JINA - Virtual Journal of Nuclear Astrophysics, 11 September 2026
Volume 24, Issue 37 (15 Articles)
- # 1 - Constraining the Equation of State of Neutron Stars with third-generation Gravitational Wave detectors
- # 2 - Free Neutron Decay in Kilonova Ejecta: X-ray/UV Flashes with Non-Thermal Effects
- # 3 - Supernova microlensing as a probe of ultracompact minihalos and primordial cosmology
- # 4 - Supernovae Unite: Host-Galaxy Mass Measurements of Type Ia Supernovae and Their Impact on Cosmology
- # 5 - Precision $beta$-delayed charged-particle emission spectroscopy at FRIB: Proof of principle with the $beta$-decay of $^{25}mathrm{Si}$
- # 6 - Astrophysical $S$-factors in primordial nucleosynthesis
- # 7 - How AI is changing PhD programmes: join our free webinar
- # 8 - The Kelvin scale’s creator William Thomson made many scientific advances
- # 9 - Machine- and deep-learning regression for equations of state of compact objects
- Physical Review C
- http://link.aps.org/doi/10.1103/v98s-bh7z
- # 10 - Neutron star matter with hyperons: Bayesian comparison of nucleonic and SU(6)/SU(3) hyperonic models
- Physical Review C
- http://link.aps.org/doi/10.1103/6jzv-s7dq
- # 11 - Multimessenger search strategy for composite dark matter with white dwarf data and gravitational wave detectors
- Physical Review D
- http://link.aps.org/doi/10.1103/8snb-pfbr
- # 12 - Can wormholes have vanishing Love numbers?
- Physical Review D
- http://link.aps.org/doi/10.1103/z8hm-fvx3
- # 13 - Dynamical tidal Love numbers of black holes under generic perturbations: Connecting black hole perturbation theory with effective field theory
- Physical Review D
- http://link.aps.org/doi/10.1103/lfq4-49k1
- # 14 - Surface gravity wave on a neutron star ocean trapped around a magnetic pole
- Physical Review D
- http://link.aps.org/doi/10.1103/1x62-nw3p
- # 15 - Astrophysics Equation of State Inference with Bayesian Chiral Effective Field Theory Uncertainties
- The Astrophysical Journal
- https://iopscience.iop.org/article/10.3847/1538-4357/ae92f9
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.

