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Superfluid properties of the inner crust of neutron stars
KTH, Superseded Departments, Physics.
KTH, Superseded Departments, Physics.
2004 (English)In: Physical Review C. Nuclear Physics, ISSN 0556-2813, E-ISSN 1089-490X, Vol. 69, no 4, 045802- p.Article in journal (Refereed) Published
Abstract [en]

Superfluid properties of the inner crust matter of neutron stars, formed by nuclear clusters immersed in a dilute neutron gas, are analyzed in a self-consistent Hartree-Fock-Bogoliubov approach. The calculations are performed with two pairing forces, fixed so as to obtain in infinite nuclear matter the pairing gaps provided by the Gogny force or by induced interactions. It is shown that the nuclear clusters can either suppress or enhance the pairing correlations inside the inner crust matter, depending on the density of the surrounding neutrons. The profile of the pairing field in the inner crust is rather similar for both pairing forces, but the values of the pairing gaps are drastically reduced for the force which simulates the polarization effects in infinite neutron matter.

Place, publisher, year, edition, pages
2004. Vol. 69, no 4, 045802- p.
National Category
Atom and Molecular Physics and Optics
Identifiers
URN: urn:nbn:se:kth:diva-45012DOI: 10.1103/PhysRevC.69.045802ISI: 000221427500058Scopus ID: 2-s2.0-3042547281OAI: oai:DiVA.org:kth-45012DiVA: diva2:451765
Note
C 20111027Available from: 2011-10-27 Created: 2011-10-26 Last updated: 2017-12-08Bibliographically approved

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