxiv:1004.4443v2 [nucl-th] 18 May 2011
More informationMatrix elements for processes that could compete in double beta decay
Matrix elements for processes that could compete in double beta decay Mihai Horoi Department of Physics, Central Michigan University, Mount Pleasant, Michigan 48859, USA Ø Support from NSF grant PHY-106817
More informationTowards a universal nuclear structure model. Xavier Roca-Maza Congresso del Dipartimento di Fisica Milano, June 28 29, 2017
Towards a universal nuclear structure model Xavier Roca-Maza Congresso del Dipartimento di Fisica Milano, June 28 29, 217 1 Table of contents: Brief presentation of the group Motivation Model and selected
More informationTesting the validity of the Spin-orbit interaction Nuclear forces at the drip-line O. Sorlin (GANIL, Caen, France)
PART 1: Testing the validity of the Spin-orbit interaction Nuclear forces at the drip-line O. Sorlin (GANIL, Caen, France) Introduction to the SO interaction Historical picture -> magic numbers The SO
More informationTowards first-principle description of electromagnetic reactions in medium-mass nuclei
Canada s National Laboratory for Particle and Nuclear Physics Laboratoire national canadien pour la recherche en physique nucléaire et en physique des particules Towards first-principle description of
More informationNew T=1 effective interactions for the f 5/2 p 3/2 p 1/2 g 9/2 model space: Implications for valence-mirror symmetry and seniority isomers
PHYSICAL REVIEW C 70, 044314 (2004) New T=1 effective interactions for the f 5/2 p 3/2 p 1/2 g 9/2 model space: Implications for valence-mirror symmetry and seniority isomers A. F. Lisetskiy, 1 B. A. Brown,
More informationEvolution Of Shell Structure, Shapes & Collective Modes. Dario Vretenar
Evolution Of Shell Structure, Shapes & Collective Modes Dario Vretenar vretenar@phy.hr 1. Evolution of shell structure with N and Z A. Modification of the effective single-nucleon potential Relativistic
More informationRemarks about weak-interaction processes
Remarks about weak-interaction processes K. Langanke GSI Darmstadt and TUD, Darmstadt March 9, 2006 K. Langanke (GSI and TUD, Darmstadt)Remarks about weak-interaction processes March 9, 2006 1 / 35 Nuclear
More informationShell model calculation ー from basics to the latest methods ー
Shell model calculation ー from basics to the latest methods ー Takahiro Mizusaki Senshu university / CNS, the univ. of Tokyo Basics What we will learn? What is Shell Model? Shell model basis states M-scheme
More informationNew Trends in the Nuclear Shell Structure O. Sorlin GANIL Caen
New Trends in the Nuclear Shell Structure O. Sorlin GANIL Caen I. General introduction to the atomic nucleus Charge density, shell gaps, shell occupancies, Nuclear forces, empirical monopoles, additivity,
More informationProbing the evolution of shell structure with in-beam spectroscopy
Probing the evolution of shell structure with in-beam spectroscopy Alexandra Gade National Superconducting Cyclotron Laboratory and Department of Physics and Astronomy at Michigan State University, East
More informationPart III: The Nuclear Many-Body Problem
Part III: The Nuclear Many-Body Problem To understand the properties of complex nuclei from first principles Microscopic Valence- Space Interactions Model spaces Many-body perturbation theory (MBPT) Calculating
More informationThe Nuclear Many-Body Problem. Lecture 2
The Nuclear Many-Body Problem Lecture 2 How do we describe nuclei? Shell structure in nuclei and the phenomenological shell model approach to nuclear structure. Ab-initio approach to nuclear structure.
