JINA - Virtual Journal of Nuclear Astrophysics, 2 February 2024
Volume 22, Issue 5 (43 Articles)
- # 1 - 3D code for MAgneto-Thermal evolution in Isolated Neutron Stars, MATINS: thermal evolution and lightcurves. (arXiv:2401.15711v1 [astro-ph.HE])
- # 2 - A $lambda$ 3 mm line survey towards the circumstellar envelope of the carbon-rich AGB star IRC+10216 (CW Leo). (arXiv:2401.16089v1 [astro-ph.SR])
- # 3 - A Channel to Form Fast-spinning Black Hole-Neutron Star Binary Mergers as Multimessenger Sources. II. Accretion-induced Spin-up
- # 4 - A Theory for Neutron Star and Black Hole Kicks and Induced Spins
- # 5 - Collapsing massive stars and their EM transients. (arXiv:2401.17156v1 [astro-ph.HE])
- # 6 - Ejecta-circumstellar medium interaction in high-density environment to kilonova emission: Application for GRB 191019A. (arXiv:2401.14418v1 [astro-ph.HE])
- # 7 - Hyperonic uncertainties in neutron stars, mergers and supernovae
- # 8 - Impact of Hot Inner Crust on The Properties of Hot Compact Stars. (arXiv:2401.16957v1 [nucl-th])
- # 9 - Impact of the molecular resonances on the 12C+12C fusion reaction rate
- # 10 - JWST NIRSpec+MIRI Observations of the nearby Type IIP supernova 2022acko. (arXiv:2401.14474v1 [astro-ph.HE])
- # 11 - Neutron star kick driven by asymmetric fast-neutrino flavor conversion. (arXiv:2401.15180v1 [astro-ph.HE])
- # 12 - Origin of $^{60}$Fe nuclei in cosmic rays: the contribution of local OB associations
- # 13 - Prospects for detecting neutron star-white dwarf mergers with decihertz gravitational-wave observatories
- # 14 - The 2024 BBN baryon abundance update. (arXiv:2401.15054v1 [astro-ph.CO])
- # 15 - The enigmatic double-peaked stripped-envelope SN 2023aew
- # 16 - The Guided Moments formalism: a new efficient full-neutrino treatment for astrophysical simulations
- # 17 - The metamorphosis of the Type Ib SN 2019yvr: late-time interaction. (arXiv:2401.15052v1 [astro-ph.HE])
- # 18 - A comparison of the neutron detection efficiency and response characteristics of two pixelated PSD-capable organic scintillator detectors with different photo-detection readout methods
- # 19 - Analysis methodology of neutron time-of-flight spectra based on Bayesian unfolding and accurate Monte Carlo simulations
- # 20 - Clarifying the Radiative Decay of the Hoyle State with Charged-Particle Spectroscopy
- # 21 - Direct high-precision measurement of the mass difference of $^{77}$As-$^{77}$Se related to neutrino mass determination. (arXiv:2401.15242v1 [nucl-ex])
- # 22 - Exploring the compactness of $alpha$ cluster in the $^{16}$O nuclei with relativistic $^{16}$O+$^{16}$O collisions. (arXiv:2401.15723v1 [nucl-th])
- # 23 - Understanding the total width of the $3_{1}^{-}$ state in $mathrm{^{12}C}$
- # 24 - Neutron-star Measurements in the Multi-messenger Era. (arXiv:2401.14930v1 [astro-ph.HE])
- # 25 - Nuclear ground-state properties probed by the relativistic Hartree–Bogoliubov approach
- # 26 - General relativistic moving-mesh hydrodynamic simulations with arepo and applications to neutron star mergers
- Monthly Notices of the Royal Astronomical Society - Volume: 528, Issue: 2
- https://academic.oup.com/mnras/article/528/2/1906/7515304?rss=1
- # 27 - Oxygen abundance of γ Vel from [O iii] 88 μm Herschel/PACS spectroscopy
- Monthly Notices of the Royal Astronomical Society - Volume: 528, Issue: 2
- https://academic.oup.com/mnras/article/528/2/2026/7529211?rss=1
- # 28 - The preliminary statistical analysis of LAMOST DR10 low resolution AFGK stars based on different metal abundances
- # 29 - High count rate gamma ray pile-up correction method of NaI(Tl) detector based on deconvolution method
- # 30 - Cross section measurements of 27Al(γ, x)24Na reactions as monitors for laser-driven bremsstrahlung γ-ray
- # 31 - Determining the $^{9}mathrm{Be}(n,γ)^{10}mathrm{Be}$ integral cross section at fission neutron energies
- Physical Review C
- http://link.aps.org/doi/10.1103/PhysRevC.109.014625
- # 32 - Far-from-equilibrium bulk-viscous transport coefficients in neutron star mergers
- Physical Review C
- http://link.aps.org/doi/10.1103/PhysRevC.109.015805
- # 33 - Understanding the total width of the ${3}_{1}^{−}$ state in $^{12}mathrm{C}$
- Physical Review C
- http://link.aps.org/doi/10.1103/PhysRevC.109.015806
- # 34 - New model comparison for semi-inclusive charged-current electron and muon neutrino scattering by $^{40}mathrm{Ar}$ in the energy range of the MicroBooNE experiment
- Physical Review D
- http://link.aps.org/doi/10.1103/PhysRevD.109.013004
- # 35 - Massive neutron stars as mass gap candidates: Exploring equation of state and magnetic field
- Physical Review D
- http://link.aps.org/doi/10.1103/PhysRevD.109.023027
- # 36 - New and robust gravitational-waveform model for high-mass-ratio binary neutron star systems with dynamical tidal effects
- Physical Review D
- http://link.aps.org/doi/10.1103/PhysRevD.109.024062
- # 37 - Shear oscillations in neutron stars and the nuclear symmetry energy
- Physical Review D
- http://link.aps.org/doi/10.1103/PhysRevD.109.023030
- # 38 - Thallium-208: A Beacon of <i>In Situ</i> Neutron Capture Nucleosynthesis
- Physical Review Letters
- http://link.aps.org/doi/10.1103/PhysRevLett.132.052701
- # 39 - Does or Did the Supernova Remnant Cassiopeia A Operate as a PeVatron?
- The Astrophysical Journal Letters
- https://doi.org/10.3847/2041-8213/ad1d62
- # 40 - Evolution and Final Fate of Solar Metallicity Stars in the Mass Range 7–15 M⊙. I. The Transition from Asymptotic Giant Branch to Super-AGB Stars, Electron Capture, and Core-collapse Supernova Progenitors
- The Astrophysical Journal Supplement
- https://doi.org/10.3847/1538-4365/ad12c1
- # 41 - The Presolar Grain Database. I. Silicon Carbide
- The Astrophysical Journal Supplement
- https://doi.org/10.3847/1538-4365/ad1102
- # 42 - Constraining equations of state for massive neutron star within relativistic mean field models
- # 43 - High-resolution cross section measurements for neutron interactions on $$^{89}$$ Y with incident neutron energies up to 95 keV
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.

