Effective Field Theory of Neutron Star Superfluidity

Details Effective Field Theory of Neutron Star Superfluidity Effective Field Theory of Neutron Star Superfluidity

1998-11-04

arxiv.org/abs/nucl-th/9811017v2

Physics

Nuclear Physics

Nuclear Theory

10 pages, 3 figures, LaTeX, improved discussion of medium effects

Scientific paper

We apply effective field theory and renormalization group techniques to the
problem of Cooper pair formation in neutron stars. Simple analytical
expressions for the $^1 S_0$ condensate are derived which are free of nuclear
potential model dependencies. The condensate is evaluated using phase shift
data from neutron-neutron scattering.

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