Physics Reports, ISSN 0370-1573, 03/2016, Volume 621, Issue C, pp. 127 - 164

Recent developments in the theory of pure neutron matter and experiments concerning the symmetry energy of nuclear matter, coupled with recent measurements of...

Neutron stars | Dense matter in equilibrium | Dense matter off-equilibrium | Equation of state of dense matter | Thermal effects | Heavy-ions | ELASTIC PROTON-SCATTERING | PHYSICS, MULTIDISCIPLINARY | MOMENTUM-DEPENDENT INTERACTIONS | BLACK-HOLE FORMATION | COLLECTIVE MOTION | MILLISECOND PULSAR | SYMMETRY ENERGY | HEAVY-ION COLLISIONS | MASS-RADIUS RELATION | CONSTRAINTS | NUCLEAR-EQUATION | Collisions (Nuclear physics) | Thermal properties

Neutron stars | Dense matter in equilibrium | Dense matter off-equilibrium | Equation of state of dense matter | Thermal effects | Heavy-ions | ELASTIC PROTON-SCATTERING | PHYSICS, MULTIDISCIPLINARY | MOMENTUM-DEPENDENT INTERACTIONS | BLACK-HOLE FORMATION | COLLECTIVE MOTION | MILLISECOND PULSAR | SYMMETRY ENERGY | HEAVY-ION COLLISIONS | MASS-RADIUS RELATION | CONSTRAINTS | NUCLEAR-EQUATION | Collisions (Nuclear physics) | Thermal properties

Journal Article

Nuclear Physics, Section A, ISSN 0375-9474, 08/2014, Volume 928, pp. 260 - 275

Gerry Brown has had the most influence on my career in Physics, and my life after graduate studies. This article gives a brief account of some of the many ways...

Observations | Neutron stars | Theoretical insights | ROTATION | PHYSICS, NUCLEAR | BLACK-HOLES | CRUST | EQUATION-OF-STATE | RADIUS | MASS | CHANDRA | CASSIOPEIA | DENSE MATTER | Physics - Solar and Stellar Astrophysics

Observations | Neutron stars | Theoretical insights | ROTATION | PHYSICS, NUCLEAR | BLACK-HOLES | CRUST | EQUATION-OF-STATE | RADIUS | MASS | CHANDRA | CASSIOPEIA | DENSE MATTER | Physics - Solar and Stellar Astrophysics

Journal Article

Physics Reports, ISSN 0370-1573, 2007, Volume 442, Issue 1, pp. 109 - 165

We investigate how current and proposed observations of neutron stars can lead to an understanding of the state of their interiors and the key unknowns: the...

Neutron stars | Observations | Structure | Equation of state of dense matter | SOFT GAMMA-REPEATERS | neutron stars | THOMAS-FERMI CALCULATIONS | GENERAL-RELATIVITY | PHYSICS, MULTIDISCIPLINARY | structure | STRONG MAGNETIC-FIELDS | X-RAY OSCILLATIONS | KAON CONDENSATION | NUCLEAR-MATTER | equation of state of dense matter | WEAK INTERACTION | observations | HEAVY-ION COLLISIONS | FINITE-TEMPERATURE

Neutron stars | Observations | Structure | Equation of state of dense matter | SOFT GAMMA-REPEATERS | neutron stars | THOMAS-FERMI CALCULATIONS | GENERAL-RELATIVITY | PHYSICS, MULTIDISCIPLINARY | structure | STRONG MAGNETIC-FIELDS | X-RAY OSCILLATIONS | KAON CONDENSATION | NUCLEAR-MATTER | equation of state of dense matter | WEAK INTERACTION | observations | HEAVY-ION COLLISIONS | FINITE-TEMPERATURE

Journal Article

1997, Physics reports, Volume 280, no. 1., viii, 78

Book

Physical Review Letters, ISSN 0031-9007, 03/2005, Volume 94, Issue 11

Journal Article

Pramana, ISSN 0304-4289, 5/2015, Volume 84, Issue 5, pp. 927 - 941

Neutron stars have long been regarded as extraterrestrial laboratories from which we can learn about extreme energy density matter at low temperatures. In this...

