The Ame2012 atomic mass evaluation
By G. Audi, Mei Wang, A. H. Wapstra, F. Kondev, M. Maccormick, X. Xu, B. Pfeiffer. 2003
378 citations recorded by the source corpus.
Subfields: Inorganic Chemistry, Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/01fa68dad4a3ba7b1e8c23ade700ec09ad9ada92
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In Inorganic Chemistry
In Nuclear and High Energy Physics
- Alexey Boyarsky
- H. Hammer
- Oleg Ruchayskiy
- Thierry Lasserre
- Marco Drewes
- Susanne Mertens
- C. Ji
- D. Phillips
Citations in the corpus
- Sterile neutrino Dark Matter (2018, background): “∆ are the usual tabulated mass excess and Q β denotes the tabulated Q-value assuming mν = 0 [511].”
- The In-Medium Similarity Renormalization Group: A novel ab initio method for nuclei (2015, neutral): “Black bars indicate experimental data [29, 124].”
- Nuclear equation of state from ground and collective excited state properties of nuclei (2018, result): “a 21 fixed from other considerations than fit to masses; b With respect to AME2003[149]; c Estimated properties[137]; d With respect to AME2012[150]; e Some of them fixed manually [62]; f Only even-even nuclei with N,Z > 8 have been considered and compared with AME2003[149]; g Only even-even nuclei ”
- Mean field and beyond description of nuclear structure with the Gogny force: a review (2018, methodology): “[313]) and (a) HFB; and, (b) GCM total energies calculated with an axial SCCM method (including PNAMP and axial quadrupole shape mixing) with the D1M parametrization.”
- The impact of individual nuclear properties on $r$-process nucleosynthesis (2015, methodology): “As much as 53% new data exists between the latest evaluation (AME2012) and the previous evaluation (AME2003) [163] most of which is from measurements on neutron-rich nuclei, thus providing more experimental input for r-process simulations.”
- Effective field theory description of halo nuclei (2017, methodology): “The one-neutron separation energies S1n of (11)Be and (15)C are determined in the atomic mass evaluation [78, 79]; while the first excitation energies of the cores E∗ c are obtained from the nuclear data evaluation [81, 82] (see Table 1).”
- A White Paper on keV sterile neutrino Dark Matter (2016, neutral): “016) keV published by the Atomic Mass Evaluation edited in 2012 [946].”