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Nuclear Properties for Astrophysical Applications

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abstract

We tabulate the ground-state odd-proton and odd-neutron spins and parities, proton and neutron pairing gaps, binding energy, one- and two-neutron separation energies, quantities related to beta-delayed one- and two-neutron emission probabilities, beta-decay energy release and half-life with respect to Gamow-Teller decay, one- and two-proton separation energies, and alpha-decay energy release and half-life for 8979 nuclei ranging from oxygen-16 to Z = 136, A = 339 and extending from the proton drip line to the neutron drip line. Single-particle level diagrams and other quantities are also presented in graphical form. The starting point of our present work is a study of nuclear ground-state masses and deformations based on the finite-range droplet model and folded-Yukawa single-particle potential published in a previous issue of Atomic Data and Nuclear Data Tables. The beta-delayed neutron-emission probabilities and Gamow-Teller beta-decay rates are obtained from a quasi-particle random-phase approximation with single-particle levels and wave functions at the calculated nuclear ground-state shapes as input quantities.

fields

hep-ph 1

years

2026 1

verdicts

CONDITIONAL 1

representative citing papers

Scalar baryons in neutron stars

hep-ph · 2026-08-10 · conditional · novelty 6.0

Scalar baryons made inside neutron stars require non-perturbatively large repulsive self-couplings, lambda_4 greater than 1000, to permit two-solar-mass stars, and attractive self-interactions make even scalars heavier than the core chemical potential testable.

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  • Scalar baryons in neutron stars hep-ph · 2026-08-10 · conditional · none · ref 41 · internal anchor

    Scalar baryons made inside neutron stars require non-perturbatively large repulsive self-couplings, lambda_4 greater than 1000, to permit two-solar-mass stars, and attractive self-interactions make even scalars heavier than the core chemical potential testable.