NSR Query Results
Output year order : Descending NSR database version of April 26, 2024. Search: Author = F.Raimondi Found 12 matches. 2020SO01 Phys.Rev. C 101, 014318 (2020) V.Soma, P.Navratil, F.Raimondi, C.Barbieri, T.Duguet Novel chiral Hamiltonian and observables in light and medium-mass nuclei NUCLEAR STRUCTURE 3H, 3,4,6,8He, 6,7,9Li, 7,8,9,10Be, 10,11B, 12,13,14C, 14N, 14,16O, 36Ca, 68Ni; calculated ground-state energies. 6,7,9Li, 8,9Be, 10,11B, 12,13C; calculated levels, J, π. 12,13,14,15,16,17,18,19,20,21,22,23,24,25,26,27,28O, 34,35,36,37,38,39,40,41,42,43,44,45,46,47,48,49,50,51,52,53,54,55,56,57,58,59,60,70Ca, 48,49,50,51,52,53,54,55,56,57,58,59,60,61,62,63,64,65,66,67,68,69,70,71,72,73,74,75,76,77,78Ni; calculated total binding energies, S(2n), rms charge radii. 16O, 40Ca, 58Ni; calculated charge density distribution. 47,49,53,55Ca, 53K, 55Sc; calculated levels, J, π populated in one-neutron removal and addition from and to 48Ca and 54Ca. 37,39,41,43,45,47,49,51,53,55K; calculated energies of the first excited states. 16O, 36Ca, 56Ni; calculated binding energies. 18O, 52Ca, 64Ni; calculated rms charge radii. 39K, 49,53Ca; calculated one-nucleon separation energies. 16,22,24O, 36,40,48,52,54,60Ca, 48,56,68Ni; calculated binding energy per particle for doubly closed-shell nuclei. State-of-the-art no-core shell model and self-consistent Green's function approaches with NN+3N(lnl) interaction, and with comparisons made with NNLOsat and NN+3N(400) interactions, and with experimental data.
doi: 10.1103/PhysRevC.101.014318
2020SU06 Phys.Lett. B 802, 135215 (2020) Y.L.Sun, A.Obertelli, P.Doornenbal, C.Barbieri, Y.Chazono, T.Duguet, H.N.Liu, P.Navratil, F.Nowacki, K.Ogata, T.Otsuka, F.Raimondi, V.Soma, Y.Utsuno, K.Yoshida, N.Achouri, H.Baba, F.Browne, D.Calvet, F.Chateau, S.Chen, N.Chiga, A.Corsi, M.L.Cortes, A.Delbart, J.-M.Gheller, A.Giganon, A.Gillibert, C.Hilaire, T.Isobe, T.Kobayashi, Y.Kubota, V.Lapoux, T.Motobayashi, I.Murray, H.Otsu, V.Panin, N.Paul, W.Rodriguez, H.Sakurai, M.Sasano, D.Steppenbeck, L.Stuhl, Y.Togano, T.Uesaka, K.Wimmer, K.Yoneda, O.Aktas, T.Aumann, L.X.Chung, F.Flavigny, S.Franchoo, I.Gasparic, R.-B.Gerst, J.Gibelin, K.I.Hahn, D.Kim, T.Koiwai, Y.Kondo, P.Koseoglou, J.Lee, C.Lehr, B.D.Linh, T.Lokotko, M.MacCormick, K.Moschner, T.Nakamura, S.Y.Park, D.Rossi, E.Sahin, D.Sohler, P.-A.Soderstrom, S.Takeuchi, H.Tornqvist, V.Vaquero, V.Wagner, S.Wang, V.Werner, X.Xu, H.Yamada, D.Yan, Z.Yang, M.Yasuda, L.Zanetti Restoration of the natural E(1/2+1)-E(3/2+1) energy splitting in odd-K isotopes towards N = 40 NUCLEAR REACTIONS 52,54Ca(p, 2p)51K/53K, E ∼ 250 MeV/nucleon; measured reaction products, Eγ, Iγ; deduced γ-ray energies, J, π, partial σ. Comparison with ab initio and shell-model calculations with improved phenomenological effective interactions.
doi: 10.1016/j.physletb.2020.135215
2019CH43 Phys.Rev.Lett. 123, 142501 (2019) S.Chen, J.Lee, P.Doornenbal, A.Obertelli, C.Barbieri, Y.Chazono, P.Navratil, K.Ogata, T.Otsuka, F.Raimondi, V.Soma, Y.Utsuno, K.Yoshida, H.Baba, F.Browne, D.Calvet, F.Chateau, N.Chiga, A.Corsi, M.L.Cortes, A.Delbart, J.-M.Gheller, A.Giganon, A.Gillibert, C.Hilaire, T.Isobe, J.Kahlbow, T.Kobayashi, Y.Kubota, V.Lapoux, H.N.Liu, T.Motobayashi, I.Murray, H.Otsu, V.Panin, N.Paul, W.Rodriguez, H.Sakurai, M.Sasano, D.Steppenbeck, L.Stuhl, Y.L.Sun, Y.Togano, T.Uesaka, K.Wimmer, K.Yoneda, N.Achouri, O.Aktas, T.Aumann, L.X.Chung, F.Flavigny, S.Franchoo, I.Gasparic, R.-B.Gerst, J.Gibelin, K.I.Hahn, D.Kim, T.Koiwai, Y.Kondo, P.Koseoglou, C.Lehr, B.D.Linh, T.Lokotko, M.MacCormick, K.Moschner, T.Nakamura, S.Y.Park, D.Rossi, E.Sahin, D.Sohler, P.-A.Soderstrom, S.Takeuchi, H.Tornqvist, V.Vaquero, V.Wagner, S.Wang, V.Werner, X.Xu, H.Yamada, D.Yan, Z.Yang, M.Yasuda, L.Zanetti Quasifree Neutron Knockout from 54Ca Corroborates Arising N=34 Neutron Magic Number NUCLEAR REACTIONS 1H(54Ca, X)53Ca, E=216 MeV/nucleon; measured reaction products, Eγ, Iγ; deduced γ-ray energies, exclusive σ, inclusive parallel momentum distributions. Comparison with theoretical calculations.
