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1. Binary Neutron Star System

   Linked via "Tidal deformability"

   Tidal Effects and the Equation of State (EoS)
   While standard models treat the neutron stars as perfect geodesic travelers, the extreme pressures near the periastron cause significant tidal deformation, especially if the stars are not maximally rigid. Neutron stars possess an internal structure defined by their Equation of State (EoS), which describes the pressure-density relationship within the [degenerate matter](/entries…