Inman 1965

Inman, C.I., 1965: Baryon star models. Astrophys. J., 141, 187-194, doi:10.1086/148101.

We consider, in the framework of general relativity, large masses consisting of identical baryons (whose mass is taken to be that of the neutron). Four assumptions are made as to their interactions, leading to four equations of states, and for each the masses and radii of a number of configurations are calculated for various values of the central number density. The relations of the mass to a parameter t₀ (= 4 sinh^-1 [ℏ/m_Bc(3π²n₀)^1/3], where n₀ is the central number density) for each of the four equations of state are strikingly similar.

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Inman, C.I.: Baryon star models, Astrophys. J., 141, 187-194, doi:10.1086/148101, 1965.

Inman, C.I. (1965), Baryon star models, Astrophys. J., 141, 187-194, doi:10.1086/148101.

Inman, C.I., 1965: Baryon star models. Astrophys. J., 141, 187-194, doi:10.1086/148101.

Inman, C.I. 1965, Astrophys. J., 141, 187, doi:10.1086/148101.

Inman CI. Baryon star models, Astrophys J 1965;141:187-194. doi:10.1086/148101.

C.I. Inman, Astrophys. J. 141, 187-194, doi:10.1086/148101 (1965).