Abstract
The calculated energy-density relation of a well-defined superdense neutron liquid model is compared with other microscopic calculations. All techniques except one give consistent results. This finding has an important bearing on the existence of solid cores in neutron stars.
| Original language | English |
|---|---|
| Pages (from-to) | 371-373 |
| Number of pages | 3 |
| Journal | Physical Review D |
| Volume | 10 |
| Issue number | 2 |
| DOIs | |
| Publication status | Published - 1974 |
| Externally published | Yes |
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