More informationMICROSCOPIC NATURE OF THE PHOTON STRENGTH FUNCTION: STABLE AND UNSTABLE Ni AND Sn ISOTOPES
MICROSCOPIC NATURE OF THE PHOTON STRENGTH FUNCTION: STABLE AND UNSTABLE Ni AND Sn ISOTOPES O. Achakovskiy 4, A. Avdeenkov 4, S. Goriely 2, S. Kamerdzhiev 1, S. Krewald 3, D. Voitenkov 4 1. Institute for
More informationHigh-spin studies and nuclear structure in three semi-magic regions of the nuclide chart High-seniority states in Sn isotopes
High-spin studies and nuclear structure in three semi-magic regions of the nuclide chart High-seniority states in Sn isotopes Outline: Alain Astier, CSNSM Orsay, France Motivations Experimental conditions
More informationMean field studies of odd mass nuclei and quasiparticle excitations. Luis M. Robledo Universidad Autónoma de Madrid Spain
Mean field studies of odd mass nuclei and quasiparticle excitations Luis M. Robledo Universidad Autónoma de Madrid Spain Odd nuclei and multiquasiparticle excitations(motivation) Nuclei with odd number
More informationarxiv:nucl-th/ v1 20 Dec 2000
Shell model study of the isobaric chains A = 5, A = 5 and A = 5 A. Poves and J. Sánchez-Solano arxiv:nucl-th/77v Dec Departamento de Física Teórica C-XI, Universidad Autónoma de Madrid, E 89 Madrid, Spain
More informationCharge exchange reactions and photo-nuclear reactions
Charge exchange reactions and photo-nuclear reactions σ( 7 Li, 7 Be) and σ(γ,n) S. Nakayama (Univ of Tokushima) Determination of σ(γ,n) from CE reactions (CE reaction = Charge Exchange reaction) Application
More informationProjected shell model for nuclear structure and weak interaction rates
for nuclear structure and weak interaction rates Department of Physics, Shanghai Jiao Tong University, Shanghai 200240, China E-mail: sunyang@sjtu.edu.cn The knowledge on stellar weak interaction processes
More informationShell Model A Unified View of Nuclear Structure
Shell Model A Unified View of Nuclear Structure Frédéric Nowacki 1 18 th STFC UK Postgraduate Summer School Lancaster, August 4 th -September 5 th -15 1 Strasbourg-Madrid Shell-Model collaboration Bibliography
More informationLow-lying gamma-strength within microscopic models
Low-lying gamma-strength within microscopic models Elena Litvinova 1,2 1 GSI Helmholtzzentrum für Schwerionenforschung mbh, Darmstadt, Germany 2 Institut für Theoretische Physik, Goethe Universität, Frankfurt
More informationProbing neutron-rich isotopes around doubly closed-shell 132 Sn and doubly mid-shell 170 Dy by combined β-γ and isomer spectroscopy.
Probing neutron-rich isotopes around doubly closed-shell 132 Sn and doubly mid-shell 170 Dy by combined β-γ and isomer spectroscopy Hiroshi Watanabe Outline Prospects for decay spectroscopy of neutron-rich
More informationSpectroscopic Quadrupole Moment in 96,98 Sr : Shape coexistence at N=60. E.Clément-GANIL IS451 Collaboration
Spectroscopic Quadrupole Moment in 96,98 Sr : Shape coexistence at N=60 E.Clément-GANIL IS451 Collaboration Shape Transition at N=60 P. Campbell, I.D. Moore, M.R. Pearson Progress in Particle and Nuclear
More informationNuclear Structure Theory II
uclear Structure Theory II The uclear Many-body Problem Alexander Volya Florida State University Physics of light nuclei 1 H 4 Li 3 He 2 H 8 7 6 Be 5 Li 4 He 3 B H 10 9 8 7 Be 6 Li 5 He 4 B H 12 11 10
More informationAb Initio Nuclear Structure Theory
Ab Initio Nuclear Structure Theory Lecture 3: Light Nuclei Robert Roth Overview Lecture 1: Hamiltonian Prelude Many-ody Quantum Mechanics Nuclear Hamiltonian Matrix Elements Lecture 2: orrelations Two-ody
More informationThree-step gamma cascades following the neutron capture in 161 Dy
Three-step gamma cascades following the neutron capture in 161 Dy F. Beèváø, T. Belgya, G. de France, M. Jentschel, U. Koester, J. Kroll, M. Krtièka, P. Mutti, R. Schwengner, G. Simpson, I. Tomandl, W.
