Abstract
The relationships between the neutron-rich skin of a heavy nucleus such as 208Pb and the crust of a neutron star were studied. Relativistic effective field theories with a neutron-rich skin in 208Pb had lower liquid-to-solid transition density and a larger electron fraction. It was found that an exact measurement of the neutron radius in 208Pb via parity violating electron scattering has important implications for the neutron star structure.
| Original language | English |
|---|---|
| Pages (from-to) | 5647-5650 |
| Number of pages | 4 |
| Journal | Physical Review Letters |
| Volume | 86 |
| Issue number | 25 |
| DOIs | |
| State | Published - 18 Jun 2001 |
| Externally published | Yes |
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