Neutron stars | Astrophysics and Astroparticles | theoretical insights | observations | Physics, general | Physics | Astronomy, Observations and Techniques | Observations | Theoretical insights | EQUATION-OF-STATE | RADIUS | PHYSICS, MULTIDISCIPLINARY | MASS | PULSAR | DISCOVERY | Specific gravity

Neutron stars | Astrophysics and Astroparticles | theoretical insights | observations | Physics, general | Physics | Astronomy, Observations and Techniques | Observations | Theoretical insights | EQUATION-OF-STATE | RADIUS | PHYSICS, MULTIDISCIPLINARY | MASS | PULSAR | DISCOVERY | Specific gravity

Journal Article

Physical Review Letters, ISSN 0031-9007, 02/2011, Volume 106, Issue 8, p. 081101

We propose that the observed cooling of the neutron star in Cassiopeia A is due to enhanced neutrino emission from the recent onset of the breaking and...

PHYSICS, MULTIDISCIPLINARY | EMISSION | A SUPERNOVA REMNANT

PHYSICS, MULTIDISCIPLINARY | EMISSION | A SUPERNOVA REMNANT

Journal Article

Physical Review C - Nuclear Physics, ISSN 0556-2813, 05/2012, Volume 85, Issue 5

The interpretation of the measured elliptic and higher order collective flows in heavy-ion collisions in terms of viscous hydrodynamics depends sensitively on...

TRANSPORT-COEFFICIENTS | KINETIC GAS THEORY | ELLIPTIC FLOW | SPS | QUARK-GLUON PLASMA | PHYSICS, NUCLEAR | NUCLEUS-NUCLEUS COLLISIONS

TRANSPORT-COEFFICIENTS | KINETIC GAS THEORY | ELLIPTIC FLOW | SPS | QUARK-GLUON PLASMA | PHYSICS, NUCLEAR | NUCLEUS-NUCLEUS COLLISIONS

Journal Article

Annals of Physics, ISSN 0003-4916, 12/2015, Volume 363, Issue C, pp. 533 - 555

Analytical formulas for next-to-leading order temperature corrections to the thermal state variables of interacting nucleons in bulk matter are derived in the...

Potential and field-theoretical models | Hot and dense matter | Thermal effects | PHYSICS, MULTIDISCIPLINARY | FERMI LIQUIDS | STATE | NUCLEAR-EQUATION | LANDAU-THEORY | Thermodynamics | Analysis | Nuclear physics | Astronomy

Potential and field-theoretical models | Hot and dense matter | Thermal effects | PHYSICS, MULTIDISCIPLINARY | FERMI LIQUIDS | STATE | NUCLEAR-EQUATION | LANDAU-THEORY | Thermodynamics | Analysis | Nuclear physics | Astronomy

Journal Article

International Journal of Modern Physics E, ISSN 0218-3013, 2017, Volume 26, Issue 1-2, p. 1740005

The formalism of next-to-leading order (NLO) Fermi Liquid Theory (FLT) is employed to calculate the thermal properties of symmetric nuclear and pure neutron...

Thermal effects in dense matter | next-to-leading order Fermi liquid theory | field-theoretical models | STARS | STATE | PHYSICS, NUCLEAR | EQUATION | PHYSICS, PARTICLES & FIELDS | Physics - Nuclear Theory | Physics

Thermal effects in dense matter | next-to-leading order Fermi liquid theory | field-theoretical models | STARS | STATE | PHYSICS, NUCLEAR | EQUATION | PHYSICS, PARTICLES & FIELDS | Physics - Nuclear Theory | Physics

Journal Article

The Astrophysical Journal, ISSN 0004-637X, 12/2009, Volume 707, Issue 2, pp. 1131 - 1140

The minimal cooling paradigm for neutron star cooling assumes that enhanced cooling due to neutrino emission from any direct Urca process, due either to...

