Neutron star structure with modern nucleonic three-body forces
By Z. H. Li, H. Schulze. 2008
136 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/14637bdc9b35d3b2580cd630ed7117f8b27d83bf
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In Astronomy and Astrophysics
In Nuclear and High Energy Physics
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): “The points APR refer to the calculations of Akmal et al. (1998) labelled as ‘A18 + δ v + UIX∗’, while the points LS2 refer to those labelled as ‘V18’ in Li & Schulze (2008). given the much softer EoS of NeuM to which it has been fitted.”
- Unified equation of state for neutron stars on a microscopic basis (2015, methodology): “Recently the connection between two-body and three-body forces within the meson-nucleon theory of the nuclear interaction has been extensively discussed and developed in (Grangé et al. 1989; Zuo et al. 2002; Li & Schulze 2008; Li et al. 2008).”
- The Nuclear Symmetry Energy (2016, methodology): “[267, 268] with the Bonn B two-body interaction and consistent (’microscopic’) three-body force.”