NSR Query Results
Output year order : Descending NSR database version of April 26, 2024. Search: Author = A.Carbone Found 16 matches. 2021MA52 Phys.Rev. C 104, 024315 (2021) F.Marino, C.Barbieri, A.Carbone, G.Colo, A.Lovato, F.Pederiva, X.Roca-Maza, E.Vigezzi Nuclear energy density functionals grounded in ab initio calculations NUCLEAR STRUCTURE 16O, 34Si, 36S, 36,40,48,52Ca, 90Zr, 132Sn, 208Pb; calculated energies per nucleon and charge radii by ab initio computation of equations of state (EoSs) of symmetric nuclear and pure neutron matter using the chiral NNLOsat-based nuclear energy density functional (EDF), and the phenomenological AV4+UIXc Hamiltonians. Comparison with experimental data. Discussed practical and systematic way to merge ab initio nuclear theory and density functional theory.
doi: 10.1103/PhysRevC.104.024315
2019CA20 Phys.Rev. C 100, 025805 (2019) Ab initio constraints on thermal effects of the nuclear equation of state
doi: 10.1103/PhysRevC.100.025805
2019XU11 Phys.Rev. C 100, 024618 (2019) J.Xu, A.Carbone, Z.Zhang, C.Ko Nuclear matter properties at finite temperatures from effective interactions
doi: 10.1103/PhysRevC.100.024618
2018CA20 Phys.Rev. C 98, 025804 (2018) Microscopic predictions of the nuclear matter liquid-gas phase transition
doi: 10.1103/PhysRevC.98.025804
2017KL03 Eur.Phys.J. A 53, 168 (2017); Erratum Eur.Phys.J. A 54, 76 (2018) P.Klos, A.Carbone, K.Hebeler, J.Menendez, A.Schwenk Uncertainties in constraining low-energy constants from 3H β decay RADIOACTIVITY 3H(β-); calculated low-energy constants of chiral effective field theory from T1/2; deduced uncertainty.
doi: 10.1140/epja/i2017-12357-7
2017RI07 Phys.Rev. C 96, 014003 (2017) Comparison of nuclear Hamiltonians using spectral function sum rules
doi: 10.1103/PhysRevC.96.014003
2016DI12 Phys.Rev. C 94, 025802 (2016); Pub.Note Phys.Rev. C 94, 029901 (2016) D.Ding, A.Rios, H.Dussan, W.H.Dickhoff, S.J.Witte, A.Carbone, A.Polls Pairing in high-density neutron matter including short- and long-range correlations
doi: 10.1103/PhysRevC.94.025802
2016DR13 Phys.Rev. C 94, 054307 (2016) C.Drischler, A.Carbone, K.Hebeler, A.Schwenk Neutron matter from chiral two- and three-nucleon calculations up to N3 LO
doi: 10.1103/PhysRevC.94.054307
2014CA04 Eur.Phys.J. A 50, 13 (2014) A.Carbone, A.Polls, C.Providencia, A.Rios, I.Vidana Tensor force effects and high-momentum components in the nuclear symmetry energy
doi: 10.1140/epja/i2014-14013-2
2014CA41 Phys.Rev. C 90, 054322 (2014) Correlated density-dependent chiral forces for infinite-matter calculations within the Green's function approach
doi: 10.1103/PhysRevC.90.054322
2013CA20 Phys.Rev. C 88, 044302 (2013) Symmetric nuclear matter with chiral three-nucleon forces in the self-consistent Green's functions approach
doi: 10.1103/PhysRevC.88.044302
2013CA24 Phys.Rev. C 88, 054326 (2013) A.Carbone, A.Cipollone, C.Barbieri, A.Rios, A.Polls Self-consistent Green's functions formalism with three-body interactions
doi: 10.1103/PhysRevC.88.054326
2012CA02 Europhys.Lett. 97, 22001 (2012) High-momentum components in the nuclear symmetry energy
doi: 10.1209/0295-5075/97/22001
2011CA03 Phys.Rev. C 83, 024308 (2011); Publishers Note Phys.Rev. C 83, 039901 (2011) A.Carbone, A.Polls, A.Rios, I.Vidana Latent heat of nuclear matter
doi: 10.1103/PhysRevC.83.024308
2010CA11 Phys.Rev. C 81, 041301 (2010) A.Carbone, G.Colo, A.Bracco, L.-G.Cao, P.F.Bortignon, F.Camera, O.Wieland Constraints on the symmetry energy and neutron skins from pygmy resonances in 68Ni and 132Sn NUCLEAR STRUCTURE 68Ni, 132Sn, 208Pb; calculated dipole strength function, neutron symmetry energy, neutron skin radius, and EWSR from pygmy dipole resonances using random-phase approximation (RPA). Comparison with experimental data.
doi: 10.1103/PhysRevC.81.041301
1997QU01 Nucl.Phys. A621, 345c (1997) P.Quarati, A.Carbone, G.Gervino, G.Kaniadakis, A.Lavagno, E.Miraldi Constraints for Solar Neutrinos Fluxes
doi: 10.1016/S0375-9474(97)00269-8
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