NSR Query Results


Output year order : Descending
Format : Normal

NSR database version of May 21, 2024.

Search: Author = F.Raimondi

Found 12 matches.

Back to query form



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
Citations: PlumX Metrics


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
Citations: PlumX Metrics

Data from this article have been entered in the XUNDL database. For more information, click here.


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
Citations: PlumX Metrics

Data from this article have been entered in the EXFOR database. For more information, access X4 datasetE2644. Data from this article have been entered in the XUNDL database. For more information, click here.


2019RA12      Phys.Rev. C 99, 054327 (2019)

F.Raimondi, C.Barbieri

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
Citations: PlumX Metrics


2019RA20      Phys.Rev. C 100, 024317 (2019)

F.Raimondi, C.Barbieri

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
Citations: PlumX Metrics


2018RA06      Phys.Rev. C 97, 054308 (2018)

F.Raimondi, C.Barbieri

Algebraic diagrammatic construction formalism with three-body interactions

doi: 10.1103/PhysRevC.97.054308
Citations: PlumX Metrics


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
Citations: PlumX Metrics


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
Citations: PlumX Metrics


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
Citations: PlumX Metrics


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
Citations: PlumX Metrics


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
Citations: PlumX Metrics


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
Citations: PlumX Metrics


Back to query form