The European Physical Journal C, ISSN 1434-6044, 6/2017, Volume 77, Issue 6, pp. 1 - 9

We report the result of a search for sterile neutrinos with the latest cosmological observations. Both cases of massless and massive sterile neutrinos are...

Nuclear Physics, Heavy Ions, Hadrons | Measurement Science and Instrumentation | Nuclear Energy | Quantum Field Theories, String Theory | Physics | Elementary Particles, Quantum Field Theory | Astronomy, Astrophysics and Cosmology | PLANCK | MATTER | DARK ENERGY | BARYON ACOUSTIC-OSCILLATIONS | CONSTRAINTS | CONSTANT | MASSIVE NEUTRINOS | UNIVERSE | LOCAL VALUE | PROBES | PHYSICS, PARTICLES & FIELDS | General Relativity and Quantum Cosmology | Phenomenology | High Energy Physics - Phenomenology | High Energy Physics | Astrophysics | Cosmology and Extragalactic Astrophysics | Experiment | Nuclear and particle physics. Atomic energy. Radioactivity | Astrophysics - Cosmology and Nongalactic Astrophysics | High Energy Astrophysical Phenomena

Nuclear Physics, Heavy Ions, Hadrons | Measurement Science and Instrumentation | Nuclear Energy | Quantum Field Theories, String Theory | Physics | Elementary Particles, Quantum Field Theory | Astronomy, Astrophysics and Cosmology | PLANCK | MATTER | DARK ENERGY | BARYON ACOUSTIC-OSCILLATIONS | CONSTRAINTS | CONSTANT | MASSIVE NEUTRINOS | UNIVERSE | LOCAL VALUE | PROBES | PHYSICS, PARTICLES & FIELDS | General Relativity and Quantum Cosmology | Phenomenology | High Energy Physics - Phenomenology | High Energy Physics | Astrophysics | Cosmology and Extragalactic Astrophysics | Experiment | Nuclear and particle physics. Atomic energy. Radioactivity | Astrophysics - Cosmology and Nongalactic Astrophysics | High Energy Astrophysical Phenomena

Journal Article

Journal of High Energy Physics, ISSN 1126-6708, 8/2010, Volume 2010, Issue 8, pp. 1 - 19

We perform a global analysis of cosmological observables in generalized cosmologies which depart from ΛCDM models by allowing non-vanishing curvature Ω k 6= 0,...

Neutrino Physics | Quantum Physics | Cosmology of Theories beyond the SM | Quantum Field Theories, String Theory | Classical and Quantum Gravitation, Relativity Theory | Physics | Elementary Particles, Quantum Field Theory | MASSES | MICROWAVE BACKGROUND ANISOTROPIES | MASSIVE NEUTRINOS | PARAMETERS | ANGULAR POWER SPECTRUM | TEMPERATURE | CONSTRAINTS | PROBE | POLARIZATION | DOUBLE-BETA DECAY | PHYSICS, PARTICLES & FIELDS | Red shift | Parameters | Supernovae | Large scale structure of the universe | Big Bang theory | Equations of state | Beta decay | Cosmic microwave background | Neutrinos | Astronomical models | Hubble constant | Distance measurement | Dark energy

Neutrino Physics | Quantum Physics | Cosmology of Theories beyond the SM | Quantum Field Theories, String Theory | Classical and Quantum Gravitation, Relativity Theory | Physics | Elementary Particles, Quantum Field Theory | MASSES | MICROWAVE BACKGROUND ANISOTROPIES | MASSIVE NEUTRINOS | PARAMETERS | ANGULAR POWER SPECTRUM | TEMPERATURE | CONSTRAINTS | PROBE | POLARIZATION | DOUBLE-BETA DECAY | PHYSICS, PARTICLES & FIELDS | Red shift | Parameters | Supernovae | Large scale structure of the universe | Big Bang theory | Equations of state | Beta decay | Cosmic microwave background | Neutrinos | Astronomical models | Hubble constant | Distance measurement | Dark energy

Journal Article

Astrophysical Journal, ISSN 0004-637X, 02/2013, Volume 764, Issue 1, pp. 99 - 19

By implementing the widely used equations of state (EOS) from Lattimer & Swesty (LS) and H. Shen et al. (SHEN) in core-collapse supernova simulations, we...

