Showing 1–20 of 59 results
/ Date/ Name
Dec 23, 2019Empirical constraints on the high-density equation of state from multi-messenger observablesJun 1, 2012Description of light clusters in relativistic nuclear modelsJul 9, 2013Nuclear matter EOS with light clusters within the mean-field approximationJan 11, 2024From NS observations to nuclear matter properties: a machine learning approachMay 31, 2025Learning about neutron star composition from the slope of the mass-radius diagramAug 28, 2020Quark matter in light neutron starsDec 2, 2022Hybrid stars with large strange quark coresJun 7, 2021Crust-core transition of a neutron star: effect of the temperature under strong magnetic fieldsJun 13, 2014Strange quark chiral phase transition in hot 2+1-flavor magnetized quark matterJul 11, 2023Neutron star equation of state: identifying hadronic matter characteristicsDec 10, 2021Hybrid stars from a constrained equation of stateOct 12, 2020Effect of the crust on neutron star empirical relationsMay 13, 2021Hybrid stars with large strange quark cores constrained by GW170817Oct 1, 2021Constraints on high density equation of state from maximum neutron star massSep 19, 2024Detecting Hyperons in neutron stars -- a machine learning approachMay 21, 2020Neutron stars with large quark coresOct 12, 2019Unveiling the nuclear matter EoS from neutron star properties: a supervised machine learning approachSep 19, 2022Extracting nuclear matter properties from the neutron star matter equation of state using deep neural networksDec 10, 2021Determination of the symmetry energy from the neutron star equation of stateJun 12, 2023Decoding Neutron Star Observations: Revealing Composition through Bayesian Neural Networks