Table 5.
Posterior estimations of the fractional thickness Rpasta/Rcrust, moment of inertia Ipasta/Icrust, and mass mpasta/mcrust of the pasta layer, normalised to the corresponding crustal quantity.
| n ≥ 0.02 fm−3 | n ≥ 0.1 fm−3 | |
|---|---|---|
| Rpasta/Rcrust | 0.128 ± 0.047 | 0.104 ± 0.063 |
| Ipasta/Icrust | 0.480 ± 0.137 | 0.411 ± 0.212 |
| mpasta/mcrust | 0.485 ± 0.138 | 0.415 ± 0.214 |
Notes. Values in the table are given for a neutron star with a mass M = Mmax. Both low-density EFT filters and high-density filters are applied. The chiral EFT filter is applied from either n = 0.02 fm−3 (left column) or n = 0.1 fm−3 (right column). The uncertainties indicate 1σ deviations.
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