JINA - Virtual Journal of Nuclear Astrophysics, 1 March 2019
Volume 17, Issue 9 (12 Articles)
- # 1 - $^{3}{rm He}(alpha, gamma)^{7}{rm Be}$ and $^{3}{rm H}(alpha,gamma)^{7}{rm Li}$ reaction rates and the implication for Big Bang nucleosynthesis in the potential model. (arXiv:1902.09767v1 [nucl-th])
- # 2 - A Systematic Study Of Superluminous Supernova Lightcurve Models Using Clustering. (arXiv:1902.09484v1 [astro-ph.HE])
- # 3 - Discovery of a nitrogen-enhanced metal-poor binary system: Possible evidence for pollution from an extinct massive AGB Star. (arXiv:1902.10635v1 [astro-ph.GA])
- # 4 - Effects of spin on magnetized binary neutron star mergers and jet launching. (arXiv:1902.08636v1 [astro-ph.HE])
- # 5 - Neutron-induced cross sections -- from raw data to astrophysical rates. (arXiv:1902.09838v1 [astro-ph.IM])
- # 6 - Reexamination of the $beta^+$ decay process of $^{13}rm{N}$ nucleus. (arXiv:1902.10925v1 [nucl-th])
- # 7 - Reproductions of super-orbital X-ray light-curves with the precessing accretion ring model and implications on accretion flows through accretion rings. (arXiv:1902.08917v1 [astro-ph.HE])
- # 8 - Theoretical study of the $alpha+d$ $rightarrow$ $^6$Li + $gamma $ astrophysical capture process in a three-body model. (arXiv:1902.09764v1 [nucl-th])
- # 9 - Reduction of the maximum mass-loss rate of OH/IR stars due to unnoticed binary interaction
- Reduction of the maximum mass-loss rate of OH/IR stars due to unnoticed binary interaction
- https://www.nature.com/articles/s41550-019-0703-5
- # 10 - $^{56,54}mathrm{Fe}(n,α)^{53,51}mathrm{Cr}$ cross sections in the MeV region
- Physical Review C
- http://link.aps.org/doi/10.1103/PhysRevC.99.024619
- # 11 - Reactions leading to the first excited states of $^{7}mathrm{Li}$ and $^{7}mathrm{Be}$ and isospin-mixed states in $^{8}mathrm{Be}$
- Physical Review C
- http://link.aps.org/doi/10.1103/PhysRevC.99.024320
- # 12 - Experimental constraints on the $^{73}mathrm{Zn}(n,γ)^{74}mathrm{Zn}$ reaction rate
- Physical Review C
- http://link.aps.org/doi/10.1103/PhysRevC.99.034601