JINA - Virtual Journal of Nuclear Astrophysics, 4 March 2022
Volume 20, Issue 9 (15 Articles)
- # 1 - Constraining Type Ia supernova explosions and early flux excesses with the Zwicky Transient Factory. (arXiv:2202.12914v1 [astro-ph.HE])
- # 2 - Electromagnetic counterparts of binary neutron star mergers leading to a strongly magnetized long-lived remnant neutron star. (arXiv:2202.13149v1 [astro-ph.HE])
- # 3 - History of Solar Neutrino Observations. (arXiv:2202.12421v1 [hep-ex])
- # 4 - Jet Launching from Binary Neutron Star Mergers: Incorporating Neutrino Transport and Magnetic Fields. (arXiv:2202.12901v1 [astro-ph.HE])
- # 5 - Low-luminosity supernovae: SN 2005cs and SN 2020cxd as very low-energy iron core-collapse explosions. (arXiv:2203.00473v1 [astro-ph.SR])
- # 6 - Insights into the equation of state of neutron-rich matter since GW170817. (arXiv:2202.13191v1 [nucl-th])
- # 7 - Gamow shell model description of the radiative capture reaction $^8$Li$(n,gamma)$$^9$Li. (arXiv:2202.13350v1 [nucl-th])
- # 8 - In-beam $gamma$-ray spectroscopy of $^{32}$Mg via direct reactions. (arXiv:2202.12820v1 [nucl-ex])
- # 9 - The Equation of State of Neutron-Rich Matter at Fourth Order of Chiral Effective Field Theory and the Radius of a Medium-Mass Neutron Star. (arXiv:2202.13475v1 [nucl-th])
- # 10 - The first large-scale shell-model calculation of the two-neutrino double beta decay of $^{76}$Ge to the ground and excited states in $^{76}$Se. (arXiv:2203.00109v1 [nucl-th])
- # 11 - Did astronomers see hints of first stars? Experiment casts doubt on bold claim
- # 12 - Thermalization of nuclear matter in heavy-ion collisions at Fermi energies
- # 13 - Correlated and integrated directionality for sub-MeV solar neutrinos in Borexino
- Physical Review D
- http://link.aps.org/doi/10.1103/PhysRevD.105.052002
- # 14 - First Directional Measurement of Sub-MeV Solar Neutrinos with Borexino
- Physical Review Letters
- http://link.aps.org/doi/10.1103/PhysRevLett.128.091803
- # 15 - Imposing multi-physics constraints at different densities on the neutron Star 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.

