The AME2003 atomic mass evaluation . (II). Tables, graphs and references

By G. Audi, A. H. Wapstra, C. Thibault. 2003

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NEW EQUATIONS OF STATE IN SIMULATIONS OF CORE-COLLAPSE SUPERNOVAE (2011, methodology): “The HS EOS include up to 8000 nuclei, based on experimentally known masses of Audi et al. (2003) and different theoretical nuclear structure calculations.”
Double Beta Decay, Majorana Neutrinos, and Neutrino Mass (2007, methodology): “Precision measurements of the other Q-values would be useful because energy resolution is improving.”
Delayed outflows from black hole accretion tori following neutron star binary coalescence (2013, background): “…energy becoming eint = eint,0 − Qα mα Xα, (12) where eint,0 is the specific internal energy provided by the Helmholtz EOS, Xα is the mass fraction of alpha particles, mα is the mass of an alpha particle, and Qα ≃ 28.3 MeV is the nuclear binding energy of an alpha particle (e.g., Audi et al. 2003).”
Detecting non-relativistic cosmic neutrinos by capture on tritium: phenomenology and physics potential (2014, background): “ exercise, since Eq. (A.9) depends only on the neutrino mass, we feel that it is illustrative to the reader. The nuclear masses of tritium and helium-3 are not provided directly in the AME2003 tables [92]. Instead they must be derived from the atomic masses, which are M 3H(atomic) = 3016049:2777(25)”
ENDF/B-VII.1 Nuclear Data for Science and Technology: Cross Sections, Covariances, Fission Product Yields and Decay Data (2011, methodology): “0 makes use of the 2003 Audi mass evaluation [263].”