The Neutron star properties are calculated with the various interactions such as charge dependent Reid potential (Reid93) as well as Reid68 and AV₁₈ interactions within the lowest order constrained variational method (LOCV). It is shown that at low densities, neutron star masses exhibit a minimum (\simeq 0.1M_\odot ) and a maximum mass between 1.4 M_\odot and 1.9 M_\odot which is strongly dependent on the equation of state.

PACS numbers: 21.65.+f, 26.60.+c, 97.60.Jd