JINA - Virtual Journal of Nuclear Astrophysics, 30 May 2025
Volume 23, Issue 14 (34 Articles)
- # 1 - Charting circumstellar chemistry of carbon-rich asymptotic giant branch stars. II. Abundances and spatial distributions of CS
- # 2 - Chemical Abundances in the Milky Way's Nuclear Stellar Disc
- # 3 - Connecting the m-dots: accretion rates and thermonuclear burst recurrence times on neutron stars and white dwarfs
- # 4 - Explodability criteria for the neutrino-driven supernova mechanism
- # 5 - Infrared diagnostics of late-time core-collapse supernova spectra
- # 6 - Mixing neutron star material into the jets in the common envelope jets supernova r-process scenario
- # 7 - Neutron Star crust informed by nuclear structure data
- # 8 - Observing Supernova Neutrino Light Curves with Super-Kamiokande.VI. A Practical Data Analysis Technique Considering Realistic Experimental Backgrounds
- # 9 - Improved direct measurement of low-energy resonances in the $^{21}$Ne(p,$gamma$)$^{22}$Na reaction
- # 10 - Astrophysics with Compact Objects: An Indian Perspective, Present Status and Future Vision
- # 11 - Constraints on maximum neutron star mass from proto-neutron star evolution
- # 12 - Fully general relativistic description of rapidly-rotating axially-symmetric neutron stars for constraining nuclear matter equations of state
- # 13 - High-precision Penning trap mass measurements of neutron-rich chlorine isotopes at the N=28 shell closure
- # 14 - Microscopic constraints for the equation of state and structure of neutron stars: a Bayesian model mixing framework
- # 15 - Prospect of Constraining the EoS of Neutron Stars Using Post-Merger Signals
- # 16 - The $alpha+{}^2n+{}^2n$ 3-body cluster structures and dineutron breaking in ${}^8 mathrm{He}$
- # 17 - Time Evolution of Prompt Gamma-Ray Emission in $^{252}$Cf(sf) and $^{233,235}$U($n$,f) Reactions
- # 18 - Emulation of the calculations of final r-process abundance patterns with a neural network
- Journal of Physics G
- https://doi.org/10.1088/1361-6471/add360
- # 19 - CTADIR: A He Cryogenic TArget for DIrect Reactions at low energy
- # 20 - Excitation Functions of (α,xn) Reactions in Natural Sb
- # 21 - Study of β-decay properties of N = 81 & 82 isotones
- # 22 - What's new? An ab initio investigation of the 3He-4He radiative capture into 7Be
- # 23 - Evidence for shape coexistence in $^{120}mathrm{Sn}$ from the first ${0}_{3}^{+}$ lifetime measurement
- Physical Review C
- http://link.aps.org/doi/10.1103/PhysRevC.111.L051307
- # 24 - Extension of the particle x-ray coincidence technique: The lifetimes and branching ratios apparatus
- Physical Review C
- http://link.aps.org/doi/10.1103/PhysRevC.111.055806
- # 25 - Data Driven Approach for Extracting Tidal Information from Neutron Star Binary Mergers Observed with the Einstein Telescope
- Physical Review Letters
- http://link.aps.org/doi/10.1103/PhysRevLett.134.211401
- # 26 - Experimental Test of the Ratio Method for Nuclear-Reaction Analysis
- Physical Review Letters
- http://link.aps.org/doi/10.1103/PhysRevLett.134.212501
- # 27 - Quantum physics of stars
- Reviews of Modern Physics
- http://link.aps.org/doi/10.1103/RevModPhys.97.025003
- # 28 - Model-independent Determination of the Tidal Deformability of a 1.4 M⊙ Neutron Star from Gravitational-wave Measurements
- The Astrophysical Journal
- https://doi.org/10.3847/1538-4357/add5ef
- # 29 - r-process Nucleosynthesis and Radioactively Powered Transients from Magnetar Giant Flares
- The Astrophysical Journal
- https://doi.org/10.3847/1538-4357/adceb7
- # 30 - Comparing $$^{3}$$He content in magnetron sputtered and implanted targets for nuclear studies
- # 31 - Evaluation of the p-11B reaction cross section through a silicon telescope in the 0.3–4.7 MeV range
- # 32 - Experimental investigations on near-barrier reactions with weakly-bound nuclei at the China Institute of Atomic Energy
- # 33 - Fine-tunings in nucleosynthesis and the emergence of life: status and perspectives
- # 34 - Impact of the uncertainty of nuclear mass predictions on $$beta $$-decay half-lives predictions based on the gross theory
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.

