Figure 64: Neutrino emissivity from the Cooper pair formation mechanism, calculated for strong
(uniform) neutron superfluidity with the maximum critical temperature (a
model from [231]). For comparison, from two most efficient other mechanisms, plasmon decay
and electron Bremsstrahlung, are also plotted. The smooth composition ground-state crust model of
Kaminker et al. [231] is used; it predicts a specific in the inner crust. This crust model is
described in detail in Appendix B.2 of Haensel et al. [184]). From [428].
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