equation of state | hydrodynamics | neutrinos | supernovae: general | stars: neutron | MASSIVE STARS | ACCRETION SHOCK INSTABILITY | CIRCLE-DOT STAR | RADIATION HYDRODYNAMICS | BLACK-HOLE FORMATION | EVOLUTION | MODELS | ASTRONOMY & ASTROPHYSICS | CORE-COLLAPSE SUPERNOVAE | GRAVITATIONAL-WAVE SIGNALS | SIMULATIONS | Equations of state | Heating | Neutrinos | Supernovas | Progenitors (astrophysics) | Explosions | Entropy | Two dimensional | Symmetry | LUMINOSITY | AXIAL SYMMETRY | INSTABILITY | NEUTRONS | ELECTRON ANTINEUTRINOS | HEATING | HYDRODYNAMICS | COMPARATIVE EVALUATIONS | SIMULATION | SUPERNOVAE | SPHERICAL CONFIGURATION | HEAVY LEPTONS | EXPLOSIONS | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | EQUATIONS OF STATE | ENTROPY

equation of state | hydrodynamics | neutrinos | supernovae: general | stars: neutron | MASSIVE STARS | ACCRETION SHOCK INSTABILITY | CIRCLE-DOT STAR | RADIATION HYDRODYNAMICS | BLACK-HOLE FORMATION | EVOLUTION | MODELS | ASTRONOMY & ASTROPHYSICS | CORE-COLLAPSE SUPERNOVAE | GRAVITATIONAL-WAVE SIGNALS | SIMULATIONS | Equations of state | Heating | Neutrinos | Supernovas | Progenitors (astrophysics) | Explosions | Entropy | Two dimensional | Symmetry | LUMINOSITY | AXIAL SYMMETRY | INSTABILITY | NEUTRONS | ELECTRON ANTINEUTRINOS | HEATING | HYDRODYNAMICS | COMPARATIVE EVALUATIONS | SIMULATION | SUPERNOVAE | SPHERICAL CONFIGURATION | HEAVY LEPTONS | EXPLOSIONS | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | EQUATIONS OF STATE | ENTROPY

Journal Article

The Astrophysical Journal Supplement Series, ISSN 0067-0049, 04/2006, Volume 163, Issue 2, pp. 335 - 343

We show that neutrino-driven pulsar kicks can increase the energy of the supernova shock. The observed large velocities of pulsars are believed to originate in...

Supernovae: general | PULSAR KICKS | CORE-COLLAPSE | MASSIVE STARS | CONVECTION | ASTRONOMY & ASTROPHYSICS | HYDRODYNAMICS | DARK-MATTER | STERILE NEUTRINOS | SIMULATIONS | supernovae : general | RADIATION | RUNAWAY STARS | Physics - Cosmology and Nongalactic Astrophysics | Physics - Earth and Planetary Astrophysics | Physics - Instrumentation and Methods for Astrophysics | Physics - High Energy Astrophysical Phenomena | Physics - Solar and Stellar Astrophysics | Physics - Astrophysics of Galaxies

Supernovae: general | PULSAR KICKS | CORE-COLLAPSE | MASSIVE STARS | CONVECTION | ASTRONOMY & ASTROPHYSICS | HYDRODYNAMICS | DARK-MATTER | STERILE NEUTRINOS | SIMULATIONS | supernovae : general | RADIATION | RUNAWAY STARS | Physics - Cosmology and Nongalactic Astrophysics | Physics - Earth and Planetary Astrophysics | Physics - Instrumentation and Methods for Astrophysics | Physics - High Energy Astrophysical Phenomena | Physics - Solar and Stellar Astrophysics | Physics - Astrophysics of Galaxies

Journal Article

Astrophysical Journal, Supplement Series, ISSN 0067-0049, 03/2012, Volume 199, Issue 1, pp. 17 - 32

We develop a numerical code to calculate the neutrino transfer with multi-energy and multi-angle in three dimensions (3D) for the study of core-collapse...