Dense matter | Stars: neutron | Neutrinos | Equation of state | MATTER | equation of state | neutrinos | QUASI-PARTICLE INTERACTIONS | PULSAR | STATE | stars: neutron | YOUNG | dense matter | SUPERNOVA-REMNANTS | ASTRONOMY & ASTROPHYSICS | X-RAY-EMISSION | DIRECT URCA PROCESS | XMM-NEWTON | KS-1731-260 | SUPERNOVA REMNANTS | THERMODYNAMIC PROPERTIES | NEUTRON STARS | EQUATIONS | FERMIONS | LEPTONS | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | PHYSICAL PROPERTIES | TRANSITION TEMPERATURE | ALGEBRAIC CURRENTS | EQUATIONS OF STATE | HYPERONS | STRANGE PARTICLES | PULSARS | NEUTRONS | CRITICAL TEMPERATURE | CURRENTS | ELEMENTARY PARTICLES | NUCLEONS | COSMIC RADIO SOURCES | MASSLESS PARTICLES | QUARKS | STARS | COOPER PAIRS | EMISSION | NEUTRINOS | VECTOR CURRENTS | BARYONS | HADRONS

Dense matter | Stars: neutron | Neutrinos | Equation of state | MATTER | equation of state | neutrinos | QUASI-PARTICLE INTERACTIONS | PULSAR | STATE | stars: neutron | YOUNG | dense matter | SUPERNOVA-REMNANTS | ASTRONOMY & ASTROPHYSICS | X-RAY-EMISSION | DIRECT URCA PROCESS | XMM-NEWTON | KS-1731-260 | SUPERNOVA REMNANTS | THERMODYNAMIC PROPERTIES | NEUTRON STARS | EQUATIONS | FERMIONS | LEPTONS | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | PHYSICAL PROPERTIES | TRANSITION TEMPERATURE | ALGEBRAIC CURRENTS | EQUATIONS OF STATE | HYPERONS | STRANGE PARTICLES | PULSARS | NEUTRONS | CRITICAL TEMPERATURE | CURRENTS | ELEMENTARY PARTICLES | NUCLEONS | COSMIC RADIO SOURCES | MASSLESS PARTICLES | QUARKS | STARS | COOPER PAIRS | EMISSION | NEUTRINOS | VECTOR CURRENTS | BARYONS | HADRONS

Journal Article

Physics Reports, ISSN 0370-1573, 2005, Volume 411, Issue 6, pp. 325 - 375

The roles of isospin asymmetry in nuclei and neutron stars are investigated using a range of potential and field-theoretical models of nucleonic matter. The...

Isospin asymmetry | Nuclei | Neutron stars | nuclei | neutron stars | PHYSICS, MULTIDISCIPLINARY | SPIN-ISOSPIN | PB-208 | FINITE NUCLEI | SURFACE SYMMETRY ENERGY | EQUATION-OF-STATE | isospin asymmetry | MEAN-FIELD THEORY | ELECTRON-SCATTERING | RADII | HEAVY-ION COLLISIONS | DENSE MATTER | Analysis | Astronomy

Isospin asymmetry | Nuclei | Neutron stars | nuclei | neutron stars | PHYSICS, MULTIDISCIPLINARY | SPIN-ISOSPIN | PB-208 | FINITE NUCLEI | SURFACE SYMMETRY ENERGY | EQUATION-OF-STATE | isospin asymmetry | MEAN-FIELD THEORY | ELECTRON-SCATTERING | RADII | HEAVY-ION COLLISIONS | DENSE MATTER | Analysis | Astronomy

Journal Article

Physical Review C - Nuclear Physics, ISSN 0556-2813, 08/2015, Volume 92, Issue 2

We explore the thermal properties of hot and dense matter using a model that reproduces the empirical properties of isospin symmetric and asymmetric bulk...

