JINA - Virtual Journal of Nuclear Astrophysics, 19 May 2023
Volume 21, Issue 20 (41 Articles)
- # 1 - A multi-messenger model for neutron star - black hole mergers. (arXiv:2305.07582v1 [astro-ph.HE])
- # 2 - Deducing Neutron Star Equation of State from Telescope Spectra with Machine-learning-derived Likelihoods. (arXiv:2305.07442v1 [astro-ph.HE])
- # 3 - Faint but not forgotten. I. First results from a search for astrospheres around AGB stars in the far-ultraviolet. (arXiv:2305.07735v1 [astro-ph.SR])
- # 4 - Fission and fusion of heavy nuclei induced by the passage of a radiation-mediated shock in BNS mergers. (arXiv:2305.08575v1 [astro-ph.HE])
- # 5 - How do supernova remnants cool? -- I. Morphology, optical emission lines, and shocks. (arXiv:2305.07652v1 [astro-ph.HE])
- # 6 - Multi-messenger observations of core-collapse supernovae: Exploiting the standing accretion shock instability. (arXiv:2305.07688v1 [astro-ph.HE])
- # 7 - Peculiar Spectral Evolution of the Type I Supernova 2019eix: A Possible Double Detonation from a Helium Shell on a Sub-Chandrasekhar-mass White Dwarf. (arXiv:2305.07708v1 [astro-ph.HE])
- # 8 - Phase Transition Phenomenology with Nonparametric Representations of the Neutron Star Equation of State. (arXiv:2305.07411v1 [astro-ph.HE])
- # 9 - Physics of Binary Star Evolution -- from Stars to X-ray Binaries and Gravitational Wave Sources. (arXiv:2305.09388v1 [astro-ph.HE])
- # 10 - Reducing the uncertainty on the Hubble constant up to 35% with an improved statistical analysis: different best-fit likelihoods for Supernovae Ia, Baryon Acoustic Oscillations, Quasars, and Gamma-Ray Bursts. (arXiv:2305.10030v1 [astro-ph.CO])
- # 11 - Searches for continuous gravitational waves from neutron stars: A twenty-year retrospective. (arXiv:2305.07106v1 [gr-qc])
- # 12 - SN 2016ije: An SN 2002es-like Type Ia Supernova Exploded in a Metal-poor and Low-surface Brightness Galaxy. (arXiv:2305.09417v1 [astro-ph.HE])
- # 13 - The nuclear reaction network WinNet. (arXiv:2305.07048v1 [astro-ph.IM])
- # 14 - Time-independent Simulations of Steady-State Accretion with Nuclear Burning. (arXiv:2305.10627v1 [astro-ph.HE])
- # 15 - Understanding radioactive ion beam production at ISAC through yield measurements and simulations. (arXiv:2305.10539v1 [physics.acc-ph])
- # 16 - Energy and Angle Dependence of Neutrino Scattering Rates in Proto-Neutron Star and Supernova Matter within Skyrme RPA. (arXiv:2305.09499v1 [nucl-th])
- # 17 - Evidence of bi-cluster structure in the ground state of $^{20}$Ne. (arXiv:2305.09182v1 [nucl-th])
- # 18 - Production of $p$-nuclei from $r$-process seeds: the $nu r$-process. (arXiv:2305.11050v1 [astro-ph.HE])
- # 19 - Synthesis of elements in compact stars in pycnonuclear reactions with Carbon isotopes: Quasibound states versus states of zero-points vibrations. (arXiv:2305.09389v1 [nucl-th])
- # 20 - Large-Scale Convection during Gravitational Collapse with Neutrino Transport in 2D and 3D Models on Fine Grids
- # 21 - Analytic approach to axion-like-particle emission in core-collapse supernovae
- # 22 - Probing gamma-ray burst afterglows with the Cherenkov Telescope Array
- # 23 - Signatures of wakefield acceleration in astrophysical jets via gamma-rays and UHECRs
- # 24 - Thermal evolution of neutron stars in soft X-ray transients with thermodynamically consistent models of the accreted crust
- # 25 - A radio-detected type Ia supernova with helium-rich circumstellar material
- # 26 - Exceptionally bright optical emission from a rare and distant gamma-ray burst
- Nature Astronomy
- https://www.nature.com/articles/s41550-023-01972-4
- # 27 - A systematic analysis for one proton radioactivity of ground state nuclei
- # 28 - Bayesian inference of neutron-star observables based on effective nuclear interactions
- Physical Review C
- http://link.aps.org/doi/10.1103/PhysRevC.107.055803
- # 29 - Experimental and theoretical study of the $^{65}mathrm{Cu}(n,p)^{65}mathrm{Ni}$ reaction cross section from reaction threshold up to 25 MeV
- Physical Review C
- http://link.aps.org/doi/10.1103/PhysRevC.107.054607
- # 30 - Statistical approach of nuclear multifragmentation with a realistic nuclear equation of state
- Physical Review C
- http://link.aps.org/doi/10.1103/PhysRevC.107.054605
- # 31 - Systematic analysis of the impacts of symmetry energy parameters on neutron star properties
- Physical Review C
- http://link.aps.org/doi/10.1103/PhysRevC.107.055804
- # 32 - Big bang nucleosynthesis and early dark energy in light of the EMPRESS ${Y}_{p}$ results and the ${H}_{0}$ tension
- Physical Review D
- http://link.aps.org/doi/10.1103/PhysRevD.107.103520
- # 33 - Spontaneous scalarization as a new core-collapse supernova mechanism and its multimessenger signals
- Physical Review D
- http://link.aps.org/doi/10.1103/PhysRevD.107.103025
- # 34 - Degeneracy in the Inference of Phase Transitions in the Neutron Star Equation of State from Gravitational Wave Data
- Physical Review Letters
- http://link.aps.org/doi/10.1103/PhysRevLett.130.201403
- # 35 - Hydrogen-triggered X-Ray Bursts from SAX J1808.4−3658? The Onset of Nuclear Burning
- The Astrophysical Journal
- https://doi.org/10.3847/1538-4357/acc24f
- # 36 - Nucleosynthesis of Binary-stripped Stars
- The Astrophysical Journal
- https://doi.org/10.3847/1538-4357/acc315
- # 37 - Proposed Lunar Measurements of r-Process Radioisotopes to Distinguish the Origin of Deep-sea 244Pu
- The Astrophysical Journal
- https://doi.org/10.3847/1538-4357/acbeaa
- # 38 - The Magnificent Five Images of Supernova Refsdal: Time Delay and Magnification Measurements
- The Astrophysical Journal
- https://doi.org/10.3847/1538-4357/ac4ccb
- # 39 - Uranium Abundances and Ages of r-process Enhanced Stars with Novel U ii Lines
- The Astrophysical Journal
- https://doi.org/10.3847/1538-4357/acb8af
- # 40 - First Detection of the Powerful Gamma-Ray Burst GRB 221009A by the THEMIS ESA and SST Particle Detectors on 2022 October 9
- The Astrophysical Journal Letters
- https://doi.org/10.3847/2041-8213/accfa0
- # 41 - Measuring neutron capture cross sections of radioactive nuclei
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.

