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We demonstrate in a general and analytic way how high-density information about the equation of state (EoS) of strongly interacting matter obtained using perturbative Quantum Chromodynamics (pQCD) constrains the same EoS at densities reachable in physical neutron stars.
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P. Ciarcelluti and F. Sandin, Have neutron stars a dark matter core?, Phys. Lett. B 695
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A. Del Popolo, M. Le Delliou, and M. Deliyergiyev, Neutron Stars and Dark Matter, Universe 6
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