NSR Query Results
Output year order : Descending NSR database version of April 11, 2024. Search: Author = I.Vidana Found 68 matches. 2024KU07 Eur.Phys.J. A 60, (2024) C.V.N.Kumar, L.M.Robledo, I.Vidana Structure of single Λ-hypernuclei with Gogny-type Λ-nucleon forces NUCLEAR STRUCTURE 16O, 28Si, 32S, 40Ca, 51V, 89Y, 139La, 208Pb; calculated binding energies of Λ single-particle states with the three ΛN Gogny-type forces, hypernuclei ground-state HFB and pairing energy, quadrupole moments.
doi: 10.1140/epja/s10050-024-01278-7
2023BE12 Eur.Phys.J. A 59, 159 (2023) O.G.Benvenuto, E.Bauer, I.Vidana Hot and highly magnetized neutron star matter properties with Skyrme interactions
doi: 10.1140/epja/s10050-023-01070-z
2023RO03 Phys.Rev.Lett. 130, 132501 (2023) J.L.Rodriguez-Sanchez, J.Cugnon, J.-C.David, J.Hirtz, A.Kelic-Heil, I.Vidana Constraint of the Nuclear Dissipation Coefficient in Fission of Hypernuclei NUCLEAR REACTIONS 209Bi, 238U(p, F), E=1-2.4 GeV/nucleon; calculated hypernuclear fission σ. Comparison with experimental data.
doi: 10.1103/PhysRevLett.130.132501
2023VI01 Nucl.Phys. A1032, 122625 (2023) Machine learning light hypernuclei NUCLEAR STRUCTURE 3,4H, 4He; calculated separation energies, energy levels, J, π using a feed-forward artificial neural network to extrapolate at large model spaces. Comparison with available data.
doi: 10.1016/j.nuclphysa.2023.122625
2022KO08 Eur.Phys.J. A 58, 31 (2022) H.Kochankovski, A.Ramos, I.Vidana An analytic parametrization of the hypernuclear matter equation of state
doi: 10.1140/epja/s10050-022-00669-y
2022RO11 Phys.Rev. C 106, 014618 (2022) J.L.Rodriguez-Sanchez, J.Benlliure, I.Vidana, H.Lenske, J.Vargas, C.Scheidenberger, H.Alvarez-Pol, J.Atkinson, T.Aumann, Y.Ayyad, S.Beceiro Novo, K.Boretzky, M.Caamano, E.Casarejos, D.Cortina-Gil, P.Diaz Fernandez, A.Estrade, H.Geissel, E.Haettner, A.Kelic-Heil, Yu.A.Litvinov, C.Paradela, D.Perez-Loureiro, S.Pietri, A.Prochazka, M.Takechi, Y.K.Tanaka, H.Weick, J.S.Winfield Systematic study of Δ(1232) resonance excitations using single isobaric charge-exchange reactions induced by medium-mass projectiles of Sn NUCLEAR REACTIONS 1H, 12C, Cu, Pb(112Sn, 112In), (112Sn, 112Sb), 1H, C(124Sn, 124Sb), E=1 GeV/nucleon; measured reaction products; deduced total σ, quasielastic and inelastic σ; missing energy spectra. Observed energy shift for the Δ-resonance peak of about 63 ± 5 MeV and quenching of the quasielastic component. Comparison to theoretical predictions using random phase approximation (RPA) with Giessen energy density functional (GiEDF). FRS spectrometer with SIS-18 synchrotron beam (GSI).
doi: 10.1103/PhysRevC.106.014618
2022VI05 Phys.Rev. C 106, 035804 (2022) I.Vidana, D.Logoteta, I.Bombaci Effect of chiral nuclear forces on the neutrino mean free path in hot neutron matter
doi: 10.1103/PhysRevC.106.035804
2021BO11 Phys.Rev.Lett. 126, 162702 (2021) I.Bombaci, A.Drago, D.Logoteta, G.Pagliara, I.Vidana Was GW190814 a Black Hole-Strange Quark Star System?
