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Nuclear Properties for Astrophysical Applications

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arxiv nucl-th/9601043 v1 pith:ZIMRVCDV submitted 1996-01-27 nucl-th

classification nucl-th
keywords nuclearenergyground-stateone-quantitiessingle-particlebeta-decaybeta-delayed
verification ladder T0 review T1 audit T2 compute T3 formal

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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.

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    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 heavie...

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