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Equation of State Sub-Library: Version 0.910
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The class cold_nstar computes the structure of zero-temperature spherically-symmetric neutron stars. It uses tov_solve to compute the structure, given a hadronic equation of state (of type hadronic_eos). It also computes the adiabatic index, the speed of sound, and determines the possibility of the direct Urca process as a function of density or radius.
This class is still experimental.
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