stars: massive | neutrinos | methods: numerical | supernovae: general | radiative transfer | stars: neutron | PAIR ANNIHILATION | POSTBOUNCE EVOLUTION | ACCRETION-SHOCK INSTABILITY | CIRCLE-DOT STAR | RADIATION HYDRODYNAMICS | BLACK-HOLE FORMATION | EXPLOSION MECHANISM | EQUATION-OF-STATE | RAY-TRACING METHOD | ASTRONOMY & ASTROPHYSICS | 3-DIMENSIONAL SIMULATIONS | Boltzmann equation | Computer simulation | Supernovae | Mathematical analysis | Neutrinos | Boltzmann transport equation | Mathematical models | Three dimensional | RADIANT HEAT TRANSFER | NEUTRINO REACTIONS | GRAVITATIONAL COLLAPSE | DISCRETE ORDINATE METHOD | EXACT SOLUTIONS | HYDRODYNAMICS | BOLTZMANN EQUATION | COMPARATIVE EVALUATIONS | SUPERNOVAE | THREE-DIMENSIONAL CALCULATIONS | COMPUTERIZED SIMULATION | RELATIVISTIC RANGE | COSMOLOGY | SYMMETRY | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | GENERAL RELATIVITY THEORY | COMPUTER CODES | DIFFUSION | EQUATIONS OF STATE | NEUTRINOS

stars: massive | neutrinos | methods: numerical | supernovae: general | radiative transfer | stars: neutron | PAIR ANNIHILATION | POSTBOUNCE EVOLUTION | ACCRETION-SHOCK INSTABILITY | CIRCLE-DOT STAR | RADIATION HYDRODYNAMICS | BLACK-HOLE FORMATION | EXPLOSION MECHANISM | EQUATION-OF-STATE | RAY-TRACING METHOD | ASTRONOMY & ASTROPHYSICS | 3-DIMENSIONAL SIMULATIONS | Boltzmann equation | Computer simulation | Supernovae | Mathematical analysis | Neutrinos | Boltzmann transport equation | Mathematical models | Three dimensional | RADIANT HEAT TRANSFER | NEUTRINO REACTIONS | GRAVITATIONAL COLLAPSE | DISCRETE ORDINATE METHOD | EXACT SOLUTIONS | HYDRODYNAMICS | BOLTZMANN EQUATION | COMPARATIVE EVALUATIONS | SUPERNOVAE | THREE-DIMENSIONAL CALCULATIONS | COMPUTERIZED SIMULATION | RELATIVISTIC RANGE | COSMOLOGY | SYMMETRY | ASTROPHYSICS, COSMOLOGY AND ASTRONOMY | GENERAL RELATIVITY THEORY | COMPUTER CODES | DIFFUSION | EQUATIONS OF STATE | NEUTRINOS

Journal Article

The Astrophysical Journal, ISSN 0004-637X, 12/2008, Volume 688, Issue 2, pp. 1176 - 1185

We study the progenitor dependence of black hole formation and its associated neutrino signal due to the gravitational collapse of a nonrotating massive star,...

Supernovae: General | Hydrodynamics | Stars: Neutron | Neutrinos | Equation of state | Black hole physics | MASSIVE STARS | equation of state | neutrinos | DELAYED COLLAPSE | METAL-POOR STARS | hydrodynamics | supernovae: general | stars: neutron | EQUATION-OF-STATE | EVOLUTION | black hole physics | NUCLEAR-MATTER | ASTRONOMY & ASTROPHYSICS | CORE-COLLAPSE SUPERNOVAE | HADRONIC PHASE-TRANSITIONS | NUCLEOSYNTHESIS

Supernovae: General | Hydrodynamics | Stars: Neutron | Neutrinos | Equation of state | Black hole physics | MASSIVE STARS | equation of state | neutrinos | DELAYED COLLAPSE | METAL-POOR STARS | hydrodynamics | supernovae: general | stars: neutron | EQUATION-OF-STATE | EVOLUTION | black hole physics | NUCLEAR-MATTER | ASTRONOMY & ASTROPHYSICS | CORE-COLLAPSE SUPERNOVAE | HADRONIC PHASE-TRANSITIONS | NUCLEOSYNTHESIS

Journal Article

Advances in High Energy Physics, ISSN 1687-7357, 1/2016, Volume 2016, pp. 1 - 11

The full energy shift of a massive Dirac neutrino in magnetized electron-positron plasma was investigated using the Matsubara imaginary time and real time...

