Effective Field Theory of Neutron Star Superfluidity

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

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Nuclear Theory, Astrophysics, High Energy Physics - Phenomenology

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http://salesiana.dossiersoluciones.com/handle/123456789/83036

Consulte el texto completo en el siguiente enlace:

https://arxiv.org/abs/nucl-th/9811017
 http://arxiv.org/abs/nucl-th/9811017

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arXiv