doi: 10.1103/PhysRevLett.126.162702
2021BU11 Prog.Part.Nucl.Phys. 120, 103879 (2021) G.F.Burgio, H.-J.Schulze, I.Vidana, J.-B.Wei Neutron stars and the nuclear equation of state
doi: 10.1016/j.ppnp.2021.103879
2021HU03 Phys.Rev. C 103, 024601 (2021) P.N.Huan, N.L.Anh, B.M.Loc, I.Vidana Excitation of isobaric analog states from (p, n) and (3He, t) charge-exchange reactions within the G-matrix folding method NUCLEAR REACTIONS 12C, 40Ca(p, p), E=160 MeV; 58Ni, 90Zr(3He, 3He), E=443 MeV; 208Pb(3He, 3He), E=450 MeV; 14C(p, n)14N, E=135 MeV; 48Ca(p, n)48Sc, E=134, 160 MeV; 58Ni, 90Zr, 208Pb(3He, t), E=420 MeV; calculated differential σ(θ) and compared with experimental data. Distorted wave Born approximation with the G-matrix double-folding method for nucleus-nucleus optical potential within the framework of the Lane model, and G matrices from a Brueckner-Hartree-Fock calculation using the Argonne Av18 nucleon-nucleon potential.
doi: 10.1103/PhysRevC.103.024601
2021VI04 Phys.Rev. C 103, L052801 (2021) Fermi polaron in low-density spin-polarized neutron matter
doi: 10.1103/PhysRevC.103.L052801
2020HA08 Eur.Phys.J. A 56, 55 (2020) Structure of single-Λ hypernuclei with chiral hyperon-nucleon potentials
doi: 10.1140/epja/s10050-020-00055-6
2020HA22 Eur.Phys.J. A 56, 195 (2020) J.Haidenbauer, A.Nogga, I.Vidana Predictions for charmed nuclei based on YcN forces inferred from lattice QCD simulations
doi: 10.1140/epja/s10050-020-00185-x
2020PO11 Phys.Rev. C 102, 054004 (2020) Spinodal instabilities of spin-polarized asymmetric nuclear matter
doi: 10.1103/PhysRevC.102.054004
2020RO12 Phys.Lett. B 807, 135565 (2020) J.L.Rodriguez-Sanchez, J.Benlliure, I.Vidana, H.Lenske, C.Scheidenberger, J.Vargas, H.Alvarez-Pol, J.Atkinson, T.Aumann, Y.Ayyad, S.Beceiro Novo, K.Boretzky, M.Caamano, E.Casarejos, D.Cortina-Gil, P.Diaz Fernandez, A.Estrade, H.Geissel, E.Haettner, A.Kelic-Heil, Yu.A.Litvinov, C.Paradela, D.Perez-Loureiro, S.Pietri, A.Prochazka, M.Takechi, Y.K.Tanaka, H.Weick, J.S.Winfield Study of Δ excitations in medium-mass nuclei with peripheral heavy ion charge-exchange reactions NUCLEAR REACTIONS C(112Sn, 112In), E=1 GeV/nucleon; analyzed available data; deduced missing spectra, change in the relative magnitude between the contribution of the excitation of the resonance in the target and in the projectile.
