Effective Field Theory of Neutron Star Superfluidity

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dc.creatorHormuzdiar, James
dc.creatorHsu, Stephen
dc.date1998-11-04
dc.date1999-05-03
dc.date.accessioned2026-07-07T05:42:43Z
dc.date.available2026-07-07T05:42:43Z
dc.descriptionWe 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.
dc.description10 pages, 3 figures, LaTeX, improved discussion of medium effects
dc.identifierhttps://arxiv.org/abs/nucl-th/9811017
dc.identifierhttp://arxiv.org/abs/nucl-th/9811017
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/83036
dc.subjectNuclear Theory
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Phenomenology
dc.titleEffective Field Theory of Neutron Star Superfluidity
dc.typetext

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