The Astrophysical journal, ISSN 1538-4357, 2014, Volume 789, Issue 2, pp. 127 - 7

In recent years, there have been several successful attempts to constrain the equation of state of neutron star matter using input from low-energy nuclear...

neutron | dense matter - equation of state - stars | equation of state | EQUATION-OF-STATE | GROUND-STATE | dense matter | ASTRONOMY & ASTROPHYSICS | stars: neutron | Neutron stars | Equations of state | High density | Constrictions | Quarks | Nuclear physics | Constraining | Quantum chromodynamics | DENSITY | NEUTRONS | QUANTUM CHROMODYNAMICS | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | NEUTRON STARS | EQUATIONS OF STATE | QUARK MATTER

neutron | dense matter - equation of state - stars | equation of state | EQUATION-OF-STATE | GROUND-STATE | dense matter | ASTRONOMY & ASTROPHYSICS | stars: neutron | Neutron stars | Equations of state | High density | Constrictions | Quarks | Nuclear physics | Constraining | Quantum chromodynamics | DENSITY | NEUTRONS | QUANTUM CHROMODYNAMICS | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | NEUTRON STARS | EQUATIONS OF STATE | QUARK MATTER

Journal Article

The Astrophysical journal, ISSN 1538-4357, 2018, Volume 860, Issue 2, p. 139

The detection of GW170817 and its electromagnetic counterparts allows us to constrain the equation of state of dense matter in new and complementary ways. Very...

equation of state | gravitational waves | stars: neutron | MASSES | NEUTRON-STARS | MODEL | MERGER | QUARK STARS | EQUATION-OF-STATE | NUCLEAR-MATTER | ASTRONOMY & ASTROPHYSICS | FORCES | DENSE MATTER | Equations of state | Mathematical analysis | Gravitational waves | Stars | Quarks | Formability | Gravity waves

equation of state | gravitational waves | stars: neutron | MASSES | NEUTRON-STARS | MODEL | MERGER | QUARK STARS | EQUATION-OF-STATE | NUCLEAR-MATTER | ASTRONOMY & ASTROPHYSICS | FORCES | DENSE MATTER | Equations of state | Mathematical analysis | Gravitational waves | Stars | Quarks | Formability | Gravity waves

Journal Article

Astronomy and astrophysics (Berlin), ISSN 1432-0746, 2012, Volume 543, p. A157

Journal Article

The Astrophysical journal, ISSN 1538-4357, 2018, Volume 861, Issue 1, p. 10

We study gravitational waves (GWs) from a set of 2D multigroup neutrino radiation hydrodynamic simulations of core-collapse supernovae (CCSNe). Our goal is to...

equation of state | gravitational waves | hydrodynamics | supernovae: general | NEUTRINO-DRIVEN SUPERNOVA | STELLAR COLLAPSE | RADIATION | EXPLOSIONS | EQUATION-OF-STATE | ASTRONOMY & ASTROPHYSICS | PROGENITOR STARS | DYNAMICS | SIMULATIONS | Collapse | Neutron stars | Gravitation | Computer simulation | Supernovae | Gravitational waves | Feature recognition | Radiation | Quadrupoles | Equations of state | Perturbation methods | Spectrograms | Neutrinos | Gravitational collapse | Dependence | Stellar oscillations | Opacity | Gravity waves | Physics - High Energy Astrophysical Phenomena | ASTRONOMY AND ASTROPHYSICS

equation of state | gravitational waves | hydrodynamics | supernovae: general | NEUTRINO-DRIVEN SUPERNOVA | STELLAR COLLAPSE | RADIATION | EXPLOSIONS | EQUATION-OF-STATE | ASTRONOMY & ASTROPHYSICS | PROGENITOR STARS | DYNAMICS | SIMULATIONS | Collapse | Neutron stars | Gravitation | Computer simulation | Supernovae | Gravitational waves | Feature recognition | Radiation | Quadrupoles | Equations of state | Perturbation methods | Spectrograms | Neutrinos | Gravitational collapse | Dependence | Stellar oscillations | Opacity | Gravity waves | Physics - High Energy Astrophysical Phenomena | ASTRONOMY AND ASTROPHYSICS

Journal Article

Journal of alloys and compounds, ISSN 0925-8388, 2019, Volume 792, pp. 536 - 542

A nanostructured solid solution of SnSe1âˆ’xSx with xâ€¯=â€¯0.5 synthesized by mechanical alloying and its structural stability was studied by calorimetric...