doi: 10.1016/j.physletb.2020.135565
2019LO15 Eur.Phys.J. A 55, 207 (2019) D.Logoteta, I.Vidana, I.Bombaci Impact of chiral hyperonic three-body forces on neutron stars
doi: 10.1140/epja/i2019-12909-9
2019TO06 Phys.Rev. C 99, 045808 (2019) J.Torres Patino, E.Bauer, I.Vidana Asymmetry of the neutrino mean free path in hot neutron matter under strong magnetic fields
doi: 10.1103/PhysRevC.99.045808
2019VI03 Phys.Rev. C 99, 045208 (2019) I.Vidana, A.Ramos, C.E.Jimenez-Tejero Charmed nuclei within a microscopic many-body approach
doi: 10.1103/PhysRevC.99.045208
2017FO12 Phys.Rev. C 95, 065803 (2017) M.Fortin, S.S.Avancini, C.Providencia, I.Vidana Hypernuclei and massive neutron stars NUCLEAR STRUCTURE 6He; calculated binding energy of double-Λ 6He hypernucleus as a calibrant using several different models, and compared to experimental data. Construction of unified hyperonic EoS for massive neutron stars with limited number of constraints set by phenomenological models.
doi: 10.1103/PhysRevC.95.065803
2017VI01 Nucl.Phys. A958, 48 (2017) Single-particle spectral function of the Λ hyperon in finite nuclei NUCLEAR STRUCTURE 5He, 13C, 17O, 41Ca, 91Zr, 209Pb; calculated Λ hypernuclei self-energy, mass excess, root-mean square radius, spectral strength, disoccupation number of different states using JB (Juelich B model) and NSC (Nijmegen soft-core models).
doi: 10.1016/j.nuclphysa.2016.11.002
2016BO07 Eur.Phys.J. A 52, 58 (2016) I.Bombaci, D.Logoteta, I.Vidana, C.Providencia Quark matter nucleation in neutron stars and astrophysical implications
doi: 10.1140/epja/i2016-16058-5
2016CH08 Eur.Phys.J. A 52, 29 (2016) Do hyperons exist in the interior of neutron stars?
doi: 10.1140/epja/i2016-16029-x
2016VI03 Phys.Rev. C 94, 054006 (2016) Role of correlations in spin-polarized neutron matter
doi: 10.1103/PhysRevC.94.054006
2015LO06 Phys.Rev. C 91, 064001 (2015) D.Logoteta, I.Vidana, I.Bombaci, A.Kievsky Comparative study of three-nucleon force models in nuclear matter NUCLEAR STRUCTURE 3H, 3,4He; calculated Energy per particle E/A of nuclear and pure neutron matter, binding energies of 3H, 3,4He, neutron-deuteron doublet scattering length, and symmetry energy. Microscopic many-body Brueckner-Hartree-Fock (BHF) approach with Argonne V18 (AV18) nucleon-nucleon (NN) potential using two three-nucleon force models.
doi: 10.1103/PhysRevC.91.064001
2015RA06 Phys.Rev. C 91, 045803 (2015) A.Rabhi, M.A.Perez-Garcia, C.Providencia, I.Vidana Magnetic susceptibility and magnetization properties of asymmetric nuclear matter in a strong magnetic field
doi: 10.1103/PhysRevC.91.045803
2014AG03 Phys.Rev. C 89, 035809 (2014) Neutron matter under strong magnetic fields: A comparison of models
doi: 10.1103/PhysRevC.89.035809
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
2014GR14 Phys.Rev. C 90, 045803 (2014) F.Grill, H.Pais, C.Providencia, Is.Vidana, S.S.Avancini Equation of state and thickness of the inner crust of neutron stars
doi: 10.1103/PhysRevC.90.045803
2014LI05 Eur.Phys.J. A 50, 9 (2014) B.-A.Li, A.Ramos, G.Verde, I.Vidana Topical issue on nuclear symmetry energy
doi: 10.1140/epja/i2014-14009-x
2014PR02 Eur.Phys.J. A 50, 44 (2014) C.Providencia, S.S.Avancini, R.Cavagnoli, S.Chiacchiera, C.Ducoin, F.Grill, J.Margueron, D.P.Menezes, A.Rabh, I.Vidana Imprint of the symmetry energy on the inner crust and strangeness content of neutron stars
doi: 10.1140/epja/i2014-14044-7
2013LO11 Nucl.Phys. A914, 433c (2013) D.Logoteta, I.Vidana, C.Providencia Two-meson exchange hyperonic three-body forces and consequences for neutron stars
doi: 10.1016/j.nuclphysa.2013.01.022
2013LO14 Phys.Rev. C 88, 055802 (2013) D.Logoteta, C.Providencia, I.Vidana Formation of hybrid stars from metastable hadronic stars
doi: 10.1103/PhysRevC.88.055802
2013VI03 Nucl.Phys. A914, 367c (2013) Hyperons and neutron stars
doi: 10.1016/j.nuclphysa.2013.01.015
2012BA57 Phys.Rev. C 86, 064001 (2012) M.Baldo, A.Polls, A.Rios, H.-J.Schulze, I.Vidana Comparative study of neutron and nuclear matter with simplified Argonne nucleon-nucleon potentials
doi: 10.1103/PhysRevC.86.064001
2012KH08 Phys.Rev.Lett. 109, 092501 (2012) Constraining the Nuclear Equation of State at Subsaturation Densities NUCLEAR STRUCTURE 208Pb; calculated matter density, energy per unit of volume at the crossing density. Comparison with available data.
