JINA - Virtual Journal of Nuclear Astrophysics, 18 September 2020
Volume 18, Issue 38 (18 Articles)
- # 1 - Bounds on neutrino-scalar non-standard interactions from big bang nucleosynthesis. (arXiv:2009.08104v1 [hep-ph])
- # 2 - Classifying the Equation of State from Rotating Core Collapse Gravitational Waves with Deep Learning. (arXiv:2009.07367v1 [astro-ph.IM])
- # 3 - Depletion and fractionation of nitrogen in collapsing cores. (arXiv:2009.06393v1 [astro-ph.GA])
- # 4 - Evaluation of Experimental Constraints on the $^{44}$Ti($alpha$,p)$^{47}$V Reaction Cross Section Relevant for Supernovae. (arXiv:2008.00153v2 [astro-ph.SR] UPDATED)
- # 5 - Impact of magnetic field on neutrino-matter interactions in core-collapse supernova. (arXiv:2009.07733v1 [astro-ph.HE])
- # 6 - Limiting masses and radii of neutron stars and their implications. (arXiv:2009.06441v1 [nucl-th])
- # 7 - Model Light Curves for Type Ib and Ic Supernovae. (arXiv:2009.06868v1 [astro-ph.HE])
- # 8 - Neutron conversion-diffusion: a new model for structured short gamma-ray burst jets compatible with GRB 170817. (arXiv:2009.07507v1 [astro-ph.HE])
- # 9 - Polarized kilonovae from black hole-neutron star mergers. (arXiv:2009.07279v1 [astro-ph.HE])
- # 10 - Type Ia Supernovae from wide white-dwarfs triples. (arXiv:2009.08245v1 [astro-ph.HE])
- # 11 - Final Results of GERDA on the Search for Neutrinoless Double-$beta$ Decay. (arXiv:2009.06079v1 [nucl-ex])
- # 12 - Impact of the neutron-star deformability on equation of state parameters. (arXiv:2009.05239v1 [nucl-th])
- # 13 - Planet discovered transiting a dead star
- # 14 - On the Event Rate and Luminosity Function of Superluminous Supernovae
- # 15 - New Era of Resonance Reaction Studies
- # 16 - Nucleosynthesis-Rate Dependence of Abundances of Nuclei Produced in the r-Process
- # 17 - Simulations of Early Kilonova Emission from Neutron Star Mergers
- The Astrophysical Journal
- http://iopscience.iop.org/0004-637X/901/1/29
- # 18 - Trojan horse method as an indirect approach to study resonant reactions in nuclear astrophysics
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.

