JINA - Virtual Journal of Nuclear Astrophysics, 11 August 2023
Volume 21, Issue 32 (26 Articles)
- # 1 - A catalogue of unusually long thermonuclear bursts on neutron stars. (arXiv:2308.03499v1 [astro-ph.HE])
- # 2 - Bayesian inference from gravitational waves in fast-rotating, core-collapse supernovae. (arXiv:2308.03456v1 [astro-ph.HE])
- # 3 - Chemodynamic analysis of four $r$-process enhanced stars observed with GTC. (arXiv:2308.05097v1 [astro-ph.SR])
- # 4 - Efficient production of nuclear isomer $^{93m}$Mo with laser-accelerated proton beam and an astrophysical implication on $^{92m}$Mo production. (arXiv:2308.02994v1 [nucl-ex])
- # 5 - Gamma-Ray Bursts Observed by the Transiting Exoplanet Survey Satellite: Prompt Optical Counterparts and Afterglows of Swift-XRT Localized GRBs. (arXiv:2308.05148v1 [astro-ph.HE])
- # 6 - Neutrinos and nucleosynthesis of elements. (arXiv:2308.03962v1 [astro-ph.HE])
- # 7 - Probing depressive symptoms and the desire to leave academia among scientists in large, international collaborations in STEM. (arXiv:2308.05107v1 [physics.soc-ph])
- # 8 - Radiative neutron capture reaction rates for stellar nucleosynthesis. (arXiv:2308.02579v1 [nucl-th])
- # 9 - Snowflakes in a furnace: formation of CO and dust in a recurrent nova eruption. (arXiv:2308.02871v1 [astro-ph.SR])
- # 10 - The elemental abundances of quiescent galaxies in the LEGA-C survey: the (non-)evolution of [{alpha}/Fe] from z = 0.75 to z = 0. (arXiv:2308.03441v1 [astro-ph.GA])
- # 11 - Sensitivities for coherent elastic scattering of solar and supernova neutrinos with future NaI(Tl) dark matter search detectors of COSINE-200/1T
- # 12 - X-ray reprocessing: Through the eclipse spectra of low mass X-ray binaries with XMM-Newton
- # 13 - The capability of water Cherenkov detectors arrays of the LAGO project to detect Gamma-Ray Burst and high energy astrophysics sources
- # 14 - Experimental determination of the $^{3}mathrm{He}(α,γ)^{7}mathrm{Be}$ reaction cross section above the $^{7}mathrm{Be}$ proton separation threshold
- Physical Review C
- http://link.aps.org/doi/10.1103/PhysRevC.108.025802
- # 15 - New experimental constraint on the $^{185}mathrm{W}(n,γ)^{186}mathrm{W}$ cross section
- Physical Review C
- http://link.aps.org/doi/10.1103/PhysRevC.108.025804
- # 16 - Unified equations of state for cold nonaccreting neutron stars with Brussels-Montreal functionals. IV. Role of the symmetry energy in pasta phases
- Physical Review C
- http://link.aps.org/doi/10.1103/PhysRevC.108.025805
- # 17 - Gravitational wave signatures from reheating
- Physical Review D
- http://link.aps.org/doi/10.1103/PhysRevD.108.036006
- # 18 - Early structure formation from cosmic string loops in light of early JWST observations
- Physical Review D
- http://link.aps.org/doi/10.1103/PhysRevD.108.043510
- # 19 - Machine learning cosmic inflation
- Physical Review D
- http://link.aps.org/doi/10.1103/PhysRevD.108.043509
- # 20 - Resolving the Hubble tension with early dark energy
- Physical Review D
- http://link.aps.org/doi/10.1103/PhysRevD.108.043513
- # 21 - Sensitivity to supernovae average ${ν}_{x}$ temperature with neutral current interactions in DUNE
- Physical Review D
- http://link.aps.org/doi/10.1103/PhysRevD.108.043005
- # 22 - Waveform accuracy and systematic uncertainties in current gravitational wave observations
- Physical Review D
- http://link.aps.org/doi/10.1103/PhysRevD.108.044018
- # 23 - Fast Neutrino Flavor Conversions Can Help and Hinder Neutrino-Driven Explosions
- Physical Review Letters
- http://link.aps.org/doi/10.1103/PhysRevLett.131.061401
- # 24 - O, Ne, Mg, and Fe Abundances in Hot X-Ray-emitting Halos of Galaxy Clusters, Groups, and Giant Early-type Galaxies with XMM-Newton RGS Spectroscopy
- The Astrophysical Journal
- https://doi.org/10.3847/1538-4357/ace16a
- # 25 - Modeling Solids in Nuclear Astrophysics with Smoothed Particle Hydrodynamics
- The Astrophysical Journal Supplement
- https://doi.org/10.3847/1538-4365/acdc94
- # 26 - Study of the energy dependence of the $$^6$$ Li(p, $$alpha $$ ) $$^3$$ He reaction at energies of astrophysical interest
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.