BLACK-HOLE FORMATION | EQUATION-OF-STATE | EFFECTIVE-MASS | NUCLEAR-MATTER | MOMENTUM-DEPENDENCE | SYMMETRY ENERGY | HEAVY-ION COLLISIONS | NEUTRON-STARS | PHYSICS, NUCLEAR | SUPERNOVA | DIFFERENTIAL ROTATION

BLACK-HOLE FORMATION | EQUATION-OF-STATE | EFFECTIVE-MASS | NUCLEAR-MATTER | MOMENTUM-DEPENDENCE | SYMMETRY ENERGY | HEAVY-ION COLLISIONS | NEUTRON-STARS | PHYSICS, NUCLEAR | SUPERNOVA | DIFFERENTIAL ROTATION

Journal Article

The Astrophysical Journal Supplement Series, ISSN 0067-0049, 12/2004, Volume 155, Issue 2, pp. 623 - 650

A new classification of neutron star cooling scenarios, involving either "minimal'' cooling or "enhanced'' cooling, is proposed. The minimal cooling scenario...

Dense matter | Stars: neutron | Neutrinos | Equation of state | equation of state | THERMAL EVOLUTION | neutrinos | PROTON SUPERFLUIDITY | stars : neutron | QUASI-PARTICLE INTERACTIONS | SUPERNOVA REMNANT | SURFACE-TEMPERATURE | EQUATION-OF-STATE | dense matter | S-1 NEUTRON | ASTRONOMY & ASTROPHYSICS | VS. OBSERVATIONS | X-RAY-SPECTRUM | URCA PROCESS

Dense matter | Stars: neutron | Neutrinos | Equation of state | equation of state | THERMAL EVOLUTION | neutrinos | PROTON SUPERFLUIDITY | stars : neutron | QUASI-PARTICLE INTERACTIONS | SUPERNOVA REMNANT | SURFACE-TEMPERATURE | EQUATION-OF-STATE | dense matter | S-1 NEUTRON | ASTRONOMY & ASTROPHYSICS | VS. OBSERVATIONS | X-RAY-SPECTRUM | URCA PROCESS

Journal Article

Physical Review C - Nuclear Physics, ISSN 0556-2813, 06/2014, Volume 89, Issue 6

We investigate the thermal properties of the potential model equation of state of Akmal, Pandharipande, and Ravenhall. This equation of state approximates the...

BLACK-HOLE FORMATION | INCOMPRESSIBILITY | EQUATION-OF-STATE | COLLAPSE | APPROXIMATION | ASYMMETRIC NUCLEAR-MATTER | MOMENTUM-DEPENDENCE | NEUTRON-STAR | MASS | PHYSICS, NUCLEAR | SKYRME FORCE

BLACK-HOLE FORMATION | INCOMPRESSIBILITY | EQUATION-OF-STATE | COLLAPSE | APPROXIMATION | ASYMMETRIC NUCLEAR-MATTER | MOMENTUM-DEPENDENCE | NEUTRON-STAR | MASS | PHYSICS, NUCLEAR | SKYRME FORCE

Journal Article

Annals of Physics, ISSN 0003-4916, 12/2015, Volume 363, Issue Complete

Analytical formulas for next-to-leading order temperature corrections to the thermal state variables of interacting nucleons in bulk matter are derived in the...

CORRECTIONS | NEUTRONS | FINITE-RANGE INTERACTIONS | NEUTRON STARS | CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS | MANY-BODY PROBLEM | CORRELATIONS | POTENTIALS | COMPARATIVE EVALUATIONS | SUPERNOVAE | RELATIVISTIC RANGE | NUCLEAR MATTER | NUCLEAR PHYSICS AND RADIATION PHYSICS | THERMODYNAMICS | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | TEMPERATURE DEPENDENCE | MEAN-FIELD THEORY | ASTROPHYSICS | EFFECTIVE MASS

CORRECTIONS | NEUTRONS | FINITE-RANGE INTERACTIONS | NEUTRON STARS | CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS | MANY-BODY PROBLEM | CORRELATIONS | POTENTIALS | COMPARATIVE EVALUATIONS | SUPERNOVAE | RELATIVISTIC RANGE | NUCLEAR MATTER | NUCLEAR PHYSICS AND RADIATION PHYSICS | THERMODYNAMICS | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | TEMPERATURE DEPENDENCE | MEAN-FIELD THEORY | ASTROPHYSICS | EFFECTIVE MASS

Journal Article