JINA - Virtual Journal of Nuclear Astrophysics, 29 July 2022
Volume 20, Issue 30 (27 Articles)
- # 1 - Evidence for Extended Hydrogen-Poor CSM in the Three-Peaked Light Curve of Stripped Envelope Ib Supernova. (arXiv:2207.07146v2 [astro-ph.HE] UPDATED)
- # 2 - Gravitational Waves from Strange Star Core-Crust Oscillation. (arXiv:2207.12053v1 [astro-ph.HE])
- # 3 - Potential signature of Population III pair-instability supernova ejecta in the BLR gas of the most distant quasar at z = 7.54. (arXiv:2207.11909v1 [astro-ph.GA])
- # 4 - Reaching percolation and conformal limits in neutron stars. (arXiv:2207.13059v1 [nucl-th])
- # 5 - The chemical enrichment in the early Universe as probed by JWST via direct metallicity measurements at z~8. (arXiv:2207.12375v1 [astro-ph.GA])
- # 6 - The origins of Calcium-rich supernovae from disruptions of CO white-dwarfs by hybrid He-CO white-dwarfs. (arXiv:2207.13110v1 [astro-ph.HE])
- # 7 - The Zwicky Transient Facility phase I sample of hydrogen-rich superluminous supernovae without strong narrow emission lines. (arXiv:2207.12059v1 [astro-ph.HE])
- # 8 - An Improved Method for Coupling Hydrodynamics with Astrophysical Reaction Networks. (arXiv:2206.01285v2 [astro-ph.IM] UPDATED)
- # 9 - Inner crust equations of state for CompOSE. (arXiv:2207.14153v1 [nucl-th])
- # 10 - Microscopic nuclear equation of state at finite temperature and stellar stability. (arXiv:2207.12146v1 [nucl-th])
- # 11 - Plausible presence of quark matter in neutron stars with masses above $0.97M_{rm TOV}$. (arXiv:2207.13613v1 [astro-ph.HE])
- # 12 - Temperature Effects on Core g-modes of Neutron Stars. (arXiv:2207.13488v1 [astro-ph.HE])
- # 13 - Unveiling the dynamics of nucleosynthesis in relativistic heavy-ion collisions. (arXiv:2207.12532v1 [nucl-th])
- # 14 - A force explosion condition for spherically symmetric core-collapse supernovae
- Monthly Notices of the Royal Astronomical Society - Volume: 515, Issue: 2
- https://academic.oup.com/mnras/article/515/2/1610/6623675?rss=1
- # 15 - For how long are particles accelerated in shells of recurrent novae?
- Monthly Notices of the Royal Astronomical Society - Volume: 515, Issue: 2
- https://academic.oup.com/mnras/article/515/2/1644/6649985?rss=1
- # 16 - High-energy γ-ray detection of supernova remnants in the Large Magellanic Cloud
- Monthly Notices of the Royal Astronomical Society - Volume: 515, Issue: 2
- https://academic.oup.com/mnras/article/515/2/1676/6632979?rss=1
- # 17 - A mid-infrared dream come true
- Nature Astronomy
- https://www.nature.com/articles/s41550-022-01736-6
- # 18 - Indirect measurement of the $(n,γ)^{127}mathrm{Sb}$ cross section
- Physical Review C
- http://link.aps.org/doi/10.1103/PhysRevC.106.015804
- # 19 - Pasta properties of the neutron star within effective relativistic mean-field model
- Physical Review D
- http://link.aps.org/doi/10.1103/PhysRevD.106.023031
- # 20 - Radio bursts from ‘zombie’ black holes excite astronomers
- # 21 - Connecting the Light Curves of Type IIP Supernovae to the Properties of Their Progenitors
- The Astrophysical Journal
- https://doi.org/10.3847/1538-4357/ac77f3
- # 22 - Dust Grain Growth and Dusty Supernovae in Low-metallicity Molecular Clouds
- The Astrophysical Journal
- https://doi.org/10.3847/1538-4357/ac77fe
- # 23 - Heliospheric Compression Due to Recent Nearby Supernova Explosions
- The Astrophysical Journal
- https://doi.org/10.3847/1538-4357/ac77f1
- # 24 - Implications of NICER for Neutron Star Matter: The QHC21 Equation of State
- The Astrophysical Journal
- https://doi.org/10.3847/1538-4357/ac7876
- # 25 - Neutrino Emissivities as a Probe of the Internal Magnetic Fields of White Dwarfs
- The Astrophysical Journal
- https://doi.org/10.3847/1538-4357/ac7874
- # 26 - Radio Detection of an Elusive Millisecond Pulsar in the Globular Cluster NGC 6397
- The Astrophysical Journal Letters
- https://doi.org/10.3847/2041-8213/ac81c3
- # 27 - Delta-resonances and hyperons in proto-neutron stars and merger remnants
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.