MASSIVE NEUTRINO | DENSITY | MATTER | RADIATIVE DECAY | MOMENT | ELECTRON | EARLY UNIVERSE | FIELD | OSCILLATIONS | FINITE-TEMPERATURE | PHYSICS, PARTICLES & FIELDS | Studies | Temperature | Magnetic fields | Quantum field theory | Neutrinos | Phenomenology | Instrumentation and Detectors | High Energy Physics - Phenomenology | High Energy Physics | Astrophysics | Experiment | Article Subject | Physics | High Energy Astrophysical Phenomena

MASSIVE NEUTRINO | DENSITY | MATTER | RADIATIVE DECAY | MOMENT | ELECTRON | EARLY UNIVERSE | FIELD | OSCILLATIONS | FINITE-TEMPERATURE | PHYSICS, PARTICLES & FIELDS | Studies | Temperature | Magnetic fields | Quantum field theory | Neutrinos | Phenomenology | Instrumentation and Detectors | High Energy Physics - Phenomenology | High Energy Physics | Astrophysics | Experiment | Article Subject | Physics | High Energy Astrophysical Phenomena

Journal Article

Astrophysical Journal, ISSN 0004-637X, 09/2018, Volume 864, Issue 2, p. 171

We investigate r-process nucleosynthesis in 3D general-relativistic magnetohydrodynamic simulations of rapidly rotating strongly magnetized core collapse. The...

magnetohydrodynamics (MHD) neutrinos | gamma-ray burst: general | nuclear reactions, nucleosynthesis, abundances | instabilities | supernovae: general | WEAK INTERACTION RATES | MASSIVE STARS | MATTER | neutrinos | EXPLOSIONS | NEUTRINO-DRIVEN WINDS | NUCLEI | EVOLUTION | ASTRONOMY & ASTROPHYSICS | RATE TABLES | SIMULATIONS | MAGNETO-ROTATIONAL INSTABILITY | magnetohydrodynamics (MHD) | Collapse | Magnetohydrodynamics | Nuclear fusion | Equations of state | Leptons | Simulation | Supernovae | Neutrinos | Fluid flow | Magnetic fields | Rotation | Nuclear reactions | Physics - High Energy Astrophysical Phenomena | nucleosynthesis | magnetohydrodynamics | ASTRONOMY AND ASTROPHYSICS | gamma-ray burst: general instabilities magnetohydrodynamics neutrinos supernovae: general nucleosynthesis

magnetohydrodynamics (MHD) neutrinos | gamma-ray burst: general | nuclear reactions, nucleosynthesis, abundances | instabilities | supernovae: general | WEAK INTERACTION RATES | MASSIVE STARS | MATTER | neutrinos | EXPLOSIONS | NEUTRINO-DRIVEN WINDS | NUCLEI | EVOLUTION | ASTRONOMY & ASTROPHYSICS | RATE TABLES | SIMULATIONS | MAGNETO-ROTATIONAL INSTABILITY | magnetohydrodynamics (MHD) | Collapse | Magnetohydrodynamics | Nuclear fusion | Equations of state | Leptons | Simulation | Supernovae | Neutrinos | Fluid flow | Magnetic fields | Rotation | Nuclear reactions | Physics - High Energy Astrophysical Phenomena | nucleosynthesis | magnetohydrodynamics | ASTRONOMY AND ASTROPHYSICS | gamma-ray burst: general instabilities magnetohydrodynamics neutrinos supernovae: general nucleosynthesis

Journal Article

Astrophysical Journal, ISSN 0004-637X, 02/2016, Volume 818, Issue 2

We present four ab initio axisymmetric core-collapse supernova simulations initiated from 12, 15, 20, and 25 M⊙ zero-age main sequence progenitors. All of the...

nucleosynthesis | neutrinos | stars: evolution | abundances | stars: massive | nuclear reactions | supernovae: general | stars evolution | ASTRONOMY AND ASTROPHYSICS | Massive supernovae

nucleosynthesis | neutrinos | stars: evolution | abundances | stars: massive | nuclear reactions | supernovae: general | stars evolution | ASTRONOMY AND ASTROPHYSICS | Massive supernovae

Journal Article

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