doi: 10.1103/PhysRevLett.109.092501
2012LO06 Phys.Rev. C 85, 055807 (2012) D.Logoteta, C.Providencia, I.Vidana, I.Bombaci Quark matter nucleation with a microscopic hadronic equation of state
doi: 10.1103/PhysRevC.85.055807
2012LU19 Eur.Phys.J. A 48, 124 (2012) On kinematical constraints in boson-boson systems
doi: 10.1140/epja/i2012-12124-4
2012TS04 Phys.Rev. C 86, 015803 (2012) M.B.Tsang, J.R.Stone, F.Camera, P.Danielewicz, S.Gandolfi, K.Hebeler, C.J.Horowitz, J.Lee, W.G.Lynch, Z.Kohley, R.Lemmon, P.Moller, T.Murakami, S.Riordan, X.Roca-Maza, F.Sammarruca, A.W.Steiner, I.Vidana, S.J.Yennello Constraints on the symmetry energy and neutron skins from experiments and theory NUCLEAR STRUCTURE 208Pb; analyzed neutron-skin thickness, symmetry energy constraints. Contributions of three-body forces in neutron matter models.
doi: 10.1103/PhysRevC.86.015803
2012VI02 Phys.Rev. C 85, 045808 (2012); Erratum Phys.Rev. C 90, 029901 (2014) Nuclear symmetry energy and the r-mode instability of neutron stars
doi: 10.1103/PhysRevC.85.045808
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
2011DU13 Phys.Rev. C 83, 045810 (2011) C.Ducoin, J.Margueron, C.Providencia, I.Vidana Core-crust transition in neutron stars: Predictivity of density developments
doi: 10.1103/PhysRevC.83.045810
2011JI06 Phys.Rev. C 84, 015208 (2011) C.E.Jimenez-Tejero, A.Ramos, L.Tolos, I.Vidana Open-charm mesons in nuclear matter at finite temperature beyond the zero-range approximation
doi: 10.1103/PhysRevC.84.015208
2011VI07 Phys.Rev. C 84, 062801 (2011) I.Vidana, A.Polls, C.Providencia Nuclear symmetry energy and the role of the tensor force
doi: 10.1103/PhysRevC.84.062801
2010BE04 Phys.Rev. C 81, 024305 (2010) O.Benhar, A.Polls, M.Valli, I.Vidana Microscopic calculations of transport properties of neutron matter
doi: 10.1103/PhysRevC.81.024305
2009FL02 Phys.Rev. C 79, 064617 (2009) F.Flavigny, A.Obertelli, I.Vidana Medium effects on intermediate-energy one-nucleon removal cross sections NUCLEAR REACTIONS 9Be(24Si, X)23Si, E=30-1000 MeV/nucleon; 9Be(26Ne, X)25Ne, E=83.0 MeV/nucleon; 9Be(32Ar, X)31Ar, E=65.1 MeV/nucleon; 9Be(46Ar, X)45Ar, E=70.0 MeV/nucleon; 12C(16C, X)15C, E=55 MeV/nucleon; 12C(20O, X)19O, E=62.0 MeV/nucleon; 9Be(24Si, X)23Al, E=85.3 MeV/nucleon; 9Be(40Ca, X)39Ca, 9Be(42Ca, X)40Ca, 9Be(44Ca, X)43Ca, 9Be(46Ca, X)45Ca, 9Be(48Ca, X)47Ca, 9Be(50Ca, X)49Ca, 9Be(52Ca, X)51Ca, E=80 MeV/nucleon; calculated σ for neutron and proton knockout reactions using S-matrix formalism under Glauber approximation. Brueckner-Hartree-Fock (BHF) theory. Comparison with experimental data.