Rietveld method | Density functional theory | Ab-initio | Birchâ€“Murnaghan equation of state | In-situ | X-ray diffractions | STRUCTURAL PHASE-TRANSITIONS | NANOCRYSTALLINE MATERIALS | PERFORMANCE | MATERIALS SCIENCE, MULTIDISCIPLINARY | METALLURGY & METALLURGICAL ENGINEERING | Birch-Murnaghan equation of state | CHEMISTRY, PHYSICAL | SNSE | EQUATION-OF-STATE | TIN | First principles | Densification | Equations of state | Solid solutions | Structural stability | Mathematical analysis | X-ray diffraction | Nanostructure | Mechanical alloying

Rietveld method | Density functional theory | Ab-initio | Birchâ€“Murnaghan equation of state | In-situ | X-ray diffractions | STRUCTURAL PHASE-TRANSITIONS | NANOCRYSTALLINE MATERIALS | PERFORMANCE | MATERIALS SCIENCE, MULTIDISCIPLINARY | METALLURGY & METALLURGICAL ENGINEERING | Birch-Murnaghan equation of state | CHEMISTRY, PHYSICAL | SNSE | EQUATION-OF-STATE | TIN | First principles | Densification | Equations of state | Solid solutions | Structural stability | Mathematical analysis | X-ray diffraction | Nanostructure | Mechanical alloying

Journal Article

Physical review letters, ISSN 1079-7114, 2018, Volume 120, Issue 17, p. 172702

The historical first detection of a binary neutron star merger by the LIGO-Virgo Collaboration [B. P. Abbott et al., Phys. Rev. Lett. 119, 161101 (2017)] is...

DENSITY | MATTER | EQUATION-OF-STATE | RADIUS | PHYSICS, MULTIDISCIPLINARY | MEAN-FIELD THEORY | MASS | CONSTRAINTS | NUCLEAR-EQUATION

DENSITY | MATTER | EQUATION-OF-STATE | RADIUS | PHYSICS, MULTIDISCIPLINARY | MEAN-FIELD THEORY | MASS | CONSTRAINTS | NUCLEAR-EQUATION

Journal Article

Reviews of modern physics, ISSN 1539-0756, 2012, Volume 84, Issue 4, pp. 1607 - 1653

Hydrogen and helium are the most abundant elements in the Universe. They are also, in principle, the most simple. Nonetheless, they display remarkable...

CAR-PARRINELLO EQUATIONS | QUANTUM MONTE-CARLO | EQUATION-OF-STATE | PHYSICS, MULTIDISCIPLINARY | DENSE IONIZED MATTER | AB-INITIO CALCULATIONS | X-RAY-DIFFRACTION | MOLECULAR-DYNAMICS SIMULATIONS | REFLECTED SHOCK EXPERIMENTS | PLASMA PHASE-TRANSITION | INSULATOR-METAL TRANSITION | Thermal properties | Monte Carlo method | Usage | Equations of state | Hydrogen | Optical properties | Analysis | Molecular dynamics | Quantum theory | Monte Carlo methods | Phase diagrams | Computational fluid dynamics | Computer simulation | Superconductivity | Density functional theory | Universe | Helium

