Neutron Star Structure and the Equation of State
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...The EoS, i.e., the relation that links the star’s internal pressure to its density, can be mapped to a relationship between macroscopic observables of NSs such as their mass, radius, moment of inertia, and tidal deformability (Lattimer & Prakash 2001)....
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"Neutron Star Structure and the Equa..." refers background or methods in this paper
...Solid lines labelled “Inc”, “Buch” and “T VII” show predictions for an incompressible fluid, the solution of Buchdahl (1967), and the Tolman (1939) VII solution, respectively....
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...The third analytic solution (which we will refer to as “T VII”) was discovered by Tolman (1939) and corresponds to the case when the mass-energy density ρ varies quadratically, that is, ρ = ρc[1 − (r/R)2]....
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...The curves labelled “Inc”, “T VII”, “Buch” and “RP” are for an incompressible fluid, the Tolman (1939) VII solution, the Buchdahl (1967) solution, and an approximation of Ravenhall & Pethick (1994), respectively....
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