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arXiv · nucl-th/9811017

Effective Field Theory of Neutron Star Superfluidity

James Hormuzdiar·Stephen Hsu
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Abstract

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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James Hormuzdiar, Stephen Hsu. 1999-05-03. Effective Field Theory of Neutron Star Superfluidity. https://arxiv.org/abs/nucl-th/9811017

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