More informationPhysics of neutron-rich nuclei
Physics of neutron-rich nuclei Nuclear Physics: developed for stable nuclei (until the mid 1980 s) saturation, radii, binding energy, magic numbers and independent particle. Physics of neutron-rich nuclei
More informationJoint ICTP-IAEA Workshop on Nuclear Structure Decay Data: Theory and Evaluation August Introduction to Nuclear Physics - 1
2358-19 Joint ICTP-IAEA Workshop on Nuclear Structure Decay Data: Theory and Evaluation 6-17 August 2012 Introduction to Nuclear Physics - 1 P. Van Isacker GANIL, Grand Accelerateur National d'ions Lourds
More informationCluster Models for Light Nuclei
Cluster Models for Light Nuclei N. Itagaki, T. Otsuka, University of Tokyo S. Aoyama, Niigata University K. Ikeda, RIKEN S. Okabe, Hokkaido University Purpose of the present study Cluster model explore
More informationQuantum Theory of Many-Particle Systems, Phys. 540
Quantum Theory of Many-Particle Systems, Phys. 540 Questions about organization Second quantization Questions about last class? Comments? Similar strategy N-particles Consider Two-body operators in Fock
More informationStructure at and Beyond the Neutron Dripline
Structure at and Beyond the Neutron Dripline Collaboration LPC-CHARISSA CHARISSA-DEMON H Al Falou,, FM Marqués, JL Lecouey, NA Orr, Structure at and Beyond the Neutron Dripline * Motivation Experimental
More informationNuclear Isomers: What we learn from Tin to Tin
INDIAN INSTITUTE OF TECHNOLOGY ROORKEE Nuclear Isomers: What we learn from Tin to Tin Ashok Kumar Jain Bhoomika Maheshwari Department of Physics Outline Nuclear Isomers The longest chain of Sn isotopes
More informationThe Nuclear Many Body Problem Lecture 3
The Nuclear Many Body Problem Lecture 3 Shell structure in nuclei and the phenomenological shell model approach to nuclear structure Ab initio approach to nuclear structure. Green's function Monte Carlo
More informationAligned neutron-proton pairs in N=Z nuclei
Aligned neutron-proton pairs in N=Z nuclei P. Van Isacker, GANIL, France Motivation Shell-model analysis A model with high-spin bosons Experimental tests Neutron-proton correlations, UHK, Hong Kong, July
More informationab-initio alpha-alpha scattering
ab-initio alpha-alpha scattering Elhatisari et al., Nature 528, 111 (215) http://www.nature.com/nature/journal/v528/n758/full/nature1667.html http://www.nature.com/nature/journal/v528/n758/abs/52842a.html
More informationMedium polarization effects and pairing interaction in finite nuclei
Medium polarization effects and pairing interaction in finite nuclei S. Baroni, P.F. Bortignon, R.A. Broglia, G. Colo, E. Vigezzi Milano University and INFN F. Barranco Sevilla University Commonly used
More informationNuclear structure from chiral-perturbation-theory two- plus three-nucleon interactions
Nuclear structure from chiral-perturbation-theory two- plus three-nucleon interactions Petr Navratil Lawrence Livermore National Laboratory* Collaborators: W. E. Ormand (LLNL), J. P. Vary (ISU), E. Caurier
More informationCalculating β Decay for the r Process
Calculating β Decay for the r Process J. Engel with M. Mustonen, T. Shafer C. Fröhlich, G. McLaughlin, M. Mumpower, R. Surman D. Gambacurta, M. Grasso June 3, 26 Nuclear Landscape To convincingly locate
More informationproton-neutron pairing vibrations
proton-neutron pairing vibrations Outline of this lecture: Basics of the vibrational modes of excitation in nuclei surface vibration, like-particle pairing vibration, and then Microscopic framework to
More informationIntroduction to NUSHELLX and transitions
Introduction to NUSHELLX and transitions Angelo Signoracci CEA/Saclay Lecture 4, 14 May 213 Outline 1 Introduction 2 β decay 3 Electromagnetic transitions 4 Spectroscopic factors 5 Two-nucleon transfer/
More informationMeasuring Neutron Capture Cross Sections on s-process Radioactive Nuclei
