Further explorations of Skyrme-Hartree-Fock-Bogoliubov mass formulas. XIII. The 2012 atomic mass evaluation and the symmetry coefficient

By S. Goriely, N. Chamel, J. Pearson. 2013

225 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Geophysics, Nuclear and High Energy Physics

View Paper: https://www.semanticscholar.org/paper/ae8608ef3548f95416fd4603c83457a80f99d786

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The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. A. Potekhin
2. S. Goriely
3. J. Pearson
4. N. Chamel
5. A. Fantina
6. José A. Pons
7. D. Page
8. A. Bauswein

In Geophysics

1. A. Potekhin

In Nuclear and High Energy Physics

1. A. Potekhin
2. S. Goriely
3. J. Pearson
4. G. Mart'inez-Pinedo
5. José A. Pons
6. K. Langanke
7. D. Page
8. Friedrich-Karl Thielemann

Citations in the corpus

• Unified equations of state for cold non-accreting neutron stars with Brussels-Montreal functionals. I. Role of symmetry energy (2018, methodology): “Very recently, gravitational-wave observations have been interpreted as indicating that the maximum mass of non-rotating neutron stars cannot exceed 2.16+0.17−0.15 solar masses (Rezzolla, Most & Weih 2018), supporting our assumption that the real EoS cannot be much stiffer than LS2.”