NSR Query Results
Output year order : Descending NSR database version of April 27, 2024. Search: Author = I.Bombaci Found 27 matches. 2022LO04 Eur.Phys.J. A 58, 55 (2022) D.Logoteta, I.Bombaci, A.Perego Isoentropic equations of state of β-stable hadronic matter with a quark phase transition
doi: 10.1140/epja/s10050-022-00708-8
2022LO07 Phys.Rev. C 105, 055808 (2022) A.Lovato, I.Bombaci, D.Logoteta, M.Piarulli, R.B.Wiringa Benchmark calculations of infinite neutron matter with realistic two- and three-nucleon potentials
doi: 10.1103/PhysRevC.105.055808
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
2020PI05 Phys.Rev. C 101, 045801 (2020) M.Piarulli, I.Bombaci, D.Logoteta, A.Lovato, R.B.Wiringa Benchmark calculations of pure neutron matter with realistic nucleon-nucleon interactions
doi: 10.1103/PhysRevC.101.045801
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
2018KI09 Phys.Rev.Lett. 121, 072701 (2018) A.Kievsky, M.Viviani, D.Logoteta, I.Bombaci, L.Girlanda Correlations imposed by the unitary limit between few-nucleon systems, nuclear matter, and neutron stars
doi: 10.1103/PhysRevLett.121.072701
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
2016LO17 Phys.Rev. C 94, 064001 (2016) D.Logoteta, I.Bombaci, A.Kievsky Nuclear matter properties from local chiral interactions with Δ isobar intermediate states
doi: 10.1103/PhysRevC.94.064001
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
2014ZU02 Eur.Phys.J. A 50, 12 (2014) Three-body force effect on nuclear symmetry energy and single-particle properties of asymmetric nuclear matter
doi: 10.1140/epja/i2014-14001-6
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
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
2007BO13 Eur.Phys.J. A 31, 810 (2007) Neutron stars as cosmic laboratories to explore hadronic matter at ultra-high densities
doi: 10.1140/epja/i2006-10266-6
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
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
2005BO21 Nucl.Phys. A754, 335c (2005) Strangeness in neutron stars
doi: 10.1016/j.nuclphysa.2005.01.023
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
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
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
2001BO05 Nucl.Phys. A681, 205c (2001) Possible Signatures for Deconfined Strange Quark Matter in Compact Stars
doi: 10.1016/S0375-9474(00)00504-2
1999ZU01 Phys.Rev. C60, 024605 (1999) Asymmetric Nuclear Matter from an Extended Brueckner-Hartree-Fock Approach
doi: 10.1103/PhysRevC.60.024605
1997BO06 Phys.Rev. C55, 1587 (1997) Observational Evidence for Strange Matter in Compact Objects from the X-Ray Burster 4U 1820-30
doi: 10.1103/PhysRevC.55.1587
1995BA13 Nucl.Phys. A583, 599c (1995) M.Baldo, G.Giansiracusa, U.Lombardo, I.Bombaci, L.S.Ferreira Microscopic Theory of the Nuclear Equation of State
doi: 10.1016/0375-9474(94)00733-4
1995BO09 Nucl.Phys. A583, 623c (1995) I.Bombaci, M.Prakash, M.Prakash, P.J.Ellis, J.M.Lattimer, G.E.Brown Newborn Hot Neutron Stars
doi: 10.1016/0375-9474(94)00736-7
1991BA35 Nucl.Phys. A530, 135 (1991) M.Baldo, I.Bombaci, G.Giansiracusa, U.Lombardo Momentum Distribution and Hole Strength from a Separable Representation of the Argonne v14 Interaction NUCLEAR STRUCTURE 90Zr, 208Pb; calculated quasi hole strength, hole-state spectroscopic factor. Brueckner-Bethe-Goldstone theory, realistic interactions, momentum distribution.
doi: 10.1016/0375-9474(91)90759-Y
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