Publication data of Logoteta, Domenico: Link to Inspire

Created with Highcharts 9.0.1CitationsCitationsw/o self-citaionself-citaion201020122014201620182020202220240500100015002000
Created with Highcharts 9.0.1Publicationspublications per yearPublicationsPublications per yearCumulative publications201020122014201620182020202220240153045607501.534.567.5
Created with Highcharts 9.0.1h-indexh-indexh-indexh-index w/o self-citaion20102012201420162018202020222024051015202530
Created with Highcharts 9.0.1CitationsBreakdown of Most Cited PapersrestNeutrino emission from binary neutron star mergers: characterizing light curves and mean energiesNeutrino emission from binary neutron star mergers: characterizing light cur…Quark deconfinement transition in neutron stars with the field correlator methodQuark deconfinement transition in neutron stars with the field correlator met…Effects of Chiral Effective Field Theory Equation of State on Binary Neutron Star MergersEffects of Chiral Effective Field Theory Equation of State on Binary Neutron St…Probing the Incompressibility of Nuclear Matter at Ultrahigh Density through the Prompt Collapse of Asymmetric Neutron Star BinariesProbing the Incompressibility of Nuclear Matter at Ultrahigh Density through …Microscopic equation of state of hot nuclear matter for numerical relativity simulationsMicroscopic equation of state of hot nuclear matter for numerical relativity si…Fast spinning strange stars: possible ways to constrain interacting quark matter parametersFast spinning strange stars: possible ways to constrain interacting quark mat…Correlations imposed by the unitary limit between few-nucleon systems, nuclear matter and neutron starsCorrelations imposed by the unitary limit between few-nucleon systems, nucl…Nuclear matter properties from local chiral interactions with $Delta$ isobar intermediate statesNuclear matter properties from local chiral interactions with $Delta$ isobar in…Numerical relativity simulations of prompt collapse mergers: Threshold mass and phenomenological constraints on neutron star properties after GW170817Numerical relativity simulations of prompt collapse mergers: Threshold mass …Benchmark calculations of pure neutron matter with realistic nucleon-nucleon interactionsBenchmark calculations of pure neutron matter with realistic nucleon-nucleo…Impact of chiral hyperonic three-body forces on neutron starsQuark matter nucleation in neutron stars and astrophysical implicationsQuark matter nucleation in hot hadronic matterSignatures of deconfined quark phases in binary neutron star mergersEquation of state of dense nuclear matter and neutron star structure from nuclear chiral interactionsEquation of state of dense nuclear matter and neutron star structure from n…Accretion-induced prompt black hole formation in asymmetric neutron star mergers, dynamical ejecta and kilonova signalsAccretion-induced prompt black hole formation in asymmetric neutron star …Was GW190814 a Black Hole–Strange Quark Star System?Estimation of the effect of hyperonic three-body forces on the maximum mass of neutron starsEstimation of the effect of hyperonic three-body forces on the maximum mas…Numerical Relativity Simulations of the Neutron Star Merger GW170817: Long-Term Remnant Evolutions, Winds, Remnant Disks, and NucleosynthesisNumerical Relativity Simulations of the Neutron Star Merger GW170817: Lon…201020122014201620182020202220240500100015002000
Created with Highcharts 9.0.1Fraction [%]Breakdown of Most Cited Papers (Fraction)Neutrino emission from binary neutron star mergers: characterizing light curves and mean energiesNeutrino emission from binary neutron star mergers: characterizing light cur…Quark deconfinement transition in neutron stars with the field correlator methodQuark deconfinement transition in neutron stars with the field correlator met…Effects of Chiral Effective Field Theory Equation of State on Binary Neutron Star MergersEffects of Chiral Effective Field Theory Equation of State on Binary Neutron St…Probing the Incompressibility of Nuclear Matter at Ultrahigh Density through the Prompt Collapse of Asymmetric Neutron Star BinariesProbing the Incompressibility of Nuclear Matter at Ultrahigh Density through …Microscopic equation of state of hot nuclear matter for numerical relativity simulationsMicroscopic equation of state of hot nuclear matter for numerical relativity si…Fast spinning strange stars: possible ways to constrain interacting quark matter parametersFast spinning strange stars: possible ways to constrain interacting quark mat…Correlations imposed by the unitary limit between few-nucleon systems, nuclear matter and neutron starsCorrelations imposed by the unitary limit between few-nucleon systems, nucl…Nuclear matter properties from local chiral interactions with $Delta$ isobar intermediate statesNuclear matter properties from local chiral interactions with $Delta$ isobar in…Numerical relativity simulations of prompt collapse mergers: Threshold mass and phenomenological constraints on neutron star properties after GW170817Numerical relativity simulations of prompt collapse mergers: Threshold mass …Benchmark calculations of pure neutron matter with realistic nucleon-nucleon interactionsBenchmark calculations of pure neutron matter with realistic nucleon-nucleo…Impact of chiral hyperonic three-body forces on neutron starsQuark matter nucleation in neutron stars and astrophysical implicationsQuark matter nucleation in hot hadronic matterSignatures of deconfined quark phases in binary neutron star mergersEquation of state of dense nuclear matter and neutron star structure from nuclear chiral interactionsEquation of state of dense nuclear matter and neutron star structure from n…Accretion-induced prompt black hole formation in asymmetric neutron star mergers, dynamical ejecta and kilonova signalsAccretion-induced prompt black hole formation in asymmetric neutron star …Was GW190814 a Black Hole–Strange Quark Star System?Estimation of the effect of hyperonic three-body forces on the maximum mass of neutron starsEstimation of the effect of hyperonic three-body forces on the maximum mas…Numerical Relativity Simulations of the Neutron Star Merger GW170817: Long-Term Remnant Evolutions, Winds, Remnant Disks, and NucleosynthesisNumerical Relativity Simulations of the Neutron Star Merger GW170817: Lon…201020122014201620182020202220240255075100
Created with Highcharts 9.0.1Citations/1 YearCitations/PeriodCitations / 1 YearMoving average201020122014201620182020202220240100200300400500