JINA - Virtual Journal of Nuclear Astrophysics, 26 April 2024
Volume 22, Issue 17 (14 Articles)
- # 1 - Chemical abundances of LINER galaxies -- Nitrogen abundance estimations
- # 2 - Electron-capture supernovae in NS+He star systems and the double neutron star systems
- # 3 - Extended Skyrme effective interactions for transport model and neutron stars
- # 4 - Sensitivity of 3D Convective Urca Simulations to Changes in Urca Reactions
- # 5 - Stellar Abundances at the Center of Early Type Galaxies with Fine Structure
- # 6 - Three dimensional end-to-end simulation for kilonova emission from a black-hole neutron-star merger
- # 7 - Magnetic dipole strength in $^{58}$Ni from forward-angle inelastic proton scattering
- # 8 - Parameter dependence of the $beta$-decay properties of neutron-rich Zr isotopes within the interacting boson model
- # 9 - Including a luminous central remnant in radiative transfer simulations for Type Iax supernovae
- Monthly Notices of the Royal Astronomical Society - Volume: 530, Issue: 2
- https://academic.oup.com/mnras/article/530/2/1457/7634369?rss=1
- # 10 - Proto-neutron star convection and the neutrino-driven wind: implications for the νp-process
- Monthly Notices of the Royal Astronomical Society - Volume: 530, Issue: 2
- https://academic.oup.com/mnras/article/530/2/2001/7645470?rss=1
- # 11 - $^{21}mathrm{Ne}$ energy levels approaching the $α$-particle threshold
- Physical Review C
- http://link.aps.org/doi/10.1103/PhysRevC.109.044323
- # 12 - Neutrino-driven Outflows and the Elemental Abundance Patterns of Very Metal-poor Stars
- The Astrophysical Journal
- https://doi.org/10.3847/1538-4357/ad2dfb
- # 13 - General-relativistic Radiation Transport Scheme in Gmunu. II. Implementation of Novel Microphysical Library for Neutrino Radiation—Weakhub
- The Astrophysical Journal Supplement
- https://doi.org/10.3847/1538-4365/ad2fbd
- # 14 - Effects of dilute neutron matter on the neutron star crust equation of state
This material is based upon work supported in part by the U.S. Department of Energy, Office of Science, Office of Nuclear Physics, under Award Number DE-SC0026204.

