| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 9851389 | Nuclear Physics A | 2005 | 11 Pages |
Abstract
The different superfluid states that can occur inside neutron stars are reviewed, both in the crust region and in the core. The role of correlations in determining the values of the pairing gaps is emphasized. Comparison is made on one hand with pairing in nuclear structure calculations in ordinary (terrestrial) nuclei, and on the other hand with hints from phenomenological analysis of observational data.
Related Topics
Physical Sciences and Engineering
Physics and Astronomy
Nuclear and High Energy Physics
Authors
M. Baldo, E.E. Saperstein, S.V. Tolokonnikov,