Quantify correlations between the neutron skin and other quantities characterizing finite nuclei and infinite nuclear matter. How will additional data.

Slides:

Advertisements

Similar presentations

Why CREX After PREX? Witold Nazarewicz (UTK/ORNL) Calcium Radius Experiment (CREX) Workshop at Jefferson Lab, Mar , 2013 Main contributors: Jochen.

Advertisements

Search for key nuclear structure states below 132 Sn M. Górska, M. Pfützner, H. Grawe et al.

EkEk ∆ δ A I of rigid Gap parameters from moments of Inertia.

University of Liverpool

1 Theory of neutron-rich nuclei and nuclear radii Witold Nazarewicz (with Paul-Gerhard Reinhard) PREX Workshop, JLab, August 17-19, 2008 Introduction to.

Isospin dependence and effective forces of the Relativistic Mean Field Model Georgios A. Lalazissis Aristotle University of Thessaloniki, Greece Georgios.

Lawrence Livermore National Laboratory UCRL-XXXX Lawrence Livermore National Laboratory, P. O. Box 808, Livermore, CA This work performed under.

Isospin effect in the projectile fragmentation of calcium isotopes and a possible experimental observable? Chun-Wang Ma Department of Physics, Henan Normal.

Towards a Universal Energy Density Functional Towards a Universal Energy Density Functional Study of Odd-Mass Nuclei in EDF Theory N. Schunck University.

The Collective Model Aard Keimpema.

John Daoutidis October 5 th 2009 Technical University Munich Title Continuum Relativistic Random Phase Approximation in Spherical Nuclei.

Nuclear equation of state in form suitable for quantum molecular dynamics model 1.Brief indroduction of the EOS prescription 2.New form for bullk and surface.

9/28/ :01 (00) PAIRING PROPERTIES OF SUPERHEAVY NUCLEI A. Staszczak, J. Dobaczewski and W. Nazarewicz (KFT UMCS) (IFT UW) (ORNL & UT)

Application of DFT to the Spectroscopy of Odd Mass Nuclei N. Schunck Department of Physics  Astronomy, University of Tennessee, Knoxville, TN-37996, USA.

Higher Order Multipole Transition Effects in the Coulomb Dissociation Reactions of Halo Nuclei Dr. Rajesh Kharab Department of Physics, Kurukshetra University,

Nuclear Electromagnetic Moments

XV Nuclear Physics Workshop Kazimierz 2008: "75 years of nuclear fission" Sept. 25, ISTANBUL-06 Kazimierz Dolny, Sept. 25, 2008 Technical.

P. Arumugam Centro de Física das Interacções Fundamentais and Departamento de Física, Instituto Superior Técnico, Lisbon, Portugal S.K. Patra, P.K. Sahu,

Equation of State of Neutron-Rich Matter in the Relativistic Mean-Field Approach Farrukh J. Fattoyev My TAMUC collaborators: B.-A. Li, W. G. Newton My.

Nuclear and Radiation Physics, BAU, 1 st Semester, (Saed Dababneh). 1 Nuclear Binding Energy B tot (A,Z) = [ Zm H + Nm n - m(A,Z) ] c 2 B  m.

The first systematic study of the ground-state properties of finite nuclei in the relativistic mean field model Lisheng Geng Research Center for Nuclear.

Tomohiro Oishi 1,2, Markus Kortelainen 2,1, Nobuo Hinohara 3,4 1 Helsinki Institute of Phys., Univ. of Helsinki 2 Dept. of Phys., Univ. of Jyvaskyla 3.

Exotic Nuclei in Relativistic and Non-Relativistic Models Exotic Nuclei large isospin asymmetry - nuclei close to the drip lines - superheavy nuclei non-relativistic.

1 Correlation analysis for neutron skins Witold Nazarewicz and Paul-Gerhard Reinhard (presented at PREX Workshop, JLab, August 17-19, 2008)

N. Paar 1,2 1 Department of Physics, University of Basel, Switzerland 2 Department of Physics, Faculty of Science, University of Zagreb, Croatia International.

Limits of applicability of the currently available EoS at high density matter in neutron stars and core-collapse supernovae: Discussion comments Workshop.

Spectroscopy of Odd-Mass Nuclei in Energy Density Functional Theory Impact of Terascale Computing N. Schunck University of Tennessee, 401 Nielsen Physics,

Nuclear Structure SnSn P,n p n (  )‏ ( ,Xn)‏ M1E1 p,nn X λ ?E1 ExEx  Study of the pygmy dipole resonance as a function of deformation.

ExperimentSpokesmanGoalRunning time Thesis? Scissors ModeTonchevAnalyze Scissors Mode excitations in actinide nuclei Pgymy DipoleTonchevAnalyze evolution.

NEUTRON SKIN AND GIANT RESONANCES Shalom Shlomo Cyclotron Institute Texas A&M University.

