1957

Book

The European Physical Journal A, ISSN 1434-6001, 8/2019, Volume 55, Issue 8, pp. 1 - 8

Using recent gravitational and electromagnetic constraints on the neutron star matter equation of state (EOS) coming from the merge of two neutron stars, we...

Nuclear Physics, Heavy Ions, Hadrons | Nuclear Fusion | Physics | Particle and Nuclear Physics | MATTER | COUNTERPART | MASS | LIGHT | DECONFINEMENT | PHYSICS, NUCLEAR | MODEL | PHYSICS, PARTICLES & FIELDS | Quarks

Nuclear Physics, Heavy Ions, Hadrons | Nuclear Fusion | Physics | Particle and Nuclear Physics | MATTER | COUNTERPART | MASS | LIGHT | DECONFINEMENT | PHYSICS, NUCLEAR | MODEL | PHYSICS, PARTICLES & FIELDS | Quarks

Journal Article

The European Physical Journal A, ISSN 1434-6001, 6/2018, Volume 54, Issue 6, pp. 1 - 10

We employ modern two- and three-nucleon interactions derived in chiral perturbation theory (ChPT) at next to-next-to leading order (N2LO), to calculate the...

Nuclear Physics, Heavy Ions, Hadrons | Nuclear Fusion | Physics | Particle and Nuclear Physics | INCOMPRESSIBILITY | EQUATION-OF-STATE | NEUTRON MATTER | FIELD | 3-BODY FORCES | CONVERGENCE | PHYSICS, NUCLEAR | COLD | HOT | BRUECKNER-GOLDSTONE EXPANSION | SATURATION | PHYSICS, PARTICLES & FIELDS | Analysis | Information management

Nuclear Physics, Heavy Ions, Hadrons | Nuclear Fusion | Physics | Particle and Nuclear Physics | INCOMPRESSIBILITY | EQUATION-OF-STATE | NEUTRON MATTER | FIELD | 3-BODY FORCES | CONVERGENCE | PHYSICS, NUCLEAR | COLD | HOT | BRUECKNER-GOLDSTONE EXPANSION | SATURATION | PHYSICS, PARTICLES & FIELDS | Analysis | Information management

Journal Article

Astronomy and Astrophysics, ISSN 0004-6361, 2018, Volume 609, p. A128

Aims. We report a new microscopic equation of state (EOS) of dense symmetric nuclear matter, pure neutron matter, and asymmetric and beta-stable nuclear matter...

Dense matter | Stars: neutron | Equation of state | equation of state | MASSES | FIELD | 3-BODY FORCES | SUPERNOVA | MODEL | stars: neutron | BRUECKNER-GOLDSTONE EXPANSION | dense matter | ASTRONOMY & ASTROPHYSICS | COLD | TO-LEADING ORDER | SATURATION | SYMMETRY-BREAKING | Perturbation theory | Neutron stars | Chiral dynamics | Computer simulation | Empirical equations | Saturation | Relativity | Neutrons | Nuclei (nuclear physics) | Rotation | Equations of state | Binary stars | Heavy nuclei | Stellar rotation | Mathematical models | Nuclear matter | Nuclear interactions | Symmetry

Dense matter | Stars: neutron | Equation of state | equation of state | MASSES | FIELD | 3-BODY FORCES | SUPERNOVA | MODEL | stars: neutron | BRUECKNER-GOLDSTONE EXPANSION | dense matter | ASTRONOMY & ASTROPHYSICS | COLD | TO-LEADING ORDER | SATURATION | SYMMETRY-BREAKING | Perturbation theory | Neutron stars | Chiral dynamics | Computer simulation | Empirical equations | Saturation | Relativity | Neutrons | Nuclei (nuclear physics) | Rotation | Equations of state | Binary stars | Heavy nuclei | Stellar rotation | Mathematical models | Nuclear matter | Nuclear interactions | Symmetry

Journal Article

Physics Letters B, ISSN 0370-2693, 07/2016, Volume 758, Issue C, pp. 449 - 454

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...