Measuring Neutron Capture Cross Sections on s-process Radioactive Nuclei 5th Workshop on Nuclear Level Density and Gamma Strength Oslo, May 18-22, 2015 LLNL-PRES-670315 LLNL-PRES-XXXXXX This work was performed
More informationISSN : Asian Journal of Engineering and Technology Innovation 02 (03) 2014 (08-13) QR Code for Mobile users
ISSN : 2347-7385 Calculation of the Energy Levels of 25Na-27Na Isotopes S. Mohammadi, Sima Zamani Department of Physics, Payame Noor University, PO BOX 19395-3697 Tehran, Iran. Received on: 09-03-2014
More informationNovel High Performance Computational Aspects of the Shell Model Approach for Medium Nuclei
Novel High Performance Computational Aspects of the Shell Model Approach for Medium Nuclei Mihai Horoi Department of Physics, Central Michigan University, Mount Pleasant, Michigan 48859, USA Collaborators:
More informationAuxiliary-field Monte Carlo methods in Fock space: sign problems and methods to circumvent them
Auxiliary-field Monte Carlo methods in Fock space: sign problems and methods to circumvent them Introduction Yoram Alhassid (Yale University) Finite-temperature auxiliary-field Monte Carlo methods in Fock
More informationCoupled-cluster computations of weak decays in nuclei
Coupled-cluster computations of weak decays in nuclei Gaute Hagen Oak Ridge National Laboratory Nuclear ab initio Theories and Neutrino Physics INT, March 6th, 2018 Trend in realistic ab-initio calculations
More informationCluster-gas-like states and monopole excitations. T. Yamada
Cluster-gas-like states and monopole excitations T. Yamada Cluster-gas-like states and monopole excitations Isoscalar monopole excitations in light nuclei Cluster-gas-likes states: C, 16 O, 11 B, 13 C
More informationElectromagnetic reactions from few to many-body systems Giuseppina Orlandini
Electromagnetic reactions from few to many-body systems Giuseppina Orlandini ECT* Workshop on Recent advances and challenges in the description of nuclear reactions at the limit of stability, March 5-9,
More informationNew Phenomena in Gamma-Ray Strength Functions
Text optional: Institutsname Prof. Dr. Hans Mustermann www.fzd.de Mitglied der Leibniz-Gemeinschaft Ronald Schwengner Institut für Strahlenphysik http://www.hzdr.de New Phenomena in Gamma-Ray Strength
More informationCharge Exchange and Weak Strength for Astrophysics
Charge Exchange and Weak Strength for Astrophysics Sam Austin STANfest-July 16 2004 Charge Exchange and Weak Strength for Astrophysics Interesting phenomena Electron capture strength (GT) (Langanke talk)
More informationModeling the Atomic Nucleus. Theoretical bag of tricks
Modeling the Atomic Nucleus Theoretical bag of tricks The nuclear many-body problem The Nuclear Many-Body Problem H ˆ = T ˆ + V ˆ ˆ T = A 2 p ˆ " i, V ˆ = 2m i i=1 one-body H ˆ " = E" " V ˆ 2b (i, j) +
More informationQRPA calculations of stellar weak-interaction rates
QRPA calculations of stellar weak-interaction rates P. Sarriguren Instituto de Estructura de la Materia CSIC, Madrid, Spain Zakopane Conference on Nuclear Physics: Extremes of Nuclear Landscape. August
More informationA simple effective interaction for 9 He, and Gamow-SRG
A simple effective interaction for 9 He, and Gamow-SRG Kévin Fossez February 28, 218 FRIB, MSU FRIB, MSU - Kévin Fossez Work supported by: DOE: DE-SC1336 (Michigan State University) DOE: DE-SC17887 (Michigan
More informationThree-Nucleon Forces and Masses of Neutron-Rich Nuclei Jason D. Holt
Three-Nucleon Forces and Masses of Neutron-Rich Nuclei Jason D. Holt Drip Lines and Magic Numbers: The Evolving Nuclear Landscape 3N forces important in light nuclei, nuclear matter What are the limits
More informationNucleon Pair Approximation to the nuclear Shell Model
Nucleon Pair Approximation to the nuclear Shell Model Yiyuan Cheng Department of Physics and Astronomy, Shanghai Jiao Tong University, China RCNP, Osaka university, Japan Collaborators: Yu-Min Zhao, Akito
More informationin covariant density functional theory.