1 Technology to calculate observables Global properties Spectroscopy DFT Solvers Functional form Functional optimization Estimation of theoretical errors.

Lecture 23: Applications of the Shell Model 27/11/ Generic pattern of single particle states solved in a Woods-Saxon (rounded square well)

DFT Applications Technology to calculate observables Global properties Spectroscopy DFT Solvers Functional form Functional optimization Estimation of theoretical.

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.

July 29-30, 2010, Dresden 1 Forbidden Beta Transitions in Neutrinoless Double Beta Decay Kazuo Muto Department of Physics, Tokyo Institute of Technology.

Information content of a new observable Witold Nazarewicz University of Aizu-JUSTIPEN-EFES Symposium on "Cutting-Edge Physics of Unstable Nuclei” Aizu-Wakamatsu,

MICROSCOPIC CALCULATION OF SYMMETRY PROJECTED NUCLEAR LEVEL DENSITIES Kris Van Houcke Ghent University In collaboration with S. Rombouts, K. Heyde, Y.

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)

Quantum phase transitions and structural evolution in nuclei.

Quantum Phase Transitions in Nuclei

Global fitting of pairing density functional; the isoscalar-density dependence revisited Masayuki YAMAGAMI (University of Aizu) Motivation Construction.

Symmetry energy in the neutron star equation of state and astrophysical observations David E. Álvarez C. Sept 2013 S. Kubis, D. Blaschke and T. Klaehn.

The Team: Ab initio DFT OSU (Drut, Furnstahl, Platter) MSU (Bogner, Gebremariam) DFT applications UTK (Nazarewicz, Pei, Schunck, Sheikh, Stoitsov) UW Seattle.

Symmetries of the Cranked Mean Field S. Frauendorf Department of Physics University of Notre Dame USA IKH, Forschungszentrum Rossendorf, Dresden Germany.

SFB 634 *Supported by the DFG within SFB 634 and 446 JAP 113/267/0-2 Complete Dipole Strength Distributions from High-Resolution Polarized Proton Scattering.

Electric Dipole Response, Neutron Skin, and Symmetry Energy

Uncertainty Quantification and Bayesian Model Averaging

Determining Reduced Transition Probabilities for 152 ≤ A ≤ 248 Nuclei using Interacting Boson Approximation (IBA-1) Model By Dr. Sardool Singh Ghumman.

The role of isospin symmetry in medium-mass N ~ Z nuclei

Shape parameterization

Witold Nazarewicz/Dario Vretenar

Probing the neutron skin thickness in collective modes of excitation

Nuclear Binding Energy

Probing Nuclear Skins through Density Form Factors

The Isovector Giant Quadrupole Resonance & Nuclear Matter

Structure and dynamics from the time-dependent Hartree-Fock model

Evolution of octupole collectivity in 221Th

BE and charge radii well described (mostly isoscalar)

Nuclear Structure and Reactions: Building Together for the Future

JLab6: Cluster structure connects to high-momentum components and internal quark modification of nuclei Short-Range Correlations (SRCs) dominated by np.

Nuclear masses of neutron-rich nuclei and symmetry energy

Nuclear Chemistry CHEM 396 Chapter 4, Part B Dr. Ahmad Hamaed

Technical University Munich

a non-adiabatic microscopic description

Parametrisation of Binding Energies

Symmetry energy coefficients and shell gaps from nuclear masses

Di-nucleon correlations and soft dipole excitations in exotic nuclei

Fission on the Neutron-Rich Side of the Valley of Stability

Parity – Violating Neutron Density Measurements : PREX, C-REX

Presentation transcript:

Quantify correlations between the neutron skin and other quantities characterizing finite nuclei and infinite nuclear matter. How will additional data on neutron-rich nuclei (e.g., masses) help us constraining the neutron skin? Can one make reliable estimates of neutron-to-proton radii for open-shell nuclei, important in the context of parity violation, where deformation and pairing effects are large? Quantify the regions of instability of the nuclear energy density functional Is there an evidence for the isovector component of the pairing functional?

Correlations between observables Witold Nazarewicz and Paul-Gerhard Reinhard Consider an EDF described by coupling constants The optimum parameter set Uncertainty in variable A: Correlation between variables A and B:

Alignment of variables A and B: =1: full alignment/correlation =0: not aligned/statistically independent P. Klüpfel et al, arXi:0804.3385

Quantities of interest… bulk equilibrium symmetry energy symmetry energy at surface density slope of binding energy of neutron matter dipole polarizability rescaled polarizabiliy

Correlation between observables

alignment with F(q) in 208Pb The degree of alignment for various observables highly correlated statistically independent alignment with F(q) in 208Pb

Survey of odd-even BE differences Bertsch, Bertulani, Nazarewicz, Schunck, Stoitsov