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Single Particle Energies
in Skyrme Hartree-Fock and Woods-Saxon Potentials Brian D. Newman Cyclotron Institute Texas A&M University Mentor: Dr. Shalom Shlomo
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Introduction Atomic 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.
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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 nucleons HΨ=EΨ Mean-Field Approximation R Ui(r) Single-Particle Schrödinger Equation: A-Nucleon Wave-Function: Vo A=Anti-Symmetrization operator for fermions
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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-functions 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 :
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Hartree-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 Hamiltonian
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Hartree-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:
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Hartree-Fock Method with Skyrme Interaction
The Skyrme two-body NN interaction potential is given by: operates on the right side operates on the left side is the spin exchange operator to, t1, t2, t3, xo, x1, x2, x3, , and Wo are the ten Skyrme parameters
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Skyrme 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 converge
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Determining 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 data Properties Nuclei B 16,24O, 34Si, 40,48Ca, 48,56,68,78Ni, 88Sr, 90Zr, 100,132Sn, 208Pb rch 16O, 40,48Ca, 56Ni, 88Sr, 90Zr, 208Pb rv(υ1d5/2) 17O rv(υ1f7/2) 41Ca S-O 2p orbits in 56Ni Eo 90Zr, 116Sn, 144Sm, 208Pb ρcr Nuclear Matter Table: 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.
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Values of the Skyrme Parameters
kde0 (2005) sgII (1985) to (MeV fm3) (140.63) t1 (MeV fm5) (16.67) 340.00 t2 (MeV fm5) (27.31) -41.90 t3 (MeV fm3(1+)) (680.73) xo (0.0655) x1 (0.0165) x2 (0.0179) 1.4250 x3 (0.0882) Wo (MeV fm5) (3.33) 105.00 (0.0163)
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Woods-Saxon Potential
Standard Parameterization: ro a (1- αv τz ) ro=1.27 fm with
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Woods-Saxon Potential (cont.)
We 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.
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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, …
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Nucleon Density from Hartree-Fock kde0 Interaction
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22O kde0 r2UHF Fit to r2UWS fm MeV fm2 fm MeV fm2 Protons -Vo=58.298
a=0.520 fm MeV fm2 Neutrons -Vo=52.798 R=3.420 a=0.534
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208Pb kde0 r2UHF Fit to r2UWS fm MeV fm2 fm MeV fm2 Protons -Vo=68.256
a=0.621 fm MeV fm2 Neutrons -Vo=60.875 R=7.055 a=0.636
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Single Particle Energies (in MeV) for 16O
Particle State Experimental kde0 sgII Woods-Saxon 1s1/2 35.74 35.09 33.84 1p3/2 21.8 20.05 20.63 20.10 1p1/2 15.7 13.88 14.98 16.56 1d5/2 4.14 5.89 7.03 6.44 2s1/2 3.27 3.20 3.99 4.68 1d3/2 -0.94 -1.02 0.11 1.13 408 31.58 31.37 30.03 18.4 16.19 17.11 16.64 12.1 10.17 11.57 13.11 0.60 2.37 3.75 2.96 0.10 0.12 0.98 1.50 -4.40 -3.65 -2.69 -2.02 neutrons protons
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Single Particle Energies (in MeV) for 22O
Particle State Experimental kde0 sgII Woods-Saxon 1s1/2 37.97 36.92 28.87 1p3/2 20.32 21.69 17.04 1p1/2 17.37 16.85 14.43 1d5/2 6.85 5.42 8.36 5.48 2s1/2 2.74 3.99 5.93 4.52 1d3/2 0.34 1.03 1.65 41.94 40.60 38.24 27.67 26.53 25.88 23.24 21.19 21.66 22.82 13.24 14.03 12.72 12.97 10.97 9.06 8.22 10.06 9.18 4.89 5.38 7.46 neutrons protons
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Spin-Orbit Splittings for 17F and 23F
Experimental values of single-particle energy levels (in MeV) for 17F and 23F, along with predicted values from Skyrme Hartree-Fock and Woods-Saxon calculations.
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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 asymmetry dependence in the Woods-Saxon potential well. We obtained good agreement between the experimental data for the single-particle energies for the protons in 17F and 23F, with those obtained using the Woods-Saxon potential.
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Grant number: DOE-FG03-93ER40773
Acknowledgments Grant numbers: PHY PHY Grant number: DOE-FG03-93ER40773
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