| Estimation of the effect of hyperonic three-body forces on the maximum mass of neutron stars I Vidana, D Logoteta, C Providência, A Polls, I Bombaci Europhysics Letters 94 (1), 11002, 2011 | 178 | 2011 |
| Numerical relativity simulations of the neutron star merger GW170817: long-term remnant evolutions, winds, remnant disks, and nucleosynthesis V Nedora, S Bernuzzi, D Radice, B Daszuta, A Endrizzi, A Perego, ... The Astrophysical Journal 906 (2), 98, 2021 | 143 | 2021 |
| Accretion-induced prompt black hole formation in asymmetric neutron star mergers, dynamical ejecta, and kilonova signals S Bernuzzi, M Breschi, B Daszuta, A Endrizzi, D Logoteta, V Nedora, ... Monthly Notices of the Royal Astronomical Society 497 (2), 1488-1507, 2020 | 109 | 2020 |
| Was GW190814 a black hole–strange quark star system? I Bombaci, A Drago, D Logoteta, G Pagliara, I Vidaña Physical Review Letters 126 (16), 162702, 2021 | 106 | 2021 |
| Equation of state of dense nuclear matter and neutron star structure from nuclear chiral interactions I Bombaci, D Logoteta Astronomy & Astrophysics 609, A128, 2018 | 106 | 2018 |
| Quark matter nucleation in hot hadronic matter I Bombaci, D Logoteta, PK Panda, C Providencia, I Vidana Physics Letters B 680 (5), 448-452, 2009 | 90 | 2009 |
| Quark matter nucleation in neutron stars and astrophysical implications I Bombaci, D Logoteta, I Vidana, C Providência The European Physical Journal A 52 (3), 58, 2016 | 85 | 2016 |
| Signatures of deconfined quark phases in binary neutron star mergers A Prakash, D Radice, D Logoteta, A Perego, V Nedora, I Bombaci, ... Physical Review D 104 (8), 083029, 2021 | 84 | 2021 |
| Impact of chiral hyperonic three-body forces on neutron stars D Logoteta, I Vidana, I Bombaci The European Physical Journal A 55 (11), 207, 2019 | 78 | 2019 |
| Benchmark calculations of pure neutron matter with realistic nucleon-nucleon interactions M Piarulli, I Bombaci, D Logoteta, A Lovato, RB Wiringa Physical Review C 101 (4), 045801, 2020 | 76 | 2020 |
| Nuclear matter properties from local chiral interactions with isobar intermediate states D Logoteta, I Bombaci, A Kievsky Physical Review C 94 (6), 064001, 2016 | 52 | 2016 |
| Correlations imposed by the unitary limit between few-nucleon systems, nuclear matter, and neutron stars A Kievsky, M Viviani, D Logoteta, I Bombaci, L Girlanda Physical Review Letters 121 (7), 072701, 2018 | 51 | 2018 |
| Numerical relativity simulations of prompt collapse mergers: Threshold mass and phenomenological constraints on neutron star properties after GW170817 R Kashyap, A Das, D Radice, S Padamata, A Prakash, D Logoteta, ... Physical Review D 105 (10), 103022, 2022 | 50 | 2022 |
| Fast spinning strange stars: possible ways to constrain interacting quark matter parameters S Bhattacharyya, I Bombaci, D Logoteta, AV Thampan Monthly Notices of the Royal Astronomical Society 457 (3), 3101-3114, 2016 | 50 | 2016 |
| Quark deconfinement transition in neutron stars with the field correlator method D Logoteta, I Bombaci Physical Review D—Particles, Fields, Gravitation, and Cosmology 88 (6), 063001, 2013 | 49 | 2013 |
| Effects of quark matter nucleation on the evolution of proto-neutron stars I Bombaci, D Logoteta, C Providência, I Vidana Astronomy & Astrophysics 528, A71, 2011 | 48 | 2011 |
| Effects of chiral effective field theory equation of state on binary neutron star mergers A Endrizzi, D Logoteta, B Giacomazzo, I Bombaci, W Kastaun, R Ciolfi Physical Review D 98 (4), 043015, 2018 | 46 | 2018 |
| Formation of hybrid stars from metastable hadronic stars D Logoteta, C Providência, I Vidana Physical Review C—Nuclear Physics 88 (5), 055802, 2013 | 45 | 2013 |
| Microscopic equation of state of hot nuclear matter for numerical relativity simulations D Logoteta, A Perego, I Bombaci Astronomy & Astrophysics 646, A55, 2021 | 43 | 2021 |
| Probing the incompressibility of nuclear matter at ultrahigh density through the prompt collapse of asymmetric neutron star binaries A Perego, D Logoteta, D Radice, S Bernuzzi, R Kashyap, A Das, ... Physical review letters 129 (3), 032701, 2022 | 40 | 2022 |