Nuclear Particle ISTANBUL-06 Density vibrational Functional coupling Theory for Excited States. in covariant density functional theory. Beijing, Sept. 8, 2011 Beijing, May 9, 2011 Peter Peter Ring Ring
More informationNuclear Physics and Supernova Dynamics. Karlheinz Langanke GSI Helmholtzzentrum Darmstadt Technische Universität Darmstadt
Nuclear Physics and Supernova Dynamics Karlheinz Langanke GSI Helmholtzzentrum Darmstadt Technische Universität Darmstadt Tribute to Gerry - Stony Brook, November 26, 2013 Hans Bethe s Centennial at Caltech
More informationNew Frontiers in Nuclear Structure Theory
New Frontiers in Nuclear Structure Theory From Realistic Interactions to the Nuclear Chart Robert Roth Institut für Kernphysik Technical University Darmstadt Overview Motivation Nucleon-Nucleon Interactions
More informationStatistical Approach to Nuclear Level Density
Statistical Approach to Nuclear Level Density R. A. Sen kov,v.g.zelevinsky and M. Horoi Department of Physics, Central Michigan University, Mount Pleasant, MI 889, USA Department of Physics and Astronomy
More informationTheory for nuclear processes in stars and nucleosynthesis
Theory for nuclear processes in stars and nucleosynthesis Gabriel Martínez Pinedo Nuclear Astrophysics in Germany November 15-16, 2016 Nuclear Astrophysics Virtual Institute Outline 1 Ab-initio description
More informationDipole Response of Exotic Nuclei and Symmetry Energy Experiments at the LAND R 3 B Setup
Dipole Response of Exotic Nuclei and Symmetry Energy Experiments at the LAND R 3 B Setup Dominic Rossi for the LAND collaboration GSI Helmholtzzentrum für Schwerionenforschung GmbH D 64291 Darmstadt, Germany
More information14. Structure of Nuclei
14. Structure of Nuclei Particle and Nuclear Physics Dr. Tina Potter Dr. Tina Potter 14. Structure of Nuclei 1 In this section... Magic Numbers The Nuclear Shell Model Excited States Dr. Tina Potter 14.
