Reviews of Modern Physics, ISSN 0034-6861, 07/2003, Volume 75, Issue 3, pp. 819 - 862

Recent experimental data and progress in nuclear structure modeling have led to improved descriptions of astrophysically important weak-interaction processes....

GAMOW-TELLER STRENGTH | NEUTRINO-DRIVEN WINDS | INTERMEDIATE-MASS NUCLEI | EQUATION-OF-STATE | S-PROCESS NUCLEOSYNTHESIS | PHYSICS, MULTIDISCIPLINARY | STELLAR CORE COLLAPSE | R-PROCESS NUCLEOSYNTHESIS | ABSORPTION CROSS-SECTIONS | SHELL-MODEL CALCULATIONS | RANDOM-PHASE-APPROXIMATION | Weak interactions (Nuclear physics) | Nuclear structure | Research | Nucleosynthesis

GAMOW-TELLER STRENGTH | NEUTRINO-DRIVEN WINDS | INTERMEDIATE-MASS NUCLEI | EQUATION-OF-STATE | S-PROCESS NUCLEOSYNTHESIS | PHYSICS, MULTIDISCIPLINARY | STELLAR CORE COLLAPSE | R-PROCESS NUCLEOSYNTHESIS | ABSORPTION CROSS-SECTIONS | SHELL-MODEL CALCULATIONS | RANDOM-PHASE-APPROXIMATION | Weak interactions (Nuclear physics) | Nuclear structure | Research | Nucleosynthesis

Journal Article

Reviews of Modern Physics, ISSN 0034-6861, 04/2005, Volume 77, Issue 2, pp. 427 - 488

The last decade has witnessed both quantitative and qualitative progress in shell-model studies, which have resulted in remarkable gains in our understanding...

MAGNETIC DIPOLE RESPONSE | PLUS-QUADRUPOLE MODEL | GAMOW-TELLER STRENGTH | INTERMEDIATE-MASS NUCLEI | PROTON DRIP-LINE | PHYSICS, MULTIDISCIPLINARY | MONTE-CARLO CALCULATIONS | WEAK-INTERACTION RATES | QUASI-SU TRUNCATION SCHEME | NEUTRON-RICH NUCLEI | DOUBLE-BETA DECAY | Nuclear structure | Analysis | Physics - Nuclear Theory | Nuclear Theory | Physics | DOUBLE BETA DECAY | SPECIFICITY | POTENTIALS | THREE-BODY PROBLEM | ISOSPIN | ROTATIONAL STATES | GAMOW-TELLER RULES | NUCLEAR PHYSICS AND RADIATION PHYSICS | NUCLEON-NUCLEON INTERACTIONS | TWO-BODY PROBLEM | MATRICES | NUCLEAR FORCES | NUCLEAR STRUCTURE | SHELL MODELS | NEUTRON-RICH ISOTOPES | SATURATION

MAGNETIC DIPOLE RESPONSE | PLUS-QUADRUPOLE MODEL | GAMOW-TELLER STRENGTH | INTERMEDIATE-MASS NUCLEI | PROTON DRIP-LINE | PHYSICS, MULTIDISCIPLINARY | MONTE-CARLO CALCULATIONS | WEAK-INTERACTION RATES | QUASI-SU TRUNCATION SCHEME | NEUTRON-RICH NUCLEI | DOUBLE-BETA DECAY | Nuclear structure | Analysis | Physics - Nuclear Theory | Nuclear Theory | Physics | DOUBLE BETA DECAY | SPECIFICITY | POTENTIALS | THREE-BODY PROBLEM | ISOSPIN | ROTATIONAL STATES | GAMOW-TELLER RULES | NUCLEAR PHYSICS AND RADIATION PHYSICS | NUCLEON-NUCLEON INTERACTIONS | TWO-BODY PROBLEM | MATRICES | NUCLEAR FORCES | NUCLEAR STRUCTURE | SHELL MODELS | NEUTRON-RICH ISOTOPES | SATURATION

Journal Article

Monthly Notices of the Royal Astronomical Society, ISSN 0035-8711, 2010, Volume 406, Issue 4, pp. 2650 - 2662

The most promising astrophysical sources of kHz gravitational waves (GWs) are the inspiral and merger of binary neutron star(NS)/black hole systems. Maximizing...

