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NSR database version of April 11, 2024.

Search: Author = F.Lechaftois

Found 5 matches.

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2016GO28      Phys.Rev. C 94, 044306 (2016)

S.Goriely, S.Hilaire, S.Peru, M.Martini, I.Deloncle, F.Lechaftois

Gogny-Hartree-Fock-Bogolyubov plus quasiparticle random-phase approximation predictions of the M1 strength function and its impact on radiative neutron capture cross section

NUCLEAR STRUCTURE 58,62,66,70,74,78,80,82,84Ni, 120,124,128,132,136,140,144,148,152,156,160Sn, 92Zr, 106Pd, 198Au, 208Pb, 232Th, 238U, 240Pu; N=6-150, 412 even-even nuclei; calculated B(M1) strengths, centroid M1 energies, integrated B(M1) strengths, M1 photoabsorption σ for 128,134Xe, B(E1) strengths for 232Th and 238U. A=20-250; calculated Γγ for E1 and M1 contributions. Large-scale calculations in the framework of axially-symmetric-deformed quasiparticle random phase approximation (QRPA) based on finite-range D1M Gogny force. Comparison with available experimental data. Analyzed impact on radiative neutron capture cross sections.

doi: 10.1103/PhysRevC.94.044306
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2016MA43      Phys.Rev. C 94, 014304 (2016)

M.Martini, S.Peru, S.Hilaire, S.Goriely, F.Lechaftois

Large-scale deformed quasiparticle random-phase approximation calculations of the γ-ray strength function using the Gogny force

NUCLEAR STRUCTURE 34S, 70,76Ge, 92Zr, 120Sn, 152Sm, 158Gd, 196Pt, 208Pb, 238U, 240Pu; A=10-250; calculated E1 γ-strength functions, B(E1) distributions in the GDR region. 115,120,125,130,135,140,145,150,155Sn; calculated and comparison E1 strength functions for Sn isotopes obtained with the three prescriptions used to correct the HFB+QRPA model based on D1M force. Self-consistent Hartree-Fock-Bogoliubov (HFB) plus axially symmetric deformed quasiparticle random-phase approximation (QRPA) calculations based on finite-range Gogny interactions D1S and D1M. Comparison with experimental photoabsorption data. Discussed predictions of γ-ray strength functions and Maxwellian-averaged neutron capture rates for Sn isotopes.

NUCLEAR REACTIONS 28Si, 60Ni, 70,74Ge, 76,80Se, 90,94Zr, 90,98Mo, 116,119,120Sn, 124,128Te, 138Ba, 142Ce, 144,148Nd, 144,150,154Sm, 158Gd, 174Yb, 181Ta, 190Os, 206Pb, 232Th, 236,238U, 239Pu(γ, X), E*=5-30 MeV; calculated σ and compared with experimental data near the GDR. Self-consistent Hartree-Fock-Bogoliubov (HFB) plus axially symmetric deformed quasiparticle random-phase approximation (QRPA) calculations based on finite-range Gogny interactions D1S and D1M.

doi: 10.1103/PhysRevC.94.014304
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2015CO03      Phys.Lett. B 743, 451 (2015)

A.Corsi, S.Boissinot, A.Obertelli, P.Doornenbal, M.Dupuis, F.Lechaftois, M.Matsushita, S.Peru, S.Takeuchi, H.Wang, N.Aoi, H.Baba, P.Bednarczyk, M.Ciemala, A.Gillibert, T.Isobe, A.Jungclaus, V.Lapoux, J.Lee, M.Martini, K.Matsui, T.Motobayashi, D.Nishimura, S.Ota, E.Pollacco, H.Sakurai, C.Santamaria, Y.Shiga, D.Sohler, D.Steppenbeck, R.Taniuchi

Neutron-driven collectivity in light tin isotopes: Proton inelastic scattering from 104Sn

NUCLEAR REACTIONS 1H(104Sn, 104Sn'), E=150 MeV/nucleon; measured reaction products, Eγ, Iγ. 104Sn; deduced σ(θ), energy levels, J, π. QRPA with the D1M Gogny interaction calculations.

doi: 10.1016/j.physletb.2015.03.018
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2015DU16      Eur.Phys.J. A 51, 168 (2015)

M.Dupuis, E.Bauge, S.Hilaire, F.Lechaftois, S.Peru, N.Pillet, C.Robin

Progress in microscopic direct reaction modeling of nucleon induced reactions

doi: 10.1140/epja/i2015-15168-x
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2015LE10      Phys.Rev. C 92, 034315 (2015)

F.Lechaftois, I.Deloncle, S.Peru

Introduction of a valence space in quasiparticle random-phase approximation: Impact on vibrational mass parameters and spectroscopic properties

NUCLEAR STRUCTURE 100,102,104,106,108,110,112,114,116,118,120,122,124,126,128,130,132,134,136,138,140,142,144Sn; calculated Bohr Hamiltonian vibrational mass parameters and their convergence scheme, energies of first 2+ and 3- states, B(E2), B(E3). Hartree-Fock-Bogoliubov+quasiparticle random-phase approximation (QRPA) framework with Gogny D1M interaction and using two restrictions: Tamm-Dancoff approximation and the insertion of a valence space.

doi: 10.1103/PhysRevC.92.034315
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