Erratum: Proto-neutron star structure within an extended lowest-order constrained variational method at finite temperature [Phys. Rev. C 92 , 035806 (2015)]
Author:
Publisher
American Physical Society (APS)
Link
http://harvest.aps.org/v2/journals/articles/10.1103/PhysRevC.97.049904/fulltext
Reference5 articles.
1. 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)]
2. Effects of three-body forces on the maximum mass of neutron stars in the lowest-order constrained variational formalism
3. Nuclear liquid-gas phase transition
4. The maximum and minimum mass of protoneutron stars in the Brueckner theory
5. Properties of a protoneutron star in effective field theory
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1. Proto-neutron stars in the Thomas-Fermi theory;Nuclear Physics A;2019-06
2. Thomas–Fermi approximation for β-stable nuclear matter in the Landau Fermi-liquid theory;Nuclear Physics A;2018-12
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