NSR Query Results
Output year order : Descending NSR database version of April 11, 2024. Search: Author = F.Lechaftois Found 5 matches. 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
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
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
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
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
Back to query form |