Langer et al. 1969

Langer, W.D., L.C. Rosen, J.M. Cohen, and A.G.W. Cameron, 1969: An equation of state at subnuclear densities. Astrophys. Space Sci., 5, 259-271, doi:10.1007/BF00649994.

An equation of state for cold matter above white dwarf densities is evaluated. The gas is considered to be a mixture of degenerate neutrons, protons and electrons combined with nuclei of one type (that is only one A and Z value). We derive the equilibrium equations for the mixture and calculate the number densities as well as the A and Z of the nucleus. Finally we calculate an equation of state, which smoothly goes over to that of a neutron, proton electron gas mixture at a density of 5×10¹³ g/cm³.

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Langer, W.D., Rosen, L.C., Cohen, J.M., and Cameron, A.G.W.: An equation of state at subnuclear densities, Astrophys. Space Sci., 5, 259-271, doi:10.1007/BF00649994, 1969.

Langer, W.D., L.C. Rosen, J.M. Cohen, and A.G.W. Cameron (1969), An equation of state at subnuclear densities, Astrophys. Space Sci., 5, 259-271, doi:10.1007/BF00649994.

Langer, W.D., L.C. Rosen, J.M. Cohen, and A.G.W. Cameron, 1969: An equation of state at subnuclear densities. Astrophys. Space Sci., 5, 259-271, doi:10.1007/BF00649994.

Langer, W.D., Rosen, L.C., Cohen, J.M., & Cameron, A.G.W. 1969, Astrophys. Space Sci., 5, 259, doi:10.1007/BF00649994.

Langer WD, Rosen LC, Cohen JM, Cameron AGW. An equation of state at subnuclear densities, Astrophys Space Sci 1969;5:259-271. doi:10.1007/BF00649994.

W.D. Langer, L.C. Rosen, J.M. Cohen, A.G.W. Cameron, Astrophys. Space Sci. 5, 259-271, doi:10.1007/BF00649994 (1969).