doi: 10.1103/PhysRevC.79.064617
2009JI09 Phys.Rev. C 80, 055206 (2009) C.E.Jimenez-Tejero, A.Ramos, I.Vidana Dynamically generated open-charm baryons beyond the zero-range approximation
doi: 10.1103/PhysRevC.80.055206
2009RI01 Phys.Rev. C 79, 025802 (2009) Hot neutron matter from a self-consistent Green's-functions approach
doi: 10.1103/PhysRevC.79.025802
2009VI07 Phys.Rev. C 80, 045806 (2009) I.Vidana, C.Providencia, A.Polls, A.Rios Density dependence of the nuclear symmetry energy: A microscopic perspective NUCLEAR STRUCTURE 132Sn, 208Pb; calculated neutron skin thickness, and transition densities using microscopic Brueckner-Hartree-Fock approach using the realistic AV18 potential plus a three-body force of Urbana type.
doi: 10.1103/PhysRevC.80.045806
2008VI03 J.Phys.(London) G35, 014054 (2008) I.Vidana, G.Lugones, I.Bombaci Role of color superconductivity on the nucleation of quark matter in neutron stars
doi: 10.1088/0954-3899/35/1/014054
2008ZH25 Phys.Rev. C 78, 054306 (2008) X.-R.Zhou, A.Polls, H.-J.Schulze, I.Vidana Λ hyperons and the neutron drip line NUCLEAR STRUCTURE 6,7,8,9,10,11,12,13,14,15,16,17,18,19,20Be, 22,23,24,25,26,27,28O; calculated neutron single-particle levels, binding energies, quadrupole deformations. Hypernuclei. Skyrme Hartree-Fock calculations. Comparison with experimental data.
doi: 10.1103/PhysRevC.78.054306
2006BO06 Phys.Lett. B 632, 638 (2006) I.Bombaci, A.Polls, A.Ramos, A.Rios, I.Vidana Microscopic calculations of spin polarized neutron matter at finite temperature
doi: 10.1016/j.physletb.2005.08.136
2006LO17 Phys.Rev.C 74, 068801 (2006) D.Lopez-Val, A.Rios, A.Polls, I.Vidana Ferromagnetic instabilities in neutron matter at finite temperature with the Gogny interaction
doi: 10.1103/PhysRevC.74.068801
2006SC14 Phys.Rev. C 73, 058801 (2006) H.-J.Schulze, A.Polls, A.Ramos, I.Vidana Maximum mass of neutron stars
doi: 10.1103/PhysRevC.73.058801
2005BO05 Phys.Lett. B 609, 232 (2005) I.Bombaci, A.Fabrocini, A.Polls, I.Vidana Spin-orbit and tensor interactions in homogeneous matter of nucleons: accuracy of modern many-body theories
doi: 10.1016/j.physletb.2005.01.067
2005RI06 Phys.Rev. C 71, 055802 (2005) Ferromagnetic instabilities in neutron matter at finite temperature with the Skyrme interaction
doi: 10.1103/PhysRevC.71.055802
2005RI12 Phys.Rev. C 72, 024316 (2005) A.Rios, A.Polls, A.Ramos, I.Vidana Bulk and single-particle properties of hyperonic matter at finite temperature
doi: 10.1103/PhysRevC.72.024316
2005VI09 Nucl.Phys. A754, 345c (2005) I.Vidana, I.Bombaci, I.Parenti Role of hyperons on the hadron-star to quark-star conversion mechanism
doi: 10.1016/j.nuclphysa.2005.02.081
2004VI08 Phys.Rev. C 70, 024306 (2004) ΛΛ bond energy from the Nijmegen potentials NUCLEAR STRUCTURE 6He, 10Be, 13B; calculated two-Λ hypernucleus bond energies. Microscopic approach, comparison with data.