CAR-PARRINELLO EQUATIONS | QUANTUM MONTE-CARLO | EQUATION-OF-STATE | PHYSICS, MULTIDISCIPLINARY | DENSE IONIZED MATTER | AB-INITIO CALCULATIONS | X-RAY-DIFFRACTION | MOLECULAR-DYNAMICS SIMULATIONS | REFLECTED SHOCK EXPERIMENTS | PLASMA PHASE-TRANSITION | INSULATOR-METAL TRANSITION | Thermal properties | Monte Carlo method | Usage | Equations of state | Hydrogen | Optical properties | Analysis | Molecular dynamics | Quantum theory | Monte Carlo methods | Phase diagrams | Computational fluid dynamics | Computer simulation | Superconductivity | Density functional theory | Universe | Helium

Journal Article

The Astrophysical journal, ISSN 1538-4357, 2016, Volume 831, Issue 2, p. 184

We present Chandra/ACIS-S subarray observations of the quiescent neutron star (NS) low-mass X-ray binaries X7 and X5 in the globular cluster 47 Tuc. The large...

equation of state | dense matter | stars: neutron | globular clusters: individual (47 Tucanae) | NGC 6304 | CEN X-4 | CHANDRA OBSERVATION | GLOBULAR-CLUSTER-47 TUCANAE | EQUATION-OF-STATE | ASTRONOMY & ASTROPHYSICS | CENTAURUS X-4 | THERMAL EMISSION | XMM-NEWTON OBSERVATIONS | SAX J1808.4-3658 | Neutron stars | X-ray bursts | Hydrogen | Atmospheric models | Neutrons | Star clusters | Laboratory experiments | X ray stars | Confidence intervals | Equations of state | Thermal emission | Stellar mass | X ray binaries | Binary stars | Atmosphere | Hydrogen ion concentration

equation of state | dense matter | stars: neutron | globular clusters: individual (47 Tucanae) | NGC 6304 | CEN X-4 | CHANDRA OBSERVATION | GLOBULAR-CLUSTER-47 TUCANAE | EQUATION-OF-STATE | ASTRONOMY & ASTROPHYSICS | CENTAURUS X-4 | THERMAL EMISSION | XMM-NEWTON OBSERVATIONS | SAX J1808.4-3658 | Neutron stars | X-ray bursts | Hydrogen | Atmospheric models | Neutrons | Star clusters | Laboratory experiments | X ray stars | Confidence intervals | Equations of state | Thermal emission | Stellar mass | X ray binaries | Binary stars | Atmosphere | Hydrogen ion concentration

Journal Article

Journal of computational physics, ISSN 0021-9991, 2014, Volume 268, pp. 326 - 354

We describe a novel interface-sharpening approach for efficient numerical resolution of a compressible homogeneous two-phase flow governed by a...

THINC reconstruction | Semi-discrete wave propagation method | Interface sharpening | Compressible two-phase flow | Five-equation model | Mieâ€“GrÃ¼neisen equation of state | Mie-GrÃ¼neisen equation of state | MULTICOMPONENT FLOW | IMPLEMENTATION | Mie-Gruneisen equation of state | MODEL | PHYSICS, MATHEMATICAL | GODUNOV METHOD | TRANSITION | SCHEME | COMPUTER SCIENCE, INTERDISCIPLINARY APPLICATIONS | CONSERVATION | Analysis | Wave propagation | Algorithms | Reconstruction | Algebra | Compressibility | Discretization | Mathematical analysis | Sharpening | Mathematical models

THINC reconstruction | Semi-discrete wave propagation method | Interface sharpening | Compressible two-phase flow | Five-equation model | Mieâ€“GrÃ¼neisen equation of state | Mie-GrÃ¼neisen equation of state | MULTICOMPONENT FLOW | IMPLEMENTATION | Mie-Gruneisen equation of state | MODEL | PHYSICS, MATHEMATICAL | GODUNOV METHOD | TRANSITION | SCHEME | COMPUTER SCIENCE, INTERDISCIPLINARY APPLICATIONS | CONSERVATION | Analysis | Wave propagation | Algorithms | Reconstruction | Algebra | Compressibility | Discretization | Mathematical analysis | Sharpening | Mathematical models

Journal Article

International journal of modern physics. D, Gravitation, astrophysics, cosmology, ISSN 1793-6594, 2019, Volume 28, Issue 13, p. 1941006

We provide a strange star model under the framework of general relativity by using a general linear equation of state (EOS). The solution set thus obtained is...

