Erratum: Effects of three-body forces on the maximum mass of neutron stars in the lowest-order constrained variational formalism [Phys. Rev. C 91, 054320 (2015)]
S. Goudarzi and H. R. Moshfegh
Phys. Rev. C 96, 049902 – Published 26 October 2017
(a) The EOS of symmetric nuclear matter for different two-body potentials supplemented by the TBF. (b) The EOS of asymmetric nuclear matter for a number of asymmetry parameter 's as well as -stable matter using the potential.
Density dependence of the nuclear symmetry energy obtained by the LOCV approach as well as some other many-body techniques, such as the BHF (with the AV18, the AV18 + TBF, the Bonn B, and the Bonn B + TBF) [44, 45], the BHF (the AV18 + micro-TBF) [7], the variational (the AV18, ) [11], and the DBHF [46, 47].
(a) Proton, electron, and muon fractions for -stable matter against baryon density with and without the TBF using the AV18 potential. (b) Comparison of the proton fraction obtained in the present paper (the black solid curve) with the results of the AV18 + UIX (APR) [11], the AV14 + UVII [40], the UV14 + UVII [40], the UV14 + TNI [40], the U14-DDI [43], AV18 + UIX [Zhou-Burgio-Lombardo-Schulze (ZBLS)] [7], and the AV18 + micro-TBF [7].