H. R. Moshfegh

TL;DR: In this article, the two-body correlation functions, obtained in a lowest-order constrained variational calculation for hot nuclear and neutron matter, with the Reid potential and the explicit inclusion of, are state averaged and used to calculate the three-body cluster energy.

TL;DR: In this article, the authors considered the problem of the hyperon puzzle and its suggested solution by quark deconfinement within the two-phase approach to hybrid compact stars with recently obtained hadronic and quark matter equations of state.

TL;DR: In this article, the authors used the lowest-order constrained variational calculations to calculate the equation of state of nuclear stable matter at finite temperature, where the electron and muon are treated relativistically at given temperature and density, in order to neutralize the fluid electrically and stabilize it against decay.

TL;DR: In this article, it is shown that the LOCV normalization constraint plays a major role in the convergence of the cluster expansion and the result of LOCV calculation can be as good as more sophisticated approaches which go beyond lowest order.

TL;DR: In this paper, the equation of state of neutron star matter is calculated within the lowest order constrained variational (LOCV) method using different two-body interactions and an Urbana type three-body force.