Effective Field Theory of Neutron Star Superfluidity
Hormuzdiar, James · Hsu, Stephen
Original · EN
We apply effective field theory and renormalization group techniques to the problem of Cooper pair formation in neutron stars. Simple analytical expressions for the ¹ S₀ condensate are derived which are free of nuclear potential model dependencies. The condensate is evaluated using phase shift data from neutron-neutron scattering.
English translation
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