More informationGamma-ray strength functions obtained with the Oslo method
Gamma-ray strength functions obtained with the Oslo method Ann-Cecilie Larsen July 8, 2008 DEPARTMENT OF PHYSICS UNIVERSITY OF OSLO Collaborators Oslo: A. Bürger, M. Guttormsen, S. Messelt, F. Ingebretsen,
More informationNuclear structure and stellar weak interaction rates of nuclei below the 132 Sn core
Nuclear structure and stellar weak interaction rates of nuclei below the 132 Sn core Nuclear and Atomic Physics Division, Saha Institute of Nuclear Physics, Kolkata 700064, INDIA E-mail: maitrayee.sahasarkar@saha.ac.in
More informationPARTICLE-NUMBER CONSERVING
PARTICLE-NUMBER CONSERVING MICROSCOPIC APPROACH AND APPLICATION TO ISOSPIN MIXING L. Bonneau, J. Le Bloas, H. Naidja, P. Quentin, K. Sieja (CENBG/Université Bordeaux 1) J. Bartel (IPHC/Université Louis
More informationProbing properties of the nuclear force in extreme conditions
Probing properties of the nuclear force in extreme conditions O. Sorlin (GANIL, Caen, rance) PART 1: Testing the spin-orbit force with a bubble nucleus PART 2: Proton-neutron forces at the drip-line May
More informationSemi-Classical perturbation theory Coulomb only First-order most used
direct reactions Models for breakup Semi-Classical perturbation theory Coulomb only First-order most used TDSE (Time Dependent Schrodinger Equation) Coulomb + Nuclear Semi-classical orbit needed DWBA (Distorted
More informationThe Nuclear Equation of State
The Nuclear Equation of State Theoretical models for nuclear structure studies Xavier Roca-Maza Università degli Studi di Milano e INFN, sezione di Milano Terzo Incontro Nazionale di Fisica Nucleare LNF,
More informationThe 2010 US National Nuclear Physics Summer School and the TRIUMF Summer Institute, NNPSS-TSI June 21 July 02, 2010, Vancouver, BC, Canada
TU DARMSTADT The 2010 US National Nuclear Physics Summer School and the TRIUMF Summer Institute, NNPSS-TSI June 21 July 02, 2010, Vancouver, BC, Canada Achim Richter ECT* Trento/Italy and TU Darmstadt/Germany
More informationPhases in an Algebraic Shell Model of Atomic Nuclei
NUCLEAR THEORY, Vol. 36 (2017) eds. M. Gaidarov, N. Minkov, Heron Press, Sofia Phases in an Algebraic Shell Model of Atomic Nuclei K.P. Drumev 1, A.I. Georgieva 2, J. Cseh 3 1 Institute for Nuclear Research
More informationNuclear Matter Incompressibility and Giant Monopole Resonances
Nuclear Matter Incompressibility and Giant Monopole Resonances C.A. Bertulani Department of Physics and Astronomy Texas A&M University-Commerce Collaborator: Paolo Avogadro 27th Texas Symposium on Relativistic
More informationFeatures of nuclear many-body dynamics: from pairing to clustering
Features of nuclear many-body dynamics: from pairing to clustering Alexander Volya Florida State University Collaborators: K. Kravvaris, Yu. Tchuvil sky Outline Configuration interaction approach SU(3)
More informationMagnetic Dipole and Quadrupole Transitions in Nuclei Open Problems
TU DARMSTADT Magnetic Dipole and Quadrupole Transitions in Nuclei Open Problems Qualitative nature of the M1 response Orbital M1 scissors mode: low and high Spin M1 resonance in heavy deformed nuclei Quenching
More informationNature of low-energy dipole states in exotic nuclei
Nature of low-energy dipole states in exotic nuclei Xavier Roca-Maza Università degli Studi di Milano, Via Celoria 16, I-133, Milano SPES One-day Workshop on "Collective Excitations of Exotic Nuclei" December
More informationHigh-resolution study of Gamow- Teller transitions in pf-shell nuclei. Tatsuya ADACHI
High-resolution study of Gamow- Teller transitions in pf-shell nuclei Tatsuya ADACHI Type II supernova Electron Capture (EC) & β decay Neutrino induced reaction A Z-1X N+1 daughter EC β A ZX N parent (A,Z)
More informationE1 STRENGTH FUNCTIONS FOR PHOTOABSORPTION AND EMISSION WITHIN CLOSED-FORM METHODS
E1 STRENGTH FUNCTIONS FOR PHOTOABSORPTION AND EMISSION WITHIN CLOSED-FORM METHODS 1. Introduction V.A. Plujko *), O.M.Gorbachenko *), R. Capote &), V.Bondar *) *) NPD, Taras Shevchenko National University,
More informationLaser spectroscopy studies of neutron-rich nuclei
Laser spectroscopy studies of neutron-rich nuclei Ronald Fernando Garcia Ruiz The University of Manchester Walk on the neutron-rich side ECT* Trento, April 2017 The COLLAPS Collaboration M. Bissell, K.
More information