binaries: close | gamma‐ray burst: general | nuclear reactions, nucleosynthesis, abundances | gravitation | supernovae: general | stars: neutron | Supernovae: general | Nuclear reactions, nucleosynthesis, abundances | Gravitation | Gamma-ray burst: general | Stars: neutron | Binaries: close | nucleosynthesis | gamma-ray burst: general | abundances | ASTRONOMY & ASTROPHYSICS | nuclear reactions | Acquisitions and mergers | Particle accelerators | Emissions (Pollution) | Analysis | Gamma rays | Astrophysics | Black holes | Electromagnetics | Stars & galaxies | Nuclear physics | Acquisitions | Surveys | Monte Carlo methods | Ejecta | Computer simulation | Luminosity | Mathematical models | Radioactive decay

binaries: close | gamma‐ray burst: general | nuclear reactions, nucleosynthesis, abundances | gravitation | supernovae: general | stars: neutron | Supernovae: general | Nuclear reactions, nucleosynthesis, abundances | Gravitation | Gamma-ray burst: general | Stars: neutron | Binaries: close | nucleosynthesis | gamma-ray burst: general | abundances | ASTRONOMY & ASTROPHYSICS | nuclear reactions | Acquisitions and mergers | Particle accelerators | Emissions (Pollution) | Analysis | Gamma rays | Astrophysics | Black holes | Electromagnetics | Stars & galaxies | Nuclear physics | Acquisitions | Surveys | Monte Carlo methods | Ejecta | Computer simulation | Luminosity | Mathematical models | Radioactive decay

Journal Article

Physical Review C - Nuclear Physics, ISSN 0556-2813, 06/2009, Volume 79, Issue 6, pp. 064310 - 9

We calculate the low-lying spectra and several high-spin states of zirconium isotopes (Z=40) with neutron numbers from N=50 to N=58 using a large valence space...

STATES | MASS REGION | CLOSURE | ZR-97 | PHYSICS, NUCLEAR | SHAPE COEXISTENCE | NUCLEAR-STRUCTURE | DEFORMATION | Nuclear Theory | Physics | CORRECTIONS | G MATRIX | NEUTRONS | NUCLEAR PROPERTIES | HIGH SPIN STATES | MONOPOLES | INTERACTIONS | NICKEL 78 | DEFORMED NUCLEI | COMPUTERIZED SIMULATION | SPHERICAL CONFIGURATION | NUCLEAR PHYSICS AND RADIATION PHYSICS | ZIRCONIUM 100 | ZIRCONIUM 96 | ZIRCONIUM ISOTOPES | SHELL MODELS | SPECTRA | ZIRCONIUM 98

STATES | MASS REGION | CLOSURE | ZR-97 | PHYSICS, NUCLEAR | SHAPE COEXISTENCE | NUCLEAR-STRUCTURE | DEFORMATION | Nuclear Theory | Physics | CORRECTIONS | G MATRIX | NEUTRONS | NUCLEAR PROPERTIES | HIGH SPIN STATES | MONOPOLES | INTERACTIONS | NICKEL 78 | DEFORMED NUCLEI | COMPUTERIZED SIMULATION | SPHERICAL CONFIGURATION | NUCLEAR PHYSICS AND RADIATION PHYSICS | ZIRCONIUM 100 | ZIRCONIUM 96 | ZIRCONIUM ISOTOPES | SHELL MODELS | SPECTRA | ZIRCONIUM 98

Journal Article

Progress in Particle and Nuclear Physics, ISSN 0146-6410, 11/2015, Volume 85, pp. 33 - 81

The description of nuclear reactions induced by supernova neutrinos has witnessed significant progress during the recent years. On one hand this progress is...

Nuclear models | Nucleosythesis | Supernovae | Neutrino | GAMOW-TELLER STRENGTH | R-PROCESS NUCLEOSYNTHESIS | PHYSICS, NUCLEAR | MAGNETIC DIPOLE RESPONSE | EQUATION-OF-STATE | INTERMEDIATE-MASS NUCLEI | CHARGE-EXCHANGE REACTIONS | WEAK-INTERACTION RATES | CORE-COLLAPSE SUPERNOVAE | DOUBLE-BETA DECAY | SHELL-MODEL CALCULATIONS | PHYSICS, PARTICLES & FIELDS

Nuclear models | Nucleosythesis | Supernovae | Neutrino | GAMOW-TELLER STRENGTH | R-PROCESS NUCLEOSYNTHESIS | PHYSICS, NUCLEAR | MAGNETIC DIPOLE RESPONSE | EQUATION-OF-STATE | INTERMEDIATE-MASS NUCLEI | CHARGE-EXCHANGE REACTIONS | WEAK-INTERACTION RATES | CORE-COLLAPSE SUPERNOVAE | DOUBLE-BETA DECAY | SHELL-MODEL CALCULATIONS | PHYSICS, PARTICLES & FIELDS

Journal Article

Physical Review C - Nuclear Physics, ISSN 0556-2813, 02/2012, Volume 85, Issue 2

We present a systematics of fission barriers and fission lifetimes for the whole landscape of superheavy elements (SHE), i.e., nuclei with Z >= 100. The...

