Abstract
The question of superfluidity in neutron matter is investigated in the framework of BCS-Bogoljubov-Theory. Solving the gap-equation for a semirealistic hard-core and a soft-core potential, a rapidly converging numerical method is developed. The results are applied to neutron star models.
| Original language | English |
|---|---|
| Pages (from-to) | 135-140 |
| Number of pages | 6 |
| Journal | Zeitschrift für Physik |
| Volume | 251 |
| Issue number | 2 |
| DOIs | |
| State | Published - Apr 1972 |
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