Single Particle EnergiesIntroductionMean-Field ApproximationMean Field (cont.)Hartree-Fock MethodHartree-Fock Method (cont.)Hartree-Fock Method with Skyrme InteractionSkyrme Interaction (cont.)Determining the Skyrme ParametersValues of the Skyrme ParametersWoods-Saxon PotentialWoods-Saxon Potential (cont.)Slide 13Nucleon Density from Hartree-Fock kde0 Interaction22O kde0 r2UHF Fit to r2UWS208Pb kde0 r2UHF Fit to r2UWSSingle Particle Energies (in MeV) for 16OSingle Particle Energies (in MeV) for 22OSpin-Orbit Splittings for 17F and 23FConclusionsAcknowledgmentsSingle Particle Energiesin Skyrme Hartree-Fock and Woods-Saxon PotentialsBrian D. NewmanCyclotron InstituteTexas A&M UniversityMentor: Dr. Shalom ShlomoIntroductionAtomic nuclei exhibit the interesting phenomenon of single-particle motion that can be described within the mean field approximation for the many-body system. We have carried out Hartree-Fock calculations for a wide range of nuclei, using the Skyrme-type interactions. We have examined the resulting mean field potentials UHF by fitting r2UHF to r2UWS, where UWS is the commonly used Woods-Saxon potential. We consider, in particular, the asymmetry (x=(N-Z)/A) dependence in UWS and the spin-orbit splitting in the spectra of 17F8 and the recently measured spectra of 23F14. Using UWS, we obtained good agreement with experimental data.Mean-Field Approximation•Many-body problem for nuclear wave-function generally cannot be solved analytically•In Mean-Field Approximation each nucleon interacts independently with a potential formed by other nucleonsSingle-Particle Schrödinger Equation:A-Nucleon Wave-Function:A=Anti-Symmetrization operator for fermionsMean-Field ApproximationHΨ=EΨ-60-50-40-30-20-1000 2 4 6 8 10 12RVoUi(r)•Single-particle wave-functions Φi are determined by the independent single-particle potentials•Due to spherical symmetry, the solution is separable into radial component ; angular component (spherical harmonics) ; and the isospin function :Mean Field (cont.)•The anti-symmetric ground state wave-function of a nucleus can be written as a Slater determinant of a matrix whose elements are single-particle wave-functionsHartree-Fock Method•The Hamiltonian operator is sum of kinetic and potential energy operators:where:•The ground state wave-function should give the lowest expectation value for the HamiltonianHartree-Fock Method (cont.)•We want to obtain minimum of E with the constraint that the sum of the single-particle wave-function integrals over all space is A, to conserve the number of nucleons:We obtain the Hartree-Fock Equations:Hartree-Fock Method with Skyrme Interaction•The Skyrme two-body NN interaction potential is given by:operates on the right sideoperates on the left sideijPis the spin exchange operatorto, t1, t2, t3, xo, x1, x2, x3, , and Wo are the ten Skyrme parametersSkyrme Interaction (cont.)•After all substitutions and making the coefficients of all variations equal to zero, we have the Hartree-Fock Equations:•mτ*(r), Uτ(r), and Wτ(r) are given in terms of Skyrme parameters, nucleon densities, and their derivatives•If we have a reasonable first guess for the single-particle wave-functions, i.e. harmonic oscillator, we can determine mτ*, Uτ (r), and Wτ (r) and keep reiterating the HF Method until the wave-functions convergeDetermining the Skyrme Parameters•Skyrme Parameters were determined by a fit of Hartree-Fock results to experimental data•Example: kde0 interaction was obtained with the following dataProperties NucleiB16,24O, 34Si, 40,48Ca, 48,56,68,78Ni, 88Sr, 90Zr, 100,132Sn, 208Pbrch16O, 40,48Ca, 56Ni, 88Sr, 90Zr, 208Pbrv(υ1d5/2)17Orv(υ1f7/2)41CaS-O 2p orbits in 56NiEo90Zr, 116Sn, 144Sm, 208PbρcrNuclear MatterTable: Selected experimental data for the binding energy B, charge rms radius rch , rms radii of valence neutron orbits rv, spin-orbit splitting S-O, breathing mode constrained energy Eo, and critical density ρcr used in the fit to determine the parameters of the Skyrme interaction.Values of the Skyrme Parameters Parameter kde0 (2005) sgII (1985)to (MeV fm3)-2526.51 (140.63) -2645.00t1 (MeV fm5)430.94 (16.67) 340.00t2 (MeV fm5)-398.38 (27.31) -41.90t3 (MeV fm3(1+))14235.5 (680.73) 1559.00xo0.7583 (0.0655) 0.09000x1-0.3087 (0.0165) -0.05880x2-0.9495 (0.0179) 1.4250x31.1445 (0.0882) 0.06044Wo (MeV fm5)128.96 (3.33) 105.000.1676 (0.0163) 0.16667Woods-Saxon PotentialStandard Parameterization:awith ro(1- αv τz )ro=1.27 fmWe adopt the parameterization: R = ro[(A-1)1/3+d][1-αR τz]Uo=-Vo(1- αv τz)USO=-VSO(1- αv τz)a=ao(1+ αa| |)The parameters were determined from the UHF calculated for a wide range of nuclei.Woods-Saxon Potential (cont.)Woods-Saxon Potential (cont.)Schrödinger's Equation:Separable Solution:where:Numerical Solution:Starting from uo and u1, we find u2 and continue to get u3, u4, …Nucleon Density from Hartree-Fock kde0 Interaction22O kde0 r2UHF Fit to r2UWS Protons-Vo=58.298R=3.800a=0.520Neutrons-Vo=52.798R=3.420a=0.534MeV fm2MeV fm2fmfm208Pb kde0 r2UHF Fit to r2UWS Protons-Vo=68.256R=7.355a=0.621Neutrons-Vo=60.875R=7.055a=0.636MeV fm2MeV fm2fmfmSingle Particle Energies (in MeV) for 16OParticle StateExperimental kde0 sgIIWoods-Saxon1s1/235.74 35.09 33.841p3/221.8 20.05 20.63 20.101p1/215.7 13.88 14.98 16.561d5/24.14 5.89 7.03 6.442s1/23.27 3.20 3.99 4.681d3/2-0.94 -1.02 0.11 1.131s1/240831.58 31.37 30.031p3/218.4 16.19 17.11 16.641p1/212.1 10.17 11.57 13.111d5/20.60 2.37 3.75 2.962s1/20.10 0.12 0.98 1.501d3/2-4.40 -3.65 -2.69 -2.02neutronsprotonsSingle Particle Energies (in MeV) for 22OParticle StateExperimental kde0 sgIIWoods-Saxon1s1/237.97 36.92 28.871p3/220.32 21.69 17.041p1/217.37 16.85 14.431d5/26.85 5.42 8.36 5.482s1/22.74 3.99 5.93 4.521d3/20.34 1.03 1.651s1/241.94 40.60 38.241p3/227.67 26.53 25.881p1/223.24 21.19 21.66 22.821d5/213.24 14.03 12.72 12.972s1/210.97 9.06 8.22 10.061d3/29.18 4.89 5.38 7.46neutronsprotonsSpin-Orbit Splittings for 17F and 23FExperimental values of single-particle energy levels (in MeV) for 17F and 23F, along with predicted values from Skyrme Hartree-Fock and Woods-Saxon calculations.Conclusions•We find that the single-particle energies obtained from Skyrme Hartree-Fock calculations strongly depend on the Skyrme interaction.•By examining the Hartree-Fock single-particle potential UHF, calculated for a wide range of nuclei, we have determined the