doi: 10.1103/PhysRevC.70.024306
2004VI09 Phys.Rev. C 70, 028802 (2004) Superfluidity of Σ- hyperons in β-stable neutron star matter
doi: 10.1103/PhysRevC.70.028802
2003MA76 Phys.Rev. C 68, 055806 (2003) J.Margueron, I.Vidana, I.Bombaci Microscopic calculation of the neutrino mean free path inside hot neutron matter
doi: 10.1103/PhysRevC.68.055806
2003VI07 Nucl.Phys. A719, 173c (2003) I.Vidana, I.Bombaci, A.Polls, A.Ramos Neutrino trapping effects on β-stable neutron star matter
doi: 10.1016/S0375-9474(03)00913-8
2002VI03 Phys.Rev. C65, 035804 (2002) Spin Polarized Neutron Matter and Magnetic Susceptibility within the Brueckner-Hartree-Fock Approximation
doi: 10.1103/PhysRevC.65.035804
2002VI09 Phys.Rev. C66, 045801 (2002) Equation of state and magnetic susceptibility of spin polarized isospin asymmetric nuclear matter
doi: 10.1103/PhysRevC.66.045801
2001VI10 Phys.Rev. C64, 044301 (2001) I.Vidana, A.Polls, A.Ramos, H.-J.Schulze Hypernuclear Structure with the New Nijmegen Potentials NUCLEAR STRUCTURE 13C, 17O, 29Si, 41Ca, 91Zr, 141Ce, 209Pb; calculated hypernucleus Λ single-particle levels. 10Be, 14C, 18O, 30Si, 42Ca, 92Zr, 142Ce, 210Pb; calculated two-Λ hypernucleus bond energies. Comparisons with data.
doi: 10.1103/PhysRevC.64.044301
2001VI12 Nucl.Phys. A691, 443c (2001) I.Vidana, A.Polls, A.Ramos, L.Engvik, M.Hjorth-Jensen Hyperon Effects on the Properties of β-Stable Neutron Star Matter
doi: 10.1016/S0375-9474(01)01071-5
2000VI02 Phys.Rev. C61, 025802 (2000) I.Vidana, A.Polls, A.Ramos, M.Hjorth-Jensen, V.G.J.Stoks Strange Nuclear Matter within Brueckner-Hartree-Fock Theory
doi: 10.1103/PhysRevC.61.025802
2000VI07 Phys.Rev. C62, 035801 (2000) I.Vidana, A.Polls, A.Ramos, L.Engvik, M.Hjorth-Jensen Hyperon-Hyperon Interactions and Properties of Neutron Star Matter
doi: 10.1103/PhysRevC.62.035801
1998VI07 Nucl.Phys. A644, 201 (1998) I.Vidana, A.Polls, A.Ramos, M.Hjorth-Jensen Hyperon Properties in Finite Nuclei using Realistic YN Interactions NUCLEAR STRUCTURE 13C, 17O, 41Ca, 91Zr, 209Pb; calculated hypernuclei single-particle energies. Realistic hyperon-nucleon interactions, implications for mesonic weak decay discussed.
doi: 10.1016/S0375-9474(98)00599-5
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