JINA - Virtual Journal of Nuclear Astrophysics, 14 February 2025
Volume 23, Issue 7 (29 Articles)
- # 1 - Building Neutron Stars with the MUSES Calculation Engine
- # 2 - Modelling the impact of circumbinary disk accretion on post-AGB binary evolution and surface chemistry
- # 3 - Observational and Theoretical Constraints on First-Order Phase Transitions in Neutron Stars
- # 4 - Observations and Radiative Transfer Simulations of the Carbon-rich AGB star V Oph with VLTI/MATISSE
- # 5 - Successful $nu p$-process in neutrino-driven outflows in core-collapse supernovae
- # 6 - The Equation of State of Neutron Stars: Theoretical Models, Observational Constraints, and Future Perspectives
- # 7 - The Type Ia Supernova and AGB-Regulated Interstellar Medium of Massive Galaxies
- # 8 - Directly probing existence of $alpha$-cluster structure in $^{20}$Ne by relativistic heavy-ion collisions
- # 9 - Fixing effective range parameters in elastic $alpha$-$^{12}$C scattering: an impact on resonant $2_4^+$ state of $^{16}$O and $S_{E2}$ factor of $^{12}$C($alpha$,$gamma$)$^{16}$O
- # 10 - High-precision direct decay energy measurements of the electron-capture decay of $^{97}$Tc
- # 11 - Refined topology of the N = 20 island of inversion with high precision mass measurements of $^{31-33}$Na and $^{31-35}$Mg
- # 12 - $alpha+alpha+{}^{3}$He cluster structure in ${}^{11}$C
- # 13 - Bose-Einstein condensation of five $alpha$ clusters in $^{20}$Ne and supersolidity
- # 14 - The impact of mass uncertainties on r-process nucleosynthesis in neutron star mergers
- Astronomy & Astrophysics
- https://www.aanda.org/10.1051/0004-6361/202451991
- # 15 - bpass stellar evolution models incorporating α-enhanced composition – I. Single star models from 0.1 to 316 M⊙
- Monthly Notices of the Royal Astronomical Society - Volume: 537, Issue: 3
- https://academic.oup.com/mnras/article/537/3/2433/7989468?rss=1
- # 16 - Measurement of -particles to determine cross sections relevant to the weak r-process
- # 17 - Re-evaluation of the 26Si(p,γ)27P astrophysical reaction rate
- # 18 - $α+α+^{3}mathrm{He}$ cluster structure in $^{11}mathrm{C}$
- Physical Review C
- http://link.aps.org/doi/10.1103/PhysRevC.111.024309
- # 19 - Constraining calculations of $^{239}mathrm{Pu}(n,γ)$ cross sections with multistep cascade $γ$-ray spectra measured at the DANCE facility
- Physical Review C
- http://link.aps.org/doi/10.1103/PhysRevC.111.024610
- # 20 - Measurement of the $^{175}mathrm{Hf}$ half-life
- Physical Review C
- http://link.aps.org/doi/10.1103/PhysRevC.111.024308
- # 21 - Photonuclear reactions on stable isotopes of molybdenum at bremsstrahlung endpoint energies of 10–23 MeV
- Physical Review C
- http://link.aps.org/doi/10.1103/PhysRevC.111.024604
- # 22 - Strength measurements of the ${E}_{mathrm{R}}^{mathrm{lab}}=647$ and 1842 keV resonances in the $^{40}mathrm{Ca}(p,γ)^{41}mathrm{Sc}$ reaction and their relevance in novae nucleosynthesis
- Physical Review C
- http://link.aps.org/doi/10.1103/PhysRevC.111.025804
- # 23 - Barrow cosmology and big-bang nucleosynthesis
- Physical Review D
- http://link.aps.org/doi/10.1103/PhysRevD.111.043518
- # 24 - Big bang nucleosynthesis constraints on the energy-momentum squared gravity: The ${mathbb{T}}^{2}$ model
- Physical Review D
- http://link.aps.org/doi/10.1103/PhysRevD.111.043525
- # 25 - Refined Topology of the $N=20$ Island of Inversion with High Precision Mass Measurements of $^{31−33}mathrm{Na}$ and $^{31−35}mathrm{Mg}$
- Physical Review Letters
- http://link.aps.org/doi/10.1103/PhysRevLett.134.052503
- # 26 - Direct Mass Measurements of Neutron-Rich Zinc and Gallium Isotopes: An Investigation of the Formation of the First $r$-Process Peak
- Physical Review Letters
- http://link.aps.org/doi/10.1103/PhysRevLett.134.062701
- # 27 - Neutron sources for large scale user facilities: The potential of high current accelerator-driven neutron sources
- # 28 - Cross section and isomeric ratio measurements along with covariance analysis for the (n,2n) reactions on 120,130Te
- # 29 - Impact of the nuclear equation of state on the formation of twin stars
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.

