Search Results - "Bombaci, Ignazio"
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Impact of chiral hyperonic three-body forces on neutron stars
Published in The European physical journal. A, Hadrons and nuclei (01-11-2019)“… We study the effects of the nucleon-nucleon-lambda (NN Λ three-body force on neutron stars. In particular, we consider the NN Λ force recently derived by the…”
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Accretion-induced prompt black hole formation in asymmetric neutron star mergers, dynamical ejecta, and kilonova signals
Published in Monthly notices of the Royal Astronomical Society (01-09-2020)“…ABSTRACT We present new numerical relativity results of neutron star (NS) mergers with chirp mass 1.188 M⊙ and mass ratios q = 1.67 and q = 1.8 using…”
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Quark matter nucleation in neutron stars and astrophysical implications
Published in The European physical journal. A, Hadrons and nuclei (01-03-2016)“… A phase of strong interacting matter with deconfined quarks is expected in the core of massive neutron stars. We investigate the quark deconfinement phase…”
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Isoentropic equations of state of β-stable hadronic matter with a quark phase transition
Published in The European physical journal. A, Hadrons and nuclei (01-03-2022)“…We construct isoentropic equations of state (EOSs) of β -stable dense hadronic matter considering the possibility that a quark deconfinement phase transition…”
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Nuclear matter saturation with chiral three-nucleon interactions fitted to light nuclei properties
Published in Physics letters. B (10-07-2016)“…The energy per particle of symmetric nuclear matter and pure neutron matter is calculated using the many-body Brueckner–Hartree–Fock approach and employing the…”
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Two Coexisting Families of Compact Stars: Observational Implications for Millisecond Pulsars
Published in The Astrophysical journal (10-10-2017)“…It is usually thought that a single equation of state (EoS) model "correctly" represents cores of all compact stars. Here we emphasize that two families of…”
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Constraints on Microscopic and Phenomenological Equations of State of Dense Matter from GW170817
Published in Universe (Basel) (25-09-2019)“…We discuss the constraints on the equation of state (EOS) of neutron star matter obtained by the data analysis of the neutron star-neutron star merger in the…”
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Quark Deconfinement and Implications for the Radius and the Limiting Mass of Compact Stars
Published in The Astrophysical journal (10-10-2004)“…We study the consequences of the hadron-quark deconfinement phase transition in stellar compact objects when finitesize effects between the deconfined quark…”
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Fast spinning strange stars: possible ways to constrain interacting quark matter parameters
Published in Monthly notices of the Royal Astronomical Society (11-04-2016)Get full text
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Neutron stars: Cosmic laboratories for matter under extreme conditions
Published in EPJ Web of conferences (01-01-2016)“…The true nature and the internal constitution of the compact stars known as neutron stars (NSs) is one of the most fascinating enigma in modern astrophysics…”
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Conversion of Neutron Stars to Strange Stars as the Central Engine of Gamma-Ray Bursts
Published in The Astrophysical journal (20-02-2000)“…We study the conversion of a neutron star to a strange star as a possible energy source for gamma-ray bursts. We use different recent models for the equation…”
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Comparative study of three-nucleon force models in nuclear matter
Published in Physical review. C, Nuclear physics (15-06-2015)Get full text
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The Hyperon Puzzle in Neutron Stars
Published in Nuclear physics news (2021)Get full text
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14
A link between measured neutron star masses and lattice QCD data
Published in Monthly notices of the Royal Astronomical Society. Letters (21-07-2013)“…We study the hadron-quark phase transition in neutron star matter and the structural properties of hybrid stars using an equation of state (EOS) for the quark…”
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Fast spinning strange stars: possible ways to constrain interacting quark matter parameters
Published in Monthly notices of the Royal Astronomical Society (11-04-2016)“…For a set of equation of state (EoS) models involving interacting strange quark matter, characterized by an effective bag constant (B eff) and a perturbative…”
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Three-body force effect on nuclear symmetry energy and single-particle properties of asymmetric nuclear matter
Published in The European physical journal. A, Hadrons and nuclei (2014)“…We present an upgraded review of our microscopic investigation on the single-particle properties and the EOS of isospin asymmetric nuclear matter within the…”
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Millisecond radio pulsars with known masses: Parameter values and equation of state models
Published in New astronomy (01-07-2017)“…•The work characterizes a group of millisecond pulsars at an unprecedented level.•The work provides the first detailed catalogue of some compact star…”
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Dark matter admixed neutron stars with a realistic nuclear equation of state from chiral nuclear interactions
Published 29-05-2024“…We study the effects of dark matter on the structural properties of neutron stars. In particular we investigate how the presence of a dark matter component…”
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Strangeness in neutron stars
Published in Nuclear physics. A (30-05-2005)“…We discuss the role of strangeness on the internal constitution and structural properties of neutron stars. In particular, we report on recent calculations of…”
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Composition and structure of protoneutron stars
Published in Physics reports (01-02-1997)“…We investigate the structure of neutron stars shortly after they are born, when the entropy per baryon is of order 1 or 2 and neutrinos are trapped on…”
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