Table 2
Properties of nuclear matter at saturation predicted by the EoS of this work in comparison with the empirical ranges (Newton et al. 2013; Steiner et al. 2010; Lattimer & Lim 2013; Hebeler et al. 2013; Chen et al. 2010; Tsang et al. 2012; Viñas et al. 2014).
| E / A | n 0 | K | Esym(n0) | L | |
| (MeV) | (fm-3) | (MeV) | (MeV) | (MeV) | |
|
|
|||||
| This work | −16.00 | 0.160 | 213.75 | 31.92 | 52.96 |
| Ska (Lattimer & Swesty 1991) | −16.00 | 0.155 | 263.18 | 32.91 | 74.62 |
| SLy4 (Chabanat et al. 1998) | −15.97 | 0.160 | 229.93 | 32.00 | 45.96 |
| BSk21 (Goriely et al. 2010) | −16.05 | 0.158 | 245.8 | 30.0 | 46.6 |
| TM1 (Shen et al. 1998a) | −16.26 | 0.145 | 281.14 | 36.89 | 110.79 |
| Empirical | −16.0 ± 0.1 | 0.16 ± 0.01 | 220 ± 30 | 31 ± 2 | ~ 60 ± 25 |
Notes. From left to right, the quantities are the energy per particle, density, incompressibility, symmetry energy, and slope parameter of the symmetry energy: 
. The effective nucleon mass in the present model is m∗ = m (Baldo et al. 2008b). The nuclear matter properties of other EoSs that will be considered in the sections of results are also shown.
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