Using the Gibbs construction for the phase transition in the CCT model, the authors find a mixed-phase region extending down to the inner crust, giving neutron stars a thick, massive crust.
Laskos-Patkos, G
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Does HESS J1731-347 have a thick crust ?
Using the Gibbs construction for the phase transition in the CCT model, the authors find a mixed-phase region extending down to the inner crust, giving neutron stars a thick, massive crust.