MATTER | General relativity | APPROACHING SCHWARZSCHILD LIMIT | NEUTRON-STAR | DYNAMICAL INSTABILITY | MAXIMUM MASS | EQUATION-OF-STATE | RELATIVISTIC MODEL | CONSERVATION | ASTRONOMY & ASTROPHYSICS | bag constant | homotopy perturbation method | REDSHIFT | strange stars | Physics - General Relativity and Quantum Cosmology

MATTER | General relativity | APPROACHING SCHWARZSCHILD LIMIT | NEUTRON-STAR | DYNAMICAL INSTABILITY | MAXIMUM MASS | EQUATION-OF-STATE | RELATIVISTIC MODEL | CONSERVATION | ASTRONOMY & ASTROPHYSICS | bag constant | homotopy perturbation method | REDSHIFT | strange stars | Physics - General Relativity and Quantum Cosmology

Journal Article

Monthly notices of the Royal Astronomical Society, ISSN 1365-2966, 2018, Volume 474, Issue 3, pp. 3557 - 3564

A binary neutron star merger produces a rapidly and differentially rotating compact remnant whose lifespan heavily affects the electromagnetic and...

Relativistic processes | Stars: neutron | Equation of state | Methods: numerical | Stars: rotation | relativistic processes | equation of state | EQUATION-OF-STATE | MODELS | STABILITY | ASTRONOMY & ASTROPHYSICS | NEUTRON-STARS | methods: numerical | stars: rotation | stars: neutron | MAXIMUM MASS | Differential rotation | Numerical simulations | Gravitation | Computer simulation | Equilibrium | Stellar models | Equations of state | Stability criteria | Binary stars | Gravitational collapse | Angular momentum | Dynamic stability | Astronomical models | Instability | Stellar rotation

Relativistic processes | Stars: neutron | Equation of state | Methods: numerical | Stars: rotation | relativistic processes | equation of state | EQUATION-OF-STATE | MODELS | STABILITY | ASTRONOMY & ASTROPHYSICS | NEUTRON-STARS | methods: numerical | stars: rotation | stars: neutron | MAXIMUM MASS | Differential rotation | Numerical simulations | Gravitation | Computer simulation | Equilibrium | Stellar models | Equations of state | Stability criteria | Binary stars | Gravitational collapse | Angular momentum | Dynamic stability | Astronomical models | Instability | Stellar rotation

Journal Article

The Astrophysical journal, ISSN 1538-4357, 2013, Volume 773, Issue 1, pp. 11 - 14

Microscopic calculations of neutron matter based on nuclear interactions derived from chiral effective field theory, combined with the recent observation of a...

dense matter | equation of state | stars: neutron | MATTER | RADIUS | ASTRONOMY & ASTROPHYSICS | MASS | FORCES | Neutron stars | Equations of state | Computer simulation | Mathematical analysis | Tables | Energy (nuclear) | Density | Nuclear physics | NEUTRONS | NEUTRON STARS | LIMITING VALUES | INTERACTIONS | COMPUTERIZED SIMULATION | DENSITY | FIELD THEORIES | NUCLEAR MATTER | NUCLEAR PHYSICS | SYMMETRY | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | ASTROPHYSICS | EQUATIONS OF STATE | CHIRALITY

dense matter | equation of state | stars: neutron | MATTER | RADIUS | ASTRONOMY & ASTROPHYSICS | MASS | FORCES | Neutron stars | Equations of state | Computer simulation | Mathematical analysis | Tables | Energy (nuclear) | Density | Nuclear physics | NEUTRONS | NEUTRON STARS | LIMITING VALUES | INTERACTIONS | COMPUTERIZED SIMULATION | DENSITY | FIELD THEORIES | NUCLEAR MATTER | NUCLEAR PHYSICS | SYMMETRY | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | ASTROPHYSICS | EQUATIONS OF STATE | CHIRALITY

Journal Article