CONSISTENT | ISOTOPES | DENSITIES | SYSTEMATICS | EFFECTIVE FORCES | BARRIERS | PHYSICS, NUCLEAR | PAIRING INTERACTION | PARAMETRIZATION | NEUTRON-RICH | SUPERHEAVY NUCLEI | Physics - Nuclear Theory

CONSISTENT | ISOTOPES | DENSITIES | SYSTEMATICS | EFFECTIVE FORCES | BARRIERS | PHYSICS, NUCLEAR | PAIRING INTERACTION | PARAMETRIZATION | NEUTRON-RICH | SUPERHEAVY NUCLEI | Physics - Nuclear Theory

Journal Article

Physical Review Letters, ISSN 0031-9007, 12/2012, Volume 109, Issue 25, p. 251104

We perform three-flavor Boltzmann neutrino transport radiation hydrodynamics simulations covering a period of 3 s after the formation of a protoneutron star in...

DRIVEN WINDS | EQUATION-OF-STATE | SUPERNOVA | NUCLEOSYNTHESIS | PHYSICS, MULTIDISCIPLINARY

DRIVEN WINDS | EQUATION-OF-STATE | SUPERNOVA | NUCLEOSYNTHESIS | PHYSICS, MULTIDISCIPLINARY

Journal Article

Journal of Physics G: Nuclear and Particle Physics, ISSN 0954-3899, 04/2014, Volume 41, Issue 4, pp. 44008 - 16

Observations of metal-poor stars indicate that at least two different nucleosynthesis sites contribute to the production of r-process elements. One site is...

neutrino-driven wind | r-process nucleosynthesis | supernova neutrinos | SURVEY HERES | S-PROCESS | PHYSICS, NUCLEAR | R-PROCESS | DRIVEN WINDS | EQUATION-OF-STATE | EVOLUTION | NUCLEAR-MATTER | NEUTRON-CAPTURE ELEMENTS | CORE-COLLAPSE SUPERNOVAE | GIANT BRANCH STARS | PHYSICS, PARTICLES & FIELDS | Enrichment | Correlation | Computer simulation | Neutrinos | Stars | Supernovas | Mathematical models | Energy (nuclear)

neutrino-driven wind | r-process nucleosynthesis | supernova neutrinos | SURVEY HERES | S-PROCESS | PHYSICS, NUCLEAR | R-PROCESS | DRIVEN WINDS | EQUATION-OF-STATE | EVOLUTION | NUCLEAR-MATTER | NEUTRON-CAPTURE ELEMENTS | CORE-COLLAPSE SUPERNOVAE | GIANT BRANCH STARS | PHYSICS, PARTICLES & FIELDS | Enrichment | Correlation | Computer simulation | Neutrinos | Stars | Supernovas | Mathematical models | Energy (nuclear)

Journal Article

ASTROPHYSICAL JOURNAL, ISSN 0004-637X, 12/2019, Volume 887, Issue 1, p. 58

We revisit the rates of neutrino pair emission and absorption from nucleon-nucleon bremsstrahlung in supernova matter using the T-matrix formalism in the...

WEAK INTERACTION RATES | SPIN FLUCTUATIONS | REDUCTION | Core-collapse supernovae | ASTRONOMY & ASTROPHYSICS | STARS | Supernova neutrinos | EMISSIVITIES | Supernova | Pions | Supernovae | Computer simulation | Bremsstrahlung | Mathematical analysis | Neutrinos | Nucleons | Field theory

WEAK INTERACTION RATES | SPIN FLUCTUATIONS | REDUCTION | Core-collapse supernovae | ASTRONOMY & ASTROPHYSICS | STARS | Supernova neutrinos | EMISSIVITIES | Supernova | Pions | Supernovae | Computer simulation | Bremsstrahlung | Mathematical analysis | Neutrinos | Nucleons | Field theory

Journal Article

Reports on Progress in Physics, ISSN 0034-4885, 09/2007, Volume 70, Issue 9, pp. 1525 - 1582

The nuclear structure in regions of the Segre chart which are of astrophysical importance is reviewed. The main emphasis is put on those nuclei that are...

MONTE-CARLO | MEAN-FIELD | INTERMEDIATE-MASS NUCLEI | GAMOW-TELLER STRENGTH | PHYSICS, MULTIDISCIPLINARY | R-PROCESS NUCLEOSYNTHESIS | WEAK-INTERACTION RATES | FULL PF SHELL | NEUTRON-RICH NUCLEI | ISOSPIN STRENGTH DISTRIBUTIONS | SHELL-MODEL CALCULATIONS

MONTE-CARLO | MEAN-FIELD | INTERMEDIATE-MASS NUCLEI | GAMOW-TELLER STRENGTH | PHYSICS, MULTIDISCIPLINARY | R-PROCESS NUCLEOSYNTHESIS | WEAK-INTERACTION RATES | FULL PF SHELL | NEUTRON-RICH NUCLEI | ISOSPIN STRENGTH DISTRIBUTIONS | SHELL-MODEL CALCULATIONS

Journal Article