doi: 10.1103/PhysRevLett.123.142501
2019RA12 Phys.Rev. C 99, 054327 (2019) Nuclear electromagnetic dipole response with the self-consistent Green's function formalism NUCLEAR REACTIONS 14,16,22,24O, 36,40,48,52,54,70Ca, 68Ni(γ, X), E*=0-70 MeV; calculated integrated isovector E1 photoabsorption σ(E), isovector dipole polarizabilities, and isovector dipole response function, excitation energies of pygmy dipole resonances (PDR) and giant dipole resonance (GDR) for 68Ni, integrated E1 strength of 16O above the GDR. self-consistent Green's function (SCGF) formalism, with the single-particle propagator obtained by solving the Dyson equation, and the particle-hole (ph) polarization propagator treated in the dressed random phase approximation (DRPA). Comparison with experimental data.
doi: 10.1103/PhysRevC.99.054327
2019RA20 Phys.Rev. C 100, 024317 (2019) Core-polarization effects and effective charges in O and Ni isotopes from chiral interactions NUCLEAR STRUCTURE 14,16,22,24O, 48,56,68,78Ni; calculated isoscalar E2 effective charges for the 0p1s0d and 1p0f0g9/2 valence spaces, core-polarization effects, quasiparticle energies, point-neutron and point-proton intrinsic radii. Ab initio approach through microscopic theory within the self-consistent Green's function (SCGF) formalism.
doi: 10.1103/PhysRevC.100.024317
2018RA06 Phys.Rev. C 97, 054308 (2018) Algebraic diagrammatic construction formalism with three-body interactions
doi: 10.1103/PhysRevC.97.054308
2016DO04 Phys.Lett. B 757, 430 (2016) J.Dohet-Eraly, P.Navratil, S.Quaglioni, W.Horiuchi, G.Hupin, F.Raimondi 3He(α, γ)7Be and 3H(α, γ)7Li astrophysical S factors from the no-core shell model with continuum NUCLEAR REACTIONS 3He, 3H(α, γ), E<4 MeV; calculated S-factors, σ using no-core shell model. Comparison with available data.
doi: 10.1016/j.physletb.2016.04.021
2016RA17 Phys.Rev. C 93, 054606 (2016) F.Raimondi, G.Hupin, P.Navratil, S.Quaglioni Deuteron-induced nucleon transfer reactions within an ab initio framework: First application to p-shell nuclei NUCLEAR REACTIONS 7Li(d, d), E=0.6-1.8 MeV; 7Li(d, p), E=0.25-2.5 MeV; calculated differential and integrated σ(E), eigenphase shifts, resonant phase shifts, contribution of dominant partial waves. Ab initio method using no-core shell model (NCS) and microscopic-cluster states in the framework of resonating group method (RGM). Comparison with experimental cross section data. Relevance to formation of nuclei in primordial and stellar nucleosynthesis. NUCLEAR STRUCTURE 7,8Li, 9Be; calculated levels, J, π. 2H; calculated ground-state and pseudostate energies. No-core shell model (NCS) approach. Comparison with experimental data.
doi: 10.1103/PhysRevC.93.054606
2014RA08 J.Phys.(London) G41, 055112 (2014) F.Raimondi, K.Bennaceur, J.Dobaczewski Nonlocal energy density functionals for low-energy nuclear structure
doi: 10.1088/0954-3899/41/5/055112
2011RA13 Phys.Rev. C 83, 054311 (2011) F.Raimondi, B.G.Carlsson, J.Dobaczewski Effective pseudopotential for energy density functionals with higher-order derivatives
doi: 10.1103/PhysRevC.83.054311
2011RA40 Phys.Rev. C 84, 064303 (2011) F.Raimondi, B.G.Carlsson, J.Dobaczewski, J.Toivanen Continuity equation and local gauge invariance for the N3LO nuclear energy density functionals
doi: 10.1103/PhysRevC.84.064303
2010BA24 Phys.Rev. C 82, 015807 (2010) S.Baroni, A.Pastore, F.Raimondi, F.Barranco, R.A.Broglia, E.Vigezzi Finite-size effects and collective vibrations in the inner crust of neutron stars NUCLEAR STRUCTURE 176,506Sn, 498Zr; calculated levels, J, π, energies of single-particle orbitals, energies of 2+ and 3- collective excitations, and mean-field potentials Wigner-Seitz approximation. Relevance to collective excitations of nuclei in neutron stars.
doi: 10.1103/PhysRevC.82.015807
Back to query form |