Three-body force | Chiral nuclear interactions | Nuclear matter | SYMMETRY ENERGY | ASTRONOMY & ASTROPHYSICS | PHYSICS, NUCLEAR | BRUECKNER-GOLDSTONE EXPANSION | PHYSICS, PARTICLES & FIELDS | Nuclear and High Energy Physics | Nuclear Experiment | Nuclear Theory | Chiral nuclear interactions; Nuclear matter; Three-body force; Nuclear and High Energy Physics | Physics

Three-body force | Chiral nuclear interactions | Nuclear matter | SYMMETRY ENERGY | ASTRONOMY & ASTROPHYSICS | PHYSICS, NUCLEAR | BRUECKNER-GOLDSTONE EXPANSION | PHYSICS, PARTICLES & FIELDS | Nuclear and High Energy Physics | Nuclear Experiment | Nuclear Theory | Chiral nuclear interactions; Nuclear matter; Three-body force; Nuclear and High Energy Physics | Physics

Journal Article

The European Physical Journal A, ISSN 1434-6001, 11/2019, Volume 55, Issue 11, pp. 1 - 7

We study the effects of the nucleon-nucleon-lambda (NN $ \Lambda$ Λ three-body force on neutron stars. In particular, we consider the NN $ \Lambda$ Λ force...

Nuclear Physics, Heavy Ions, Hadrons | Nuclear Fusion | Physics | Particle and Nuclear Physics | BARYON-BARYON INTERACTION | PHYSICS, NUCLEAR | TO-LEADING ORDER | BINDING | EXTRA REPULSION | LAMBDA | PHYSICS, PARTICLES & FIELDS

Nuclear Physics, Heavy Ions, Hadrons | Nuclear Fusion | Physics | Particle and Nuclear Physics | BARYON-BARYON INTERACTION | PHYSICS, NUCLEAR | TO-LEADING ORDER | BINDING | EXTRA REPULSION | LAMBDA | PHYSICS, PARTICLES & FIELDS

Journal Article

International Journal of Modern Physics D, ISSN 0218-2718, 02/2017, Volume 26, Issue 2, p. 1730004

We investigate the quark deconfinement phase transition in cold ( T = 0 ) and hot β -stable hadronic matter. Assuming a first-order phase transition, we...

Neutron stars | quark deconfinement | equations of state of neutron-star matter | MASSES | SUPERCONDUCTIVITY | CONVERSION | STRANGE STARS | MODEL | GAMMA-RAY BURSTS | VELOCITY DISTRIBUTION | MATTER NUCLEATION | TEMPERATURE | ASTRONOMY & ASTROPHYSICS | PHASE-TRANSITION | Quarks

Neutron stars | quark deconfinement | equations of state of neutron-star matter | MASSES | SUPERCONDUCTIVITY | CONVERSION | STRANGE STARS | MODEL | GAMMA-RAY BURSTS | VELOCITY DISTRIBUTION | MATTER NUCLEATION | TEMPERATURE | ASTRONOMY & ASTROPHYSICS | PHASE-TRANSITION | Quarks

Journal Article

Journal of Physics: Conference Series, ISSN 1742-6588, 2014, Volume 527, Issue 1, pp. 12021 - 8

We study the quark deconfinement phase transition in cold (T = 0) neutron star matter and we calculate various structural properties of hybrid stars. For the...

Nucleonics | Neutron stars | Transition temperature | Correlation | Mathematical models | Quarks | Density | Baryons

Nucleonics | Neutron stars | Transition temperature | Correlation | Mathematical models | Quarks | Density | Baryons

Conference Proceeding

9.
Full Text
Nuclear matter properties from local chiral interactions with Δ isobar intermediate states

Physical Review C, ISSN 2469-9985, 12/2016, Volume 94, Issue 6

Using two-nucleon and three-nucleon interactions derived in the framework of chiral perturbation theory (ChPT) with and without the explicit Delta isobar...

EFFECTIVE-FIELD THEORY | EQUATION-OF-STATE | SYMMETRY ENERGY | 3-BODY FORCES | LAGRANGIANS | PHYSICS, NUCLEAR | NEUTRON-STAR STRUCTURE | POTENTIALS | TO-LEADING ORDER | BRUECKNER-GOLDSTONE EXPANSION | FINITE-TEMPERATURE | Physics - Nuclear Theory

EFFECTIVE-FIELD THEORY | EQUATION-OF-STATE | SYMMETRY ENERGY | 3-BODY FORCES | LAGRANGIANS | PHYSICS, NUCLEAR | NEUTRON-STAR STRUCTURE | POTENTIALS | TO-LEADING ORDER | BRUECKNER-GOLDSTONE EXPANSION | FINITE-TEMPERATURE | Physics - Nuclear Theory

Journal Article

Physical Review D - Particles, Fields, Gravitation and Cosmology, ISSN 1550-7998, 09/2013, Volume 88, Issue 6

A phase of strong interacting matter with deconfined quarks is expected in the core of massive neutron stars. In this article, we perform a study of the...

JONA-LASINIO MODEL | EQUATION-OF-STATE | QCD | NUCLEAR-MATTER | COLLAPSE | STRENGTH CORRELATORS | ASTRONOMY & ASTROPHYSICS | 1ST-ORDER PHASE-TRANSITIONS | 3-BODY FORCES | PULSAR | CHARGE | PHYSICS, PARTICLES & FIELDS

JONA-LASINIO MODEL | EQUATION-OF-STATE | QCD | NUCLEAR-MATTER | COLLAPSE | STRENGTH CORRELATORS | ASTRONOMY & ASTROPHYSICS | 1ST-ORDER PHASE-TRANSITIONS | 3-BODY FORCES | PULSAR | CHARGE | PHYSICS, PARTICLES & FIELDS

Journal Article

Journal of Physics: Conference Series, ISSN 1742-6588, 03/2018, Volume 981, Issue 1, p. 12009

Conference Proceeding

Monthly Notices of the Royal Astronomical Society: Letters, ISSN 1745-3925, 2013, Volume 433, Issue 1, pp. L79 - L83

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...

Dense matter | Stars: Neutron | Equation of state | MATTER | equation of state | RESONANCE PHYSICS | CHIRAL-SYMMETRY RESTORATION | QUARK-GLUON PLASMA | NONZERO BARYON DENSITY | stars: neutron | FIELD-STRENGTH CORRELATORS | EQUATION-OF-STATE | dense matter | ASTRONOMY & ASTROPHYSICS | PHASE-TRANSITION | POLYAKOV LOOP | FINITE-TEMPERATURE

Dense matter | Stars: Neutron | Equation of state | MATTER | equation of state | RESONANCE PHYSICS | CHIRAL-SYMMETRY RESTORATION | QUARK-GLUON PLASMA | NONZERO BARYON DENSITY | stars: neutron | FIELD-STRENGTH CORRELATORS | EQUATION-OF-STATE | dense matter | ASTRONOMY & ASTROPHYSICS | PHASE-TRANSITION | POLYAKOV LOOP | FINITE-TEMPERATURE

Journal Article

Journal of Physics: Conference Series, ISSN 1742-6588, 06/2017, Volume 861, Issue 1, p. 12013

Conference Proceeding

PHYSICAL REVIEW C, ISSN 2469-9985, 10/2019, Volume 100, Issue 4

I calculate the energy per particle of symmetric nuclear matter and pure neutron matter in the framework of the microscopic Brueckner-Hartree-Fock approach...

FIELD | 3-BODY FORCES | STATE | PHYSICS, NUCLEAR | COLD | EQUATION | BRUECKNER-GOLDSTONE EXPANSION | SATURATION

FIELD | 3-BODY FORCES | STATE | PHYSICS, NUCLEAR | COLD | EQUATION | BRUECKNER-GOLDSTONE EXPANSION | SATURATION

Journal Article

Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 04/2016, Volume 457, Issue 3, pp. 3101 - 3101

For a set of equation of state (EoS) models involving interacting strange quark matter, characterized by an effective bag constant (B sub( eff)) and a...

Symbols | Evolutionary | Stars | Constants | Mathematical models | Quarks | Signatures | Spinning

Symbols | Evolutionary | Stars | Constants | Mathematical models | Quarks | Signatures | Spinning

Journal Article

Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 04/2016, Volume 457, Issue 3, pp. 3101 - 3114

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...

Numerical - stars | Neutron - pulsars | PSR J1614-2230 - pulsars | Equation of state -methods | Individual | PSR J1748-2446ad - stars | Rotation | SPECTROSCOPIC MEASUREMENTS | equation of state | ROTATING NEUTRON-STARS | NONZERO BARYON DENSITY | methods: numerical | COMPACT STARS | GAMMA-RAY BURSTS | GENERAL-RELATIVISTIC SPECTRA | stars: neutron | EQUATION-OF-STATE | ACCRETION DISCS | SYSTEMATIC UNCERTAINTIES | ASTRONOMY & ASTROPHYSICS | PHASE-TRANSITION | pulsars: individual: PSR J1614-2230 pulsars: individual: PSR J1748-2446ad | stars: rotation

Numerical - stars | Neutron - pulsars | PSR J1614-2230 - pulsars | Equation of state -methods | Individual | PSR J1748-2446ad - stars | Rotation | SPECTROSCOPIC MEASUREMENTS | equation of state | ROTATING NEUTRON-STARS | NONZERO BARYON DENSITY | methods: numerical | COMPACT STARS | GAMMA-RAY BURSTS | GENERAL-RELATIVISTIC SPECTRA | stars: neutron | EQUATION-OF-STATE | ACCRETION DISCS | SYSTEMATIC UNCERTAINTIES | ASTRONOMY & ASTROPHYSICS | PHASE-TRANSITION | pulsars: individual: PSR J1614-2230 pulsars: individual: PSR J1748-2446ad | stars: rotation

Journal Article

EPL (Europhysics Letters), ISSN 0295-5075, 04/2011, Volume 94, Issue 1, p. 11002

A model based on a microscopic Brueckner-Hartree-Fock approach of hyperonic matter supplemented with additional simple phenomenological density-dependent...

MATTER | EQUATION-OF-STATE | PHYSICS, MULTIDISCIPLINARY | PULSAR | LAMBDA-NUCLEON INTERACTION | BINDING | BRUECKNER-GOLDSTONE EXPANSION | LIGHT HYPERNUCLEI | EXTRA REPULSION | Physics - Nuclear Theory

MATTER | EQUATION-OF-STATE | PHYSICS, MULTIDISCIPLINARY | PULSAR | LAMBDA-NUCLEON INTERACTION | BINDING | BRUECKNER-GOLDSTONE EXPANSION | LIGHT HYPERNUCLEI | EXTRA REPULSION | Physics - Nuclear Theory

Journal Article

Physical Review C - Nuclear Physics, ISSN 0556-2813, 06/2015, Volume 91, Issue 6

We calculate the energy per particle of symmetric nuclear matter and pure neutron matter using the microscopic many-body Brueckner-Hartree-Fock (BHF) approach...

EQUATION-OF-STATE | NEUTRON MATTER | SYMMETRY ENERGY | FIELD | PHYSICS, NUCLEAR | BRUECKNER-GOLDSTONE EXPANSION | 3-BODY FORCE | FINITE-TEMPERATURE | H-3

EQUATION-OF-STATE | NEUTRON MATTER | SYMMETRY ENERGY | FIELD | PHYSICS, NUCLEAR | BRUECKNER-GOLDSTONE EXPANSION | 3-BODY FORCE | FINITE-TEMPERATURE | H-3

Journal Article

Physical Review C - Nuclear Physics, ISSN 0556-2813, 11/2013, Volume 88, Issue 5

We study the consequences of quark matter nucleation in cold hadronic matter employing three relativistic-mean-field models to describe the hadronic phase and...

TRANSITION | EQUATION-OF-STATE | STRONG MAGNETIC-FIELD | STRANGE MATTER | NEUTRON-STARS | DECONFINEMENT | COLOR-DIELECTRIC MODEL | PHYSICS, NUCLEAR | GAMMA-RAY BURSTS | QUARK MATTER NUCLEATION | DENSE MATTER

TRANSITION | EQUATION-OF-STATE | STRONG MAGNETIC-FIELD | STRANGE MATTER | NEUTRON-STARS | DECONFINEMENT | COLOR-DIELECTRIC MODEL | PHYSICS, NUCLEAR | GAMMA-RAY BURSTS | QUARK MATTER NUCLEATION